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Title: Detailed Study Of The Fermi Surfaces Of The Type-ii Dirac Semimetallic Candidates Xte2 (x=pd,pt).
Creator: Zheng, W., Schonemann, R., Aryal, N., Zhou, Q., Rhodes, D., Chiu, Y.-C., Chen, K.-W., Kampert, E., Foerster, T., Martin, T. J., McCandless, G. T., Chan, J. Y., Manousakis, E.,...
Show moreZheng, W., Schonemann, R., Aryal, N., Zhou, Q., Rhodes, D., Chiu, Y.-C., Chen, K.-W., Kampert, E., Foerster, T., Martin, T. J., McCandless, G. T., Chan, J. Y., Manousakis, E., Balicas, L.
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Abstract/Description: We present a detailed quantum oscillatory study on the Dirac type-II semimetallic candidates PdTe2 and PtTe2 via the temperature and the angular dependence of the de Haas-van Alphen and Shubnikov-de Haas effects. In high-quality single crystals of both compounds, i.e., displaying carrier mobilities between 10(3) and 10(4) cm(2)/Vs, we observed a large nonsaturating magnetoresistivity which in PtTe2 at a temperature T = 1.3 K leads to an increase in the resistivity up to (5 x 10(4))% under a...
Show moreWe present a detailed quantum oscillatory study on the Dirac type-II semimetallic candidates PdTe2 and PtTe2 via the temperature and the angular dependence of the de Haas-van Alphen and Shubnikov-de Haas effects. In high-quality single crystals of both compounds, i.e., displaying carrier mobilities between 10(3) and 10(4) cm(2)/Vs, we observed a large nonsaturating magnetoresistivity which in PtTe2 at a temperature T = 1.3 K leads to an increase in the resistivity up to (5 x 10(4))% under a magnetic field mu H-0 = 62 T. These high mobilities correlate with their light effective masses in the range of 0.04 to 1 bare electron mass according to our measurements. For PdTe2 the experimentally determined Fermi surface cross-sectional areas show excellent agreement with those resulting from band structure calculations. Surprisingly, this is not the case for PtTe2, whose agreement between calculations and experiments is relatively poor even when electronic correlations are included in the calculations. Therefore, our study provides strong support for the existence of a Dirac type-II node in PdTe2 and probably also for PtTe2. Band structure calculations indicate that the topologically nontrivial bands of PtTe2 do not cross the Fermi level epsilon(F). In contrast, for PdTe2 the Dirac type-II cone does intersect Bp, although our calculations also indicate that the associated cyclotron orbit on the Fermi surface is located in a distinct k(z) plane with respect to that of the Dirac type-II node. Therefore, it should yield a trivial Berry phase.
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Date Issued: 2018-06-29
Identifier: FSU_libsubv1_wos_000436907600002, 10.1103/PhysRevB.97.235154
Format: Citation

Title: Collective Dynamics And Strong Pinning Near The Onset Of Charge Order In La1.48nd0.4sr0.12cuo4.
Creator: Baity, P. G., Sasagawa, T., Popovic, Dragana
Abstract/Description: The dynamics of charge-ordered states is one of the key issues in underdoped cuprate high-temperature superconductors, but static short-range charge-order (CO) domains have been detected in almost all cuprates. We probe the dynamics across the CO (and structural) transition in La1.48Nd0.4Sr0.12CuO4 by measuring nonequilibrium charge transport, or resistance R as the system responds to a change in temperature and to an applied magnetic field. We find evidence for metastable states, collective...
Show moreThe dynamics of charge-ordered states is one of the key issues in underdoped cuprate high-temperature superconductors, but static short-range charge-order (CO) domains have been detected in almost all cuprates. We probe the dynamics across the CO (and structural) transition in La1.48Nd0.4Sr0.12CuO4 by measuring nonequilibrium charge transport, or resistance R as the system responds to a change in temperature and to an applied magnetic field. We find evidence for metastable states, collective behavior, and criticality. The collective dynamics in the critical regime indicates strong pinning by disorder. Surprisingly, nonequilibrium effects, such as avalanches in R, are revealed only when the critical region is approached from the charge-ordered phase. Our results on La1.48Nd0.4Sr0.12CuO4 provide the long-sought evidence for the fluctuating order across the CO transition, and also set important constraints on theories of dynamic stripes.
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Date Issued: 2018-04-12
Identifier: FSU_libsubv1_wos_000429777200009, 10.1103/PhysRevLett.120.156602
Format: Citation

Title: Preconditioner-free Wiener Filtering With A Dense Noise Matrix.
Creator: Huffenberger, Kevin M.
Abstract/Description: This work extends the Elsner & Wandelt (2013) iterative method for efficient, preconditioner-free Wiener filtering to cases in which the noise covariance matrix is dense, but can be decomposed into a sum whose parts are sparse in convenient bases. The new method, which uses multiple messenger fields, reproduces Wiener-filter solutions for test problems, and we apply it to a case beyond the reach of the Elsner & Wandelt (2013) method. We compute the Wiener-filter solution for a simulated...
Show moreThis work extends the Elsner & Wandelt (2013) iterative method for efficient, preconditioner-free Wiener filtering to cases in which the noise covariance matrix is dense, but can be decomposed into a sum whose parts are sparse in convenient bases. The new method, which uses multiple messenger fields, reproduces Wiener-filter solutions for test problems, and we apply it to a case beyond the reach of the Elsner & Wandelt (2013) method. We compute the Wiener-filter solution for a simulated Cosmic Microwave Background (CMB) map that contains spatially varying, uncorrelated noise, isotropic 1/f noise, and large-scale horizontal stripes (like those caused by atmospheric noise). We discuss simple extensions that can filter contaminated modes or inverse-noise-filter the data. These techniques help to address complications in the noise properties of maps from current and future generations of ground-based Microwave Background experiments, like Advanced ACTPol, Simons Observatory, and CMB-S4.
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Date Issued: 2018-05-01
Identifier: FSU_libsubv1_wos_000430944100042, 10.1093/mnras/sty232
Format: Citation

Title: Suppressed Density Of States In Self-generated Coulomb Glasses.
Creator: Rademaker, Louk, Nussinov, Zohar, Balents, Leon, Dobrosavljevic, Vladimir
Abstract/Description: We investigate the structure of metastable states in self-generated Coulomb glasses. In dramatic contrast to disordered electron glasses, we find that these states lack marginal stability. Such absence of marginal stability is reflected by the suppression of the single-particle density of states into an exponentially soft gap of the form g(c) similar to e(-V)/xi vertical bar epsilon vertical bar. To analytically explain this behavior, we extend the stability criterion of Efros and Shklovskii...
Show moreWe investigate the structure of metastable states in self-generated Coulomb glasses. In dramatic contrast to disordered electron glasses, we find that these states lack marginal stability. Such absence of marginal stability is reflected by the suppression of the single-particle density of states into an exponentially soft gap of the form g(c) similar to e(-V)/xi vertical bar epsilon vertical bar. To analytically explain this behavior, we extend the stability criterion of Efros and Shklovskii to incorporate local charge correlations, in qualitative agreement with our numerical findings. Our work suggests the existence of a new class of self-generated glasses dominated by strong geometric frustration.
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Date Issued: 2018-04-13
Identifier: FSU_libsubv1_wos_000429936200002, 10.1088/1367-2630/aab8ce
Format: Citation

Title: The Nebular Spectra Of The Transitional Type Ia Supernovae 2007on And 2011iv: Broad, Multiple Components Indicate Aspherical Explosion Cores.
Creator: Mazzali, P. A., Ashall, C., Pian, E., Stritzinger, M. D., Gall, C., Phillips, M. M., Hoflich, P., Hsiao, E.
Abstract/Description: The nebular-epoch spectrum of the rapidly declining, 'transitional' Type Ia supernova (SN) 2007on showed double emission peaks, which have been interpreted as indicating that the SN was the result of the direct collision of two white dwarfs. The spectrum can be reproduced using two distinct emission components, one redshifted and one blueshifted. These components are similar in mass but have slightly different degrees of ionization. They recede from one another at a line-of-sight speed larger...
Show moreThe nebular-epoch spectrum of the rapidly declining, 'transitional' Type Ia supernova (SN) 2007on showed double emission peaks, which have been interpreted as indicating that the SN was the result of the direct collision of two white dwarfs. The spectrum can be reproduced using two distinct emission components, one redshifted and one blueshifted. These components are similar in mass but have slightly different degrees of ionization. They recede from one another at a line-of-sight speed larger than the sum of the combined expansion velocities of their emitting cores, thereby acting as two independent nebulae. While this configuration appears to be consistent with the scenario of two white dwarfs colliding, it may also indicate an off-centre delayed detonation explosion of a near-Chandrasekhar-mass white dwarf. In either case, broad emission line widths and a rapidly evolving light curve can be expected for the bolometric luminosity of the SN. This is the case for both SNe 2007on and 2011iv, also a transitional SN Ia that exploded in the same elliptical galaxy, NGC1404. Although SN 2011iv does not show double-peaked emission line profiles, the width of its emission lines is such that a two-component model yields somewhat better results than a single-component model. Most of the mass ejected is in one component, however, which suggests that SN 2011iv was the result of the off-centre ignition of a Chandrasekhar-mass white dwarf.
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Date Issued: 2018-05-01
Identifier: FSU_libsubv1_wos_000430944100006, 10.1093/mnras/sty434
Format: Citation

Title: Sn 2016coi/asassn-16fp: An Example Of Residual Helium In A Type Ic Supernova?.
Creator: Prentice, S. J., Ashall, C., Mazzali, P. A., Zhang, J.-J., James, P. A., Wang, X.-F., Vinko, J., Percival, S., Short, L., Piascik, A., Huang, F., Mo, J., Rui, L.-M., Wang, J.-G....
Show morePrentice, S. J., Ashall, C., Mazzali, P. A., Zhang, J.-J., James, P. A., Wang, X.-F., Vinko, J., Percival, S., Short, L., Piascik, A., Huang, F., Mo, J., Rui, L.-M., Wang, J.-G., Xiang, D.-F., Xin, Y.-X., Yi, W.-M., Yu, X.-G., Zhai, Q., Zhang, T.-M., Hosseinzadeh, G., Howell, D. A., McCully, C., Valenti, S., Cseh, B., Hanyecz, O., Kriskovics, L., Pal, A., Sarneczky, K., Sodor, A., Szakats, R., Szekely, P., Varga-Verebelyi, E., Vida, K., Bradac, M., Reichart, D. E., Sand, D., Tartaglia, L.
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Abstract/Description: The optical observations of Ic-4 supernova (SN) 2016coi/ASASSN-16fp, from similar to 2 to similar to 450 d after explosion, are presented along with analysis of its physical properties. The SN shows the broad lines associated with SNe Ic-3/4 but with a key difference. The early spectra display a strong absorption feature at similar to 5400 angstrom which is not seen in other SNe Ic-3/4 at this epoch. This feature has been attributed to He I in the literature. Spectral modelling of the SN in...
Show moreThe optical observations of Ic-4 supernova (SN) 2016coi/ASASSN-16fp, from similar to 2 to similar to 450 d after explosion, are presented along with analysis of its physical properties. The SN shows the broad lines associated with SNe Ic-3/4 but with a key difference. The early spectra display a strong absorption feature at similar to 5400 angstrom which is not seen in other SNe Ic-3/4 at this epoch. This feature has been attributed to He I in the literature. Spectral modelling of the SN in the early photospheric phase suggests the presence of residual He in a C/O dominated shell. However, the behaviour of the He I lines is unusual when compared with He-rich SNe, showing relatively low velocities and weakening rather than strengthening over time. The SN is found to rise to peak similar to 16 d after core-collapse reaching a bolometric luminosity of L-p similar to 3 x 10(42) erg s(-1). Spectral models, including the nebular epoch, show that the SN ejected 2.5-4M(circle dot) of material, with similar to 1.5M(circle dot) below 5000 km s(-1), and with a kinetic energy of (4.5-7) x 10(51) erg. The explosion synthesized similar to 0.14M(circle dot) of Ni-56. There are significant uncertainties in E(B - V)(host) and the distance, however, which will affect L-p and M-Ni. SN 2016coi exploded in a host similar to the Large Magellanic Cloud (LMC) and away from star-forming regions. The properties of the SN and the host-galaxy suggest that the progenitor had M-ZAMS of 23-28M(circle dot) and was stripped almost entirely down to its C/O core at explosion.
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Date Issued: 2018-08-01
Identifier: FSU_libsubv1_wos_000441282300093, 10.1093/mnras/sty1223
Format: Citation

Title: Isotensor Dibaryon In The Pp -> Pp Pi(+)pi(-) Reaction?.
Creator: Adlarson, P., Augustyniak, W., Bardan, W., Bashkanov, M., Bergmann, F. S., Berlowski, M., Bondar, A., Buescher, M., Calen, H., Ciepal, I., Clement, H., Czerwinski, E., Demmich,...
Show moreAdlarson, P., Augustyniak, W., Bardan, W., Bashkanov, M., Bergmann, F. S., Berlowski, M., Bondar, A., Buescher, M., Calen, H., Ciepal, I., Clement, H., Czerwinski, E., Demmich, K., Engels, R., Erven, A., Erven, W., Eyrich, W., Fedorets, P., Foehl, K., Fransson, K., Goldenbaum, F., Goswami, A., Grigoryev, K., Heijkenskjold, L., Hejny, V., Huesken, N., Jarczyk, L., Johansson, T., Kamys, B., Kemmerling, G., Khoukaz, A., Khreptak, O., Kirillov, D. A., Kistryn, S., Kleines, H., Klos, B., Krzemien, W., Kulessa, P., Kupsc, A., Lalwani, K., Lersch, D., Lorentz, B., Magiera, A., Maier, R., Marciniewski, P., Marianski, B., Morsch, H. P., Moskal, P., Ohm, H., Parol, W., del Rio, E. Perez, Piskunov, N. M., Prasuhn, D., Pszczel, D., Pysz, K., Ritman, J., Roy, A., Rudy, Z., Rundel, O., Sawant, S., Schadmand, S., Schatti-Ozerianska, I., Sefzick, T., Serdyuk, V., Shwartz, B., Skorodko, T., Skurzok, M., Smyrski, J., Sopov, V., Stassen, R., Stepaniak, J., Stephan, E., Sterzenbach, G., Stockhorst, H., Stroeher, H., Szczurek, A., Trzcinski, A., Wolke, M., Wronska, A., Wuestner, P., Yamamoto, A., Zabierowski, J., Zielinski, M. J., Zlomanczuk, J., Zupranski, P., Zurek, M.
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Abstract/Description: Exclusive measurements of the quasifree pp -> pp pi(+)pi(-) reaction have been carried out at WASA@ COSY by means of pd collisions at T-p = 1.2 GeV. Total and differential cross sections have been extracted covering the energy region T-p = 1.08-1.36 GeV, which is the region of N* (1440) and Delta(123)Delta(1232) resonance excitations. Calculations describing these excitations by t-channel meson exchange are at variance with the measured differential cross sections and underpredict...
Show moreExclusive measurements of the quasifree pp -> pp pi(+)pi(-) reaction have been carried out at WASA@ COSY by means of pd collisions at T-p = 1.2 GeV. Total and differential cross sections have been extracted covering the energy region T-p = 1.08-1.36 GeV, which is the region of N* (1440) and Delta(123)Delta(1232) resonance excitations. Calculations describing these excitations by t-channel meson exchange are at variance with the measured differential cross sections and underpredict substantially the experimental total cross section. An isotensor Delta N dibaryon resonance with I(J(P)) = 2(1(+)) produced associatedly with a pion is able to overcome these deficiencies.
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Date Issued: 2018-08-01
Identifier: FSU_libsubv1_wos_000440415600003, 10.1103/PhysRevLett.121.052001
Format: Citation

Title: Nebular Spectroscopy Of The "blue Bump" Type Ia Supernova 2017cbv.
Creator: Sand, D. J., Graham, M. L., Botyanszki, J., Hiramatsu, D., McCully, C., Valenti, S., Hosseinzadeh, G., Howell, D. A., Burke, J., Cartier, R., Diamond, T., Hsiao, E. Y., Jha, S....
Show moreSand, D. J., Graham, M. L., Botyanszki, J., Hiramatsu, D., McCully, C., Valenti, S., Hosseinzadeh, G., Howell, D. A., Burke, J., Cartier, R., Diamond, T., Hsiao, E. Y., Jha, S. W., Kasen, D., Kumar, S., Marion, G. H., Suntzeff, N., Tartaglia, L., Wheeler, J. C., Wyatt, S.
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Abstract/Description: We present nebular phase optical and near-infrared spectroscopy of the Type Ia supernova (SN) 2017cbv. The early light curves of SN 2017cbv showed a prominent blue bump in the U, B, and g bands lasting for similar to 5 days. One interpretation of the early light curve is that the excess blue light is due to shocking of the SN ejecta against a nondegenerate companion star-a signature of the single degenerate scenario. If this is the correct interpretation, the interaction between the SN ejecta...
Show moreWe present nebular phase optical and near-infrared spectroscopy of the Type Ia supernova (SN) 2017cbv. The early light curves of SN 2017cbv showed a prominent blue bump in the U, B, and g bands lasting for similar to 5 days. One interpretation of the early light curve is that the excess blue light is due to shocking of the SN ejecta against a nondegenerate companion star-a signature of the single degenerate scenario. If this is the correct interpretation, the interaction between the SN ejecta and the companion star could result in significant Ha (or helium) emission at late times, possibly along with other species, depending on the companion star and its orbital separation. A search for Ha emission in our +302 d spectrum yields a nondetection, with a L-H alpha < 8.0 x 10(35) erg s(-1) (given an assumed distance of D = 12.3 Mpc), which we verified by implanting simulated Ha emission into our data. We make a quantitative comparison to models of swept-up material stripped from a nondegenerate companion star and limit the mass of hydrogen that might remain undetected to M-H < 1 x 10(-4) M-circle dot. A similar analysis of helium star related lines yields a M-He < 5 x 10(-4) M-circle dot. Taken at face value, these results argue against a nondegenerate H- or He-rich companion in Roche lobe overflow as the progenitor of SN 2017cbv. Alternatively, there could be weaknesses in the envelope-stripping and radiative transfer models necessary to interpret the strong H and He flux limits.
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Date Issued: 2018-08-10
Identifier: FSU_libsubv1_wos_000441126000010, 10.3847/1538-4357/aacde8
Format: Citation

Title: Low-energy Excitations In Quantum Spin Liquids Identified By Optical Spectroscopy.
Creator: Pustogow, A., Saito, Y., Zhukova, E., Gorshunov, B., Kato, R., Lee, T.-H., Fratini, S., Dobrosavljevic, V., Dressel, M.
Abstract/Description: The electrodynamic response of organic spin liquids with highly frustrated triangular lattices has been measured in a wide energy range. While the overall optical spectra of these Mott insulators are governed by transitions between the Hubbard bands, distinct in-gap excitations can be identified at low temperatures and frequencies, which we attribute to the quantum-spin-liquid state. For the strongly correlated ss'-EtMe3Sb[Pd(dmit)(2)](2), we discover enhanced conductivity below 175 cm(-1),...
Show moreThe electrodynamic response of organic spin liquids with highly frustrated triangular lattices has been measured in a wide energy range. While the overall optical spectra of these Mott insulators are governed by transitions between the Hubbard bands, distinct in-gap excitations can be identified at low temperatures and frequencies, which we attribute to the quantum-spin-liquid state. For the strongly correlated ss'-EtMe3Sb[Pd(dmit)(2)](2), we discover enhanced conductivity below 175 cm(-1), comparable to the energy of the magnetic coupling J approximate to 250 K. For omega -> 0, these low-frequency excitations vanish faster than the charge-carrier response subject to Mott-Hubbard correlations, resulting in a dome-shaped band peaked at 100 cm(-1). Possible relations to spinons, magnons, and disorder are discussed.
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Date Issued: 2018-08-03
Identifier: FSU_libsubv1_wos_000440724200014, 10.1103/PhysRevLett.121.056402
Format: Citation

Title: First Measurement Of Xi(-) Polarization In Photoproduction.
Creator: Bono, J., Guo, L., Raue, B. A., Adhikari, S., Kunkel, M. C., Adhikari, K. P., Akbar, Z., Amaryan, M. J., Ball, J., Barion, L., Bashkanov, M., Battaglieri, M., Batourine, V.,...
Show moreBono, J., Guo, L., Raue, B. A., Adhikari, S., Kunkel, M. C., Adhikari, K. P., Akbar, Z., Amaryan, M. J., Ball, J., Barion, L., Bashkanov, M., Battaglieri, M., Batourine, V., Bedlinskiy, I., Biselli, A. S., Brooks, W. K., Burkert, V. D., Cao, F., Carman, D. S., Celentano, A., Charles, G., Chetry, T., Ciullo, G., Clary, Brandon A., Cole, P. L., Contalbrigo, M., Crede, V., D'Angelo, A., Dashyan, N., De Vita, R., Defurne, M., Deur, A., Diehl, S., Djalali, C., Dugger, M., Egiyan, H., El Alaoui, A., El Fassi, L., Eugenio, P., Fedotov, G., Filippi, A., Fradi, A., Gavalian, G., Gevorgyan, N., Ghandilyan, Y., Girod, F. X., Glazier, D. I., Gohn, W., Golovatch, E., Gothe, R. W., Griffioen, K. A., Hafidi, K., Harrison, N., Hattawy, M., Heddle, D., Hicks, K., Holtrop, M., Ilieva, Y., Ireland, D. G., Isupov, E. L., Jo, H. S., Johnston, S., Kabir, M. L., Keller, D., Khachatryan, G., Khachatryan, M., Khandaker, M., Kim, A., Kim, W., Klein, A., Klein, F. J., Kubarovsky, V., Lenisa, P., Livingston, K., MacGregor, I. J. D., Markov, N., McKinnon, B., Mineeva, T., Montgomery, R. A., Camacho, C. Munoz, Niculescu, G., Osipenko, M., Ostrovidov, A. I., Paolone, M., Paremuzyan, R., Park, K., Pasyuk, E., Phelps, W., Pogorelko, O., Price, J. W., Prok, Y., Protopopescu, D., Ripani, M., Rizzo, A., Rosner, G., Sabatie, F., Salgado, C., Schumacher, R. A., Sharabian, Y., Skorodumina, Iu, Smith, G. D., Sokhan, D., Sparveris, N., Stepanyan, S., Strakovsky, I. I., Strauch, S., Taiuti, M., Tan, J. A., Ungaro, M., Voskanyan, H., Voutier, E., Wang, R., Wei, X., Wood, M. H., Zachariou, N., Zana, L., Zhang, J., Zhao, Z. W.
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Abstract/Description: Despite decades of studies of the photoproduction of hyperons, both their production mechanisms and their spectra of excited states are still largely unknown. While the parity-violating weak decay of hyperons offers a means of measuring their polarization, which could help discern their production mechanisms and identify their excitation spectra, no such study has been possible for doubly strange baryons in photoproduction, due to low production cross sections. However, by making use of the...
Show moreDespite decades of studies of the photoproduction of hyperons, both their production mechanisms and their spectra of excited states are still largely unknown. While the parity-violating weak decay of hyperons offers a means of measuring their polarization, which could help discern their production mechanisms and identify their excitation spectra, no such study has been possible for doubly strange baryons in photoproduction, due to low production cross sections. However, by making use of the reaction gamma p -> K+K+Xi(-), we have measured, for the first time, the induced polarization, P, and the transferred polarization from circularly polarized real photons, characterized by C-x and C-z, to recoiling Xi(-) s. The data were obtained using the CEBAF Large Acceptance Spectrometer (CLAS) at Jefferson Lab for photon energies from just over threshold (2.4 GeV) to 5.45 GeV. These first-time measurements are compared, and are shown to broadly agree, with model predictions in which cascade photoproduction proceeds through the decay of intermediate hyperon resonances that are produced via relativistic meson exchange, offering a new step forward in the understanding of the production and polarization of doubly-strange baryons. (c) 2018 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/). Funded by SCOAP(3).
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Date Issued: 2018-08-10
Identifier: FSU_libsubv1_wos_000441762300038, 10.1016/j.physletb.2018.07.004
Format: Citation

Title: Semi-inclusive Pi(0) Target And Beam-target Asymmetries From 6 Gev Electron Scattering With Clas.
Creator: Jawalkar, S., Koirala, S., Avakian, H., Bosted, P., Griffioen, K. A., Keith, C., Kuhn, S. E., Adhikari, K. P., Adhikari, S., Adikaram, D., Akbar, Z., Amaryan, M. J., Pereira, S....
Show moreJawalkar, S., Koirala, S., Avakian, H., Bosted, P., Griffioen, K. A., Keith, C., Kuhn, S. E., Adhikari, K. P., Adhikari, S., Adikaram, D., Akbar, Z., Amaryan, M. J., Pereira, S. Anefalos, Ball, J., Baltzell, N. A., Battaglieri, M., Batourine, V., Bedlinskiy, I., Biselli, A. S., Boiarinov, S., Briscoe, W. J., Brock, J., Brooks, W. K., Bultmann, S., Burkert, V. D., Cao, Frank Thanh, Carlin, C., Carman, D. S., Celentano, A., Charles, G., Chetry, T., Ciullo, G., Clark, L., Colaneri, L., Cole, P. L., Contalbrigo, M., Cortes, O., Crede, V., D'Angelo, A., Dashyan, N., De Vita, R., De Sanctis, E., Defurne, M., Deur, A., Djalali, C., Ddoge, G., Dupre, R., Egiyan, H., El Alaoui, A., El Fassi, L., Elouadrhiri, L., Eugenio, P., Fedotov, G., Fegan, S., Fersch, R., Filippi, A., Fleming, J. A., Forest, T. A., Fradi, A., Garcon, M., Ghandilyan, Y., Gilfoyle, G. P., Giovanetti, K. L., Girod, F. X., Gleason, C., Gohn, W., Golovatch, E., Gothe, R. W., Guidal, M., Guler, N., Guo, L., Hakobyan, H., Hanretty, C., Harrison, N., Hattawy, M., Heddle, D., Hicks, K., Hollis, G., Holtrop, M., Hughes, S. M., Ilieva, Y., Ireland, D. G., Ishkhanov, B. S., Isupov, E. L., Jenkins, D., Jiang, H., Joo, K., Joosten, S., Keller, D., Khachatryan, G., Khachatryan, M., Khandaker, M., Kim, A., Kim, W., Klein, A., Klein, F. J., Kubarovsky, V., Kuleshov, S. V., Lanza, L., Lenisa, P., Livingston, K., Lu, H. Y., MacGregor, I. J. D., Markov, N., Mayer, M., McCracken, M. E., McKinnon, B., Meyer, C. A., Mineeva, T., Mirazita, M., Mokeev, V., Montgomery, R. A., Movsisyan, A., Camacho, C. Munoz, Nadel-Turonski, P., Net, L. A., Niccolai, S., Niculescu, G., Niculescu, I., Osipenko, M., Ostrovidov, A. I., Paremuzyan, R., Park, K., Pasyuk, E., Phelps, E., Phelps, W., Pierce, J., Pisano, S., Pogorelko, O., Price, J. W., Prok, Y., Protopopescu, D., Raue, B. A., Ripani, M., Riser, D., Rizzo, A., Rosner, G., Rossi, P., Sabatie, F., Salgado, C., Schumacher, R. A., Seder, E., Sharabian, Y. G., Simonyan, A., Skorodumina, Iu, Smith, G. D., Sober, D. I., Sokhan, D., Sparveris, N., Stankovic, I., Strauch, S., Taiuti, M., Ungaro, M., Voskanyan, H., Voutier, E., Walford, N. K., Watts, D. P., Wei, X., Weinstein, L. B., Wood, M. H., Zachariou, N., Zhang, J., Zhao, Z. W.
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Abstract/Description: We present precision measurements of the target and beam-target spin asymmetries from neutral pion electroproduction in deep-inelastic scattering (DIS) using the CEBAF Large Acceptance Spectrometer (CLAS) at Jefferson Lab. We scattered 6-GeV, longitudinally polarized electrons off longitudinally polarized protons in a cryogenic (14)NH(3)target, and extracted double and single target spin asymmetries for ep -> e'pi(0)Xin multidimensional bins in four-momentum transfer (1.0 < Q(2) < 3.2GeV(2)),...
Show moreWe present precision measurements of the target and beam-target spin asymmetries from neutral pion electroproduction in deep-inelastic scattering (DIS) using the CEBAF Large Acceptance Spectrometer (CLAS) at Jefferson Lab. We scattered 6-GeV, longitudinally polarized electrons off longitudinally polarized protons in a cryogenic (14)NH(3)target, and extracted double and single target spin asymmetries for ep -> e'pi(0)Xin multidimensional bins in four-momentum transfer (1.0 < Q(2) < 3.2GeV(2)), Bjorken-x(0.12 < x < 0.48), hadron energy fraction (0.4 < z < 0.7), transverse pion momentum (0 < P-T < 1.0GeV), and azimuthal angel phi(h) between the lepton scattering and hadron production planes. We extracted asymmetries as a function of both xand P-T, which provide access to transverse-momentum distributions of longitudinally polarized quarks. The double spin asymmetries depend weakly on P-T. The sin2 phi(h) moments are zero within uncertainties, which is consistent with the expected suppression of the Collins fragmentation function. The observed sin phi(h) moments suggest that quark gluon correlations are significant at large x. (C) 2018 The Authors. Published by Elsevier B.V.
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Date Issued: 2018-07-10
Identifier: FSU_libsubv1_wos_000438486900099, 10.1016/j.physletb.2018.06.014
Format: Citation

Title: Near-infrared Spectral Evolution Of The Type Ia Supernova 2014j In The Nebular Phase: Implications For The Progenitor System.
Creator: Diamond, T. R., Hoeflich, P., Hsiao, E. Y., Sand, D. J., Sonneborn, G., Phillips, M. M., Hristov, B., Collins, D. C., Ashall, C., Marion, G. H., Stritzinger, M., Morrell, N.,...
Show moreDiamond, T. R., Hoeflich, P., Hsiao, E. Y., Sand, D. J., Sonneborn, G., Phillips, M. M., Hristov, B., Collins, D. C., Ashall, C., Marion, G. H., Stritzinger, M., Morrell, N., Gerardy, C. L., Penney, R. B.
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Abstract/Description: As the closest Type Ia supernova in decades, SN 2014J provides a unique opportunity for detailed investigation into observational signatures of the progenitor system, explosion mechanism, and burning product distribution. We present a late-time near-infrared spectral series from Gemini-N at 307-466 days after the explosion. Following the H-band evolution probes the distribution of radioactive iron group elements, the extent of mixing, and the presence of magnetic fields in the expanding...
Show moreAs the closest Type Ia supernova in decades, SN 2014J provides a unique opportunity for detailed investigation into observational signatures of the progenitor system, explosion mechanism, and burning product distribution. We present a late-time near-infrared spectral series from Gemini-N at 307-466 days after the explosion. Following the H-band evolution probes the distribution of radioactive iron group elements, the extent of mixing, and the presence of magnetic fields in the expanding ejecta. Comparing the isolated 1.6440 mu m [Fe II] emission line with synthetic models shows consistency with a Chandrasekhar mass white dwarf of rho(c) = 0.7 x 10(9) g cm(-3) undergoing a delayed detonation. The ratio of the flux in the neighboring 1.54 mu m emission feature to the flux in the 1.6440 mu m feature shows evidence of some limited mixing of stable and radioactive iron group elements in the central regions. Additionally, the evolution of the 1.6440 mu m line shows an intriguing asymmetry. When measuring line width of this feature, the data show an increase in line width not seen in the evolution of the synthetic spectra, corresponding to approximate to 1000 km s(-1), which could be caused by a localized transition to detonation producing asymmetric ionization in the ejecta. Using the difference in width between the different epochs, an asymmetric component in the central regions, corresponding to approximately the inner 2 x 10(-4) of white dwarf mass suggests an off-center ignition of the initial explosion and hence of the kinematic center from the chemical center. Several additional models investigated, including a He detonation and a merger, have difficulty reproducing the features seen in these spectra.
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Date Issued: 2018-07-10
Identifier: FSU_libsubv1_wos_000438598000018, 10.3847/1538-4357/aac434
Format: Citation

Title: Differential Cross Section For Gamma D -> Omega D Using Clas At Jefferson Lab.
Creator: Chetry, T., Hicks, K., Compton, N., Sargsian, M., Adhikari, S., Ball, J., Balossino, I., Barion, L., Battaglieri, M., Batourine, V., Bedlinskiy, I., Biselli, A. S., Boiarinov, S...
Show moreChetry, T., Hicks, K., Compton, N., Sargsian, M., Adhikari, S., Ball, J., Balossino, I., Barion, L., Battaglieri, M., Batourine, V., Bedlinskiy, I., Biselli, A. S., Boiarinov, S., Briscoe, W. J., Brooks, W. K., Burkert, V. D., Carman, D. S., Celentano, A., Charles, G., Ciullo, G., Clark, L., Clary, Brandon A., Cole, P. L., Contalbrigo, M., Crede, V., D'Angelo, A., Dashyan, N., De Vita, R., De Sanctis, E., Deur, A., Djalali, C., Dupre, R., El Alaoui, A., El Fassi, L., Eugenio, P., Fedotov, G., Fersch, R., Filippi, A., Gavalian, G., Ghandilyan, Y., Giovanetti, K. L., Girod, F. X., Golovatch, E., Gothe, R. W., Griffioen, K. A., Guo, L., Hafidi, K., Harrison, N., Hattawy, M., Holtrop, M., Ilieva, Y., Ireland, D. G., Ishkhanov, B. S., Isupov, E. L., Jenkins, D., Johnston, S., Kabir, M. L., Keller, D., Khachatryan, G., Khachatryan, M., Khandaker, M., Kim, A., Kim, W., Klein, F. J., Kubarovsky, V., Lanza, L., Lenisa, P., Livingston, K., MacGregor, I. J. D., Markov, N., McKinnon, B., Mokeev, V., Movsisyan, A., Camacho, C. Munoz, Nadel-Turonski, P., Niccolai, S., Niculescu, G., Osipenko, M., Ostrovidov, A. I., Paolone, M., Paremuzyan, R., Park, K., Pasyuk, E., Phelps, W., Pogorelko, O., Price, J. W., Prok, Y., Ripani, M., Riser, D., Ritchie, B. G., Rizzo, A., Rosner, G., Salgado, C., Schumacher, R. A., Skorodumina, Iu, Smith, G. D., Sober, D. I., Sokhan, D., Sparveris, N., Stepanyan, S., Strakovsky, I. I., Strauch, S., Taiuti, M., Tan, J. A., Ungaro, M., Voskanyan, H., Voutier, E., Weinstein, L. B., Wood, M. H., Zachariou, N., Zhang, J., Zhao, Z. W.
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Abstract/Description: The cross section for coherent omega-meson photoproduction off the deuteron has been measured for the first time as a function of the momentum transfer t=(P-gamma - P-omega)(2) and photon energy E-gamma using the CLAS detector at the Thomas Jefferson National Accelerator Facility. The cross sections are measured in the energy range 1.4 < E-gamma < 3.4GeV. A model based on omega- N rescattering is consistent with the data at low and intermediate momentum transfer, vertical bar t vertical bar....
Show moreThe cross section for coherent omega-meson photoproduction off the deuteron has been measured for the first time as a function of the momentum transfer t=(P-gamma - P-omega)(2) and photon energy E-gamma using the CLAS detector at the Thomas Jefferson National Accelerator Facility. The cross sections are measured in the energy range 1.4 < E-gamma < 3.4GeV. A model based on omega- N rescattering is consistent with the data at low and intermediate momentum transfer, vertical bar t vertical bar. For 2.8 < E-gamma < 3.4GeV, the total cross-section of omega - N scattering, based on fits within the framework of the Vector Meson Dominance model, is in the range of 30-40 mb. (C) 2018 The Authors. Published by Elsevier B.V.
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Date Issued: 2018-07-10
Identifier: FSU_libsubv1_wos_000438486900096, 10.1016/j.physletb.2018.06.003
Format: Citation

Title: Measurements Of Omega(-) Branching Fractions.
Creator: Xiao, T., Dobbs, S., Tomaradze, A., Seth, Kamal K.
Abstract/Description: Using e(+)e(-) annihilation data taken with the CLEO-c detector, measurements of two major Obranching fractions have been made using the reaction psi(2S) -> Omega(-)(Omega) over bar (+) . The Omega(-) decay channels are identified through momentum distributions of charged particles, and systematics of the Omega(-) branching fractions have been studied. The results are B(Omega(-) -> Lambda(0) K-) = (68.9 +/- 9.5 +/- 4.3)% and B(Omega(-) -> Xi pi(-0)) = (19.0 +/- 4.0 +/- 1.2)%.
Date Issued: 2018-07-31
Identifier: FSU_libsubv1_wos_000440384800001, 10.1103/PhysRevD.98.012007
Format: Citation

Title: The Nature Of Spin Excitations In The One-third Magnetization Plateau Phase Of Ba3cosb2o9.
Creator: Kamiya, Y., Ge, L., Hong, Tao, Qiu, Y., Quintero-Castro, D. L., Lu, Z., Cao, H. B., Matsuda, M., Choi, E. S., Batista, C. D., Mourigal, M., Zhou, N. D., Ma, J.
Abstract/Description: Magnetization plateaus in quantum magnets-where bosonic quasiparticles crystallize into emergent spin superlattices-are spectacular yet simple examples of collective quantum phenomena escaping classical description. While magnetization plateaus have been observed in a number of spin-1/2 antiferromagnets, the description of their magnetic excitations remains an open theoretical and experimental challenge. Here, we investigate the dynamical properties of the triangular-lattice spin-1/2...
Show moreMagnetization plateaus in quantum magnets-where bosonic quasiparticles crystallize into emergent spin superlattices-are spectacular yet simple examples of collective quantum phenomena escaping classical description. While magnetization plateaus have been observed in a number of spin-1/2 antiferromagnets, the description of their magnetic excitations remains an open theoretical and experimental challenge. Here, we investigate the dynamical properties of the triangular-lattice spin-1/2 antiferromagnet Ba3CoSb2O9 in its one-third magnetization plateau phase using a combination of nonlinear spin-wave theory and neutron scattering measurements. The agreement between our theoretical treatment and the experimental data demonstrates that magnons behave semiclassically in the plateau in spite of the purely quantum origin of the underlying magnetic structure. This allows for a quantitative determination of Ba3CoSb2O9 exchange parameters. We discuss the implication of our results to the deviations from semiclassical behavior observed in zero-field spin dynamics of the same material and conclude they must have an intrinsic origin.
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Date Issued: 2018-07-10
Identifier: FSU_libsubv1_wos_000438031000004, 10.1038/s41467-018-04914-1
Format: Citation

Title: Progenitor Mass Distribution For Core-collapse Supernova Remnants In M31 And M33.
Creator: Diaz-Rodriguez, Mariangelly, Murphy, Jeremiah W., Rubin, David A., Dolphin, Andrew E., Williams, Benjamin F., Dalcanton, Julianne J.
Abstract/Description: Using the star formation histories (SFHs) near 94 supernova remnants (SNRs), we infer the progenitor mass distribution for core-collapse supernovae. We use Bayesian inference and model each SFH with multiple bursts of star formation (SF), one of which is assumed to be associated with the SNR. Assuming single-star evolution, the minimum mass of CCSNe is 7.33(-0.16)(+0.02)M(circle dot), the slope of the progenitor mass distribution is alpha = -2.96(-0.25)(+0.45), and the maximum mass is greater...
Show moreUsing the star formation histories (SFHs) near 94 supernova remnants (SNRs), we infer the progenitor mass distribution for core-collapse supernovae. We use Bayesian inference and model each SFH with multiple bursts of star formation (SF), one of which is assumed to be associated with the SNR. Assuming single-star evolution, the minimum mass of CCSNe is 7.33(-0.16)(+0.02)M(circle dot), the slope of the progenitor mass distribution is alpha = -2.96(-0.25)(+0.45), and the maximum mass is greater than M-max > 59M(circle dot) with a 68% confidence. While these results are consistent with previous inferences, they also provide tighter constraints. The progenitor distribution is somewhat steeper than a Salpeter initial mass function (alpha = -2.35). This suggests that either SNR catalogs are biased against the youngest SF regions, or the most massive stars do not explode as easily as lower mass stars. If SNR catalogs are biased, it will most likely affect the slope but not the minimum mass. The uncertainties are dominated by three primary sources of uncertainty, the SFH resolution, the number of SF bursts, and the uncertainty on SF rate in each age bin. We address the first two of these uncertainties, with an emphasis on multiple bursts. The third will be addressed in future work.
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Date Issued: 2018-07-10
Identifier: FSU_libsubv1_wos_000438195500007, 10.3847/1538-4357/aac6e1
Format: Citation

Title: Evidence For Z(c)(+/-)(3900) In Semi-inclusive Decays Of B-flavored Hadrons.
Creator: Abazov, V. M., Abbott, B., Acharya, B. S., Adams, M., Adams, T., Agnew, J. P., Alexeev, G. D., Alkhazov, G., Alton, A., Askew, A., Atkins, S., Augsten, K., Aushev, V., Aushev, Y...
Show moreAbazov, V. M., Abbott, B., Acharya, B. S., Adams, M., Adams, T., Agnew, J. P., Alexeev, G. D., Alkhazov, G., Alton, A., Askew, A., Atkins, S., Augsten, K., Aushev, V., Aushev, Y., Avila, C., Badaud, F., Bagby, L., Baldin, B., Bandurin, D., Banerjee, S., Barberis, E., Baringer, P., Bartlett, J. F., Bassler, U., Bazterra, V., Bean, A., Begalli, M., Bellantoni, L., Beri, S. B., Bernardi, G., Bernhard, R., Bertram, I., Besancon, M., Beuselinck, R., Bhat, P. C., Bhatia, S., Bhatnagar, V., Blazey, G., Blessing, S., Bloom, K., Boehnlein, A., Boline, D., Boos, E. E., Borissov, G., Borysova, M., Brandt, A., Brandt, O., Brochmann, M., Brock, R., Bross, A., Brown, D., Bu, X. B., Buehler, M., Buescher, V., Bunichev, V., Burdin, S., Buszello, C. P., Camacho-Perez, E., Casey, B. C. K., Castilla-Valdez, H., Caughron, S., Chakrabarti, S., Chan, K. M., Chandra, A., Chapon, E., Chen, G., Cho, S. W., Choi, S., Choudhary, B., Cihangir, S., Claes, D., Clutter, J., Cooke, M., Cooper, W. E., Corcoran, M., Couderc, F., Cousinou, M.-C., Cuth, J., Cutts, D., Das, A., Davies, G., de Jong, S. J., De La Cruz-Burelo, E., Deliot, F., Demina, R., Denisov, D., Denisov, S. P., Desai, S., Deterre, C., DeVaughan, K., Diehl, H. T., Diesburg, M., Ding, P. F., Dominguez, A., Drutskoy, A., Dubey, A., Dudko, L., Duperrin, A., Dutt, S., Eads, M., Edmunds, D., Ellison, J., Elvira, V. D., Enari, Y., Evans, H., Evdokimov, A., Evdokimov, V. N., Faure, A., Feng, L., Ferbel, T., Fiedler, F., Filthaut, F., Fisher, W., Fisk, H. E., Fortner, M., Fox, H., Franc, J., Fuess, S., Garbincius, P. H., Garcia-Bellido, A., Garcia-Gonzalez, J. A., Gavrilov, V., Geng, W., Gerber, C. E., Gershtein, Y., Ginther, G., Gogota, O., Golovanov, G., Grannis, P. D., Greder, S., Greenlee, H., Grenier, G., Gris, Ph, Grivaz, J.-F., Grohsjean, A., Grunendahl, S., Grunewald, M. W., Guillemin, T., Gutierrez, G., Gutierrez, P., Haley, J., Han, L., Harder, K., Harel, A., Hauptman, J. M., Hays, J., Head, T., Hebbeker, T., Hedin, D., Hegab, H., Heinson, A. P., Heintz, U., Hensel, C., Heredia-De La Cruz, I., Herner, K., Hesketh, G., Hildreth, M. D., Hirosky, R., Hoang, T., Hobbs, J. D., Hoeneisen, B., Hogan, J., Hohlfeld, M., Holzbauer, J. L., Howley, I., Hubacek, Z., Hynek, V., Iashvili, I., Ilchenko, Y., Illingworth, R., Ito, A. S., Jabeen, S., Jaffre, M., Jayasinghe, A., Jeong, M. S., Jesik, R., Jiang, P., Johns, K., Johnson, E., Johnson, M., Jonckheere, A., Jonsson, P., Joshi, J., Jung, A. W., Juste, A., Kajfasz, E., Karmanov, D., Katsanos, I., Kaur, M., Kehoe, R., Kermiche, S., Khalatyan, N., Khanov, A., Kharchilava, A., Kharzheev, Y. N., Kiselevich, I., Kohli, J. M., Kozelov, A., Kraus, J., Kumar, A., Kupco, A., Kurca, T., Kuzmin, V. A., Lammers, S., Lebrun, P., Lee, H. S., Lee, S. W., Lee, W. M., Lei, X., Lellouch, J., Li, D., Li, H., Li, L., Li, Q. Z., Lim, J. K., Lincoln, D., Linnemann, J., Lipaev, V. V., Lipton, R., Liu, H., Liu, Y., Lobodenko, A., Lokajicek, M., de Sa, R. Lopes, Luna-Garcia, R., Lyon, A. L., Maciel, A. K. A., Madar, R., Magana-Villalba, R., Malik, S., Malyshev, V. L., Mansour, J., Martinez-Ortega, J., McCarthy, R., McGivern, C. L., Meijer, M. M., Melnitchouk, A., Menezes, D., Mercadante, P. G., Merkin, M., Meyer, A., Meyer, J., Miconi, F., Mondal, N. K., Mulhearn, M., Nagy, E., Narain, M., Nayyar, R., Neal, H. A., Negret, J. P., Neustroev, P., Nguyen, H. T., Nunnemann, T., Orduna, J., Osman, N., Pal, A., Parashar, N., Parihar, V., Park, S. K., Partridge, R., Parua, N., Patwa, A., Penning, B., Perfilov, M., Peters, Y., Petridis, K., Petrillo, G., Petroff, P., Pleier, M.-A., Podstavkov, V. M., Popov, A., Prewitt, M., Price, D., Prokopenko, N., Qian, J., Quadt, A., Quinn, B., Ratoff, P. N., Razumov, I., Ripp-Baudot, I., Rizatdinova, F., Rominsky, M., Ross, A., Royon, C., Rubinov, P., Ruchti, R., Sajot, G., Sanchez-Hernandez, A., Sanders, M. P., Santos, A. S., Savage, G., Savitskyi, M., Sawyer, L., Scanlon, T., Schamberger, R. D., Scheglov, Y., Schellman, H., Schott, M., Schwanenberger, C., Schwienhorst, R., Sekaric, J., Severini, H., Shabalina, E., Shary, V., Shaw, S., Shchukin, A. A., Shkola, O., Simak, V., Skubic, P., Slattery, P., Snow, G. R., Snow, J., Snyder, S., Soldner-Rembold, S., Sonnenschein, L., Soustruznik, K., Stark, J., Stefaniuk, N., Stoyanova, D. A., Strauss, M., Suter, L., Svoisky, P., Titov, M., Tokmenin, V. V., Tsai, Y.-T., Tsybychev, D., Tuchming, B., Tully, C., Uvarov, L., Uvarov, S., Uzunyan, S., Van Kooten, R., van Leeuwen, W. M., Varelas, N., Varnes, E. W., Vasilyev, I. A., Verkheev, A. Y., Vertogradov, L. S., Verzocchi, M., Vesterinen, M., Vilanova, D., Vokac, P., Wahl, H. D., Wang, M. H. L. S., Warchol, J., Watts, G., Wayne, M., Weichert, J., Welty-Rieger, L., Williams, M. R. J., Wilson, G. W., Wobisch, M., Wood, D. R., Wyatt, T. R., Xie, Y., Yamada, R., Yang, S., Yasuda, T., Yatsunenko, Y. A., Ye, W., Ye, Z., Yin, H., Yip, K., Youn, S. W., Yu, J. M., Zennamo, J., Zhao, T. G., Zhou, B., Zhu, J., Zielinski, M., Zieminska, D., Zivkovic, L.
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Abstract/Description: We present evidence for the exotic charged charmoniumlike state Z(c)(+/-)(3900) decaying to J/psi pi(+/-) in semi-inclusive weak decays of b-flavored hadrons. The signal is correlated with a parent J/psi pi(+)pi(-) system in the invariant-mass range 4.2-4.7 GeV that would include the exotic structure Y(4260). The study is based on 10.4 fb(-1) of p (p) over bar collision data collected by the D0 experiment at the Fermilab Tevatron collider.
Date Issued: 2018-09-28
Identifier: FSU_libsubv1_wos_000446281700001, 10.1103/PhysRevD.98.052010
Format: Citation

Title: Symmetry, Maximally Localized Wannier States, And A Low-energy Model For Twisted Bilayer Graphene Narrow Bands.
Creator: Kang, Jian, Vafek, Oskar
Abstract/Description: We build symmetry-adapted maximally localized Wannier states and construct the low-energy tight-binding model for the four narrow bands of twisted bilayer graphene. We do so when the twist angle is commensurate near the "magic" value and the narrow bands are separated from the rest of the bands by energy gaps. On each layer and sublattice, every Wannier state has three peaks near the triangular moire lattice sites. However, each Wannier state is localized and centered around a site of the...
Show moreWe build symmetry-adapted maximally localized Wannier states and construct the low-energy tight-binding model for the four narrow bands of twisted bilayer graphene. We do so when the twist angle is commensurate near the "magic" value and the narrow bands are separated from the rest of the bands by energy gaps. On each layer and sublattice, every Wannier state has three peaks near the triangular moire lattice sites. However, each Wannier state is localized and centered around a site of the honeycomb lattice that is dual to the triangular moire lattice. The space group and the time-reversal symmetries are realized locally. The corresponding tight-binding model provides a starting point for studying the correlated many-body phases.
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Date Issued: 2018-09-28
Identifier: FSU_libsubv1_wos_000446282000002, 10.1103/PhysRevX.8.031088
Format: Citation

Title: The Cow: Discovery Of A Luminous, Hot, And Rapidly Evolving Transient.
Creator: Prentice, S. J., Maguire, K., Smartt, S. J., Magee, M. R., Schady, P., Sim, S., Chen, T.-W., Clark, P., Colin, C., Fulton, M., McBrien, O., O'Neill, D., Smith, K. W., Ashall, C....
Show morePrentice, S. J., Maguire, K., Smartt, S. J., Magee, M. R., Schady, P., Sim, S., Chen, T.-W., Clark, P., Colin, C., Fulton, M., McBrien, O., O'Neill, D., Smith, K. W., Ashall, C., Chambers, K. C., Denneau, L., Flewelling, H. A., Heinze, A., Holoien, T. W.-S., Huber, M. E., Kochanek, C. S., Mazzali, P. A., Prieto, J. L., Rest, A., Shappee, B. J., Stalder, B., Stanek, K. Z., Stritzinger, M. D., Thompson, T. A., Tonry, J. L.
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Abstract/Description: We present the ATLAS discovery and initial analysis of the first 18 days of the unusual transient event, ATLAS18qqn/AT2018cow. It is characterized by a high peak luminosity (similar to 1.7 x 10(44) erg s(-1)),rapidly evolving light curves (>5 mag rise to peak in similar to 3.5 days), and hot blackbody spectra, peaking at similar to 27,000 K that are relatively featureless and unchanging over the first two weeks. The bolometric light curve cannot be powered by radioactive decay under realistic...
Show moreWe present the ATLAS discovery and initial analysis of the first 18 days of the unusual transient event, ATLAS18qqn/AT2018cow. It is characterized by a high peak luminosity (similar to 1.7 x 10(44) erg s(-1)),rapidly evolving light curves (>5 mag rise to peak in similar to 3.5 days), and hot blackbody spectra, peaking at similar to 27,000 K that are relatively featureless and unchanging over the first two weeks. The bolometric light curve cannot be powered by radioactive decay under realistic assumptions. The detection of high-energy emission may suggest a central engine as the powering source. Using a magnetar model, we estimated an ejected mass of 0.1-0.4 M-circle dot, which lies between that of low-energy core-collapse events and the kilonova, AT2017gfo. The spectra cooled rapidly from 27,000 to 15,000 K in just over two weeks but remained smooth and featureless. Broad and shallow emission lines appear after about 20 days, and we tentatively identify them as He I although they would be redshifted from their rest wavelengths. We rule out that there are any features in the spectra due to intermediate mass elements up to and including the Fe group. The presence of r-process elements cannot be ruled out. If these lines are due to He, then we suggest a low-mass star with residual He as a potential progenitor. Alternatively, models of magnetars formed in neutron star mergers, or accretion onto a central compact object, give plausible matches to the data.
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Date Issued: 2018-09-20
Identifier: FSU_libsubv1_wos_000444911400001, 10.3847/2041-8213/aadd90
Format: Citation

Title: Efficient Generation Of Neutral And Charged Biexcitons In Encapsulated Wse2 Monolayers.
Creator: Ye, Ziliang, Waldecker, Lutz, Ma, Eric Yue, Rhodes, Daniel, Antony, Abhinandan, Kim, Bumho, Zhang, Xiao-Xiao, Deng, Minda, Jiang, Yuxuan, Lu, Zhengguang, Smirnov, Dmitry,...
Show moreYe, Ziliang, Waldecker, Lutz, Ma, Eric Yue, Rhodes, Daniel, Antony, Abhinandan, Kim, Bumho, Zhang, Xiao-Xiao, Deng, Minda, Jiang, Yuxuan, Lu, Zhengguang, Smirnov, Dmitry, Watanabe, Kenji, Taniguchi, Takashi, Hone, James, Heinz, Tony F.
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Abstract/Description: Higher-order correlated excitonic states arise from the mutual interactions of excitons, which generally requires a significant exciton density and therefore high excitation levels. Here, we report the emergence of two biexcitons species, one neutral and one charged, in monolayer tungsten diselenide under moderate continuous-wave excitation. The efficient formation of biexcitons is facilitated by the long lifetime of the dark exciton state associated with a spin-forbidden transition, as well...
Show moreHigher-order correlated excitonic states arise from the mutual interactions of excitons, which generally requires a significant exciton density and therefore high excitation levels. Here, we report the emergence of two biexcitons species, one neutral and one charged, in monolayer tungsten diselenide under moderate continuous-wave excitation. The efficient formation of biexcitons is facilitated by the long lifetime of the dark exciton state associated with a spin-forbidden transition, as well as improved sample quality from encapsulation between hexagonal boron nitride layers. From studies of the polarization and magnetic field dependence of the neutral biexciton, we conclude that this species is composed of a bright and a dark excitons residing in opposite valleys in momentum space. Our observations demonstrate that the distinctive features associated with biexciton states can be accessed at low light intensities and excitation densities.
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Date Issued: 2018-09-13
Identifier: FSU_libsubv1_wos_000444494800002, 10.1038/s41467-018-05917-8
Format: Citation

Title: Revealing The Biexciton And Trion-exciton Complexes In Bn Encapsulated Wse2.
Creator: Li, Zhipeng, Wang, Tianmeng, Lu, Zhengguang, Jin, Chenhao, Chen, Yanwen, Meng, Yuze, Lian, Zhen, Taniguchi, Takashi, Watanabe, Kenji, Zhang, Shengbai, Smirnov, Dmitry, Shi, Su-Fei
Abstract/Description: Strong Coulomb interactions in single-layer transition metal dichalcogenides (TMDs) result in the emergence of strongly bound excitons, trions, and biexcitons. These excitonic complexes possess the valley degree of freedom, which can be exploited for quantum optoelectronics. However, in contrast to the good understanding of the exciton and trion properties, the binding energy of the biexciton remains elusive, with theoretical calculations and experimental studies reporting discrepant results....
Show moreStrong Coulomb interactions in single-layer transition metal dichalcogenides (TMDs) result in the emergence of strongly bound excitons, trions, and biexcitons. These excitonic complexes possess the valley degree of freedom, which can be exploited for quantum optoelectronics. However, in contrast to the good understanding of the exciton and trion properties, the binding energy of the biexciton remains elusive, with theoretical calculations and experimental studies reporting discrepant results. In this work, we resolve the conflict by employing low-temperature photoluminescence spectroscopy to identify the biexciton state in BN-encapsulated single-layer WSe2. The biexciton state only exists in charge-neutral WSe2, which is realized through the control of efficient electrostatic gating. In the lightly electron-doped WSe2, one free electron binds to a biexciton and forms the trion-exciton complex. Improved understanding of the biexciton and trion-exciton complexes paves the way for exploiting the many-body physics in TMDs for novel optoelectronics applications.
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Date Issued: 2018-09-13
Identifier: FSU_libsubv1_wos_000444494800003, 10.1038/s41467-018-05863-5
Format: Citation

Title: A Complete Census Of Luminous Stellar Variability On Day To Decade Timescales.
Creator: Conroy, Charlie, Strader, Jay, van Dokkum, Pieter, Dolphin, Andrew E., Weisz, Daniel R., Murphy, Jeremiah W., Dotter, Aaron, Johnson, Benjamin D., Cargile, Phillip
Abstract/Description: Stellar photometric variability offers a novel probe of the interior structure and evolutionary state of stars. Here we present a census of stellar variability on day to decade timescales across the color-magnitude diagram (CMD) for 73,000 stars brighter than M-1,M-814 = 5 in the Whirlpool Galaxy (M51). Our Cycle 24 Hubble Space Telescope (HST) program acquired V-606- and I-814-band images over 34 epochs spanning 1 year with pseudo-random cadences enabling sensitivity to periods from days to...
Show moreStellar photometric variability offers a novel probe of the interior structure and evolutionary state of stars. Here we present a census of stellar variability on day to decade timescales across the color-magnitude diagram (CMD) for 73,000 stars brighter than M-1,M-814 = 5 in the Whirlpool Galaxy (M51). Our Cycle 24 Hubble Space Telescope (HST) program acquired V-606- and I-814-band images over 34 epochs spanning 1 year with pseudo-random cadences enabling sensitivity to periods from days to months. We supplement these data with archival V-and I-band HST data obtained in 1995 and 2005, providing sensitivity to variability on decade timescales. At least 50% of stars brighter than M-1,M-814 = -7 show strong evidence for variability within our Cycle 24 data; among stars with V-606 - I-814 > 2 the variability fraction rises to approximate to 100%. Large amplitude variability (>0.3 mag) on decade timescales is restricted to red supergiants (RSGs) and very luminous blue stars. Both populations display fairly smooth variability on month-year timescales. The Cepheid instability strip is clearly visible in our data, although the variability fraction within this region never exceeds approximate to 10%. The location of variable stars across the CMD broadly agrees with theoretical sources of variability, including the instability strip, RSG pulsational instabilities, long-period fundamental mode pulsations, and radiation-dominated envelopes in massive stars. Our data can be used to place stringent constraints on the precise onset of these various instabilities and their lifetimes and growth rates.
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Date Issued: 2018-09-10
Identifier: FSU_libsubv1_wos_000443836000011, 10.3847/1538-4357/aad460
Format: Citation

Title: Infrared Spectroscopy Of The Merger Candidate Kic 9832227.
Creator: Pavlenko, Ya, Evans, A., Banerjee, D. P. K., Southworth, J., Shahbandeh, M., Davis, S.
Abstract/Description: Context. It has been predicted that the object KIC 9832227 - a contact binary star - will undergo a merger in 2022.2 +/- 0.7. We describe the near-infrared (NIR) spectrum of this object as an impetus to obtain pre-merger data. Aims. We aim to characterise (i) the nature of the individual components of the binary and (ii) the likely circumbinary environment, so that the merger - if and when it occurs - can be interpreted in an informed manner. Methods. We use infrared (IR) spectroscopy in the...
Show moreContext. It has been predicted that the object KIC 9832227 - a contact binary star - will undergo a merger in 2022.2 +/- 0.7. We describe the near-infrared (NIR) spectrum of this object as an impetus to obtain pre-merger data. Aims. We aim to characterise (i) the nature of the individual components of the binary and (ii) the likely circumbinary environment, so that the merger - if and when it occurs - can be interpreted in an informed manner. Methods. We use infrared (IR) spectroscopy in the wavelength range 0.7-2.5 mu m, to which we fit model atmospheres to represent the individual stars. We use the binary ephemeris to determine the orbital phase at the time of observation. Results. We find that the IR spectrum is best fitted by a single component with effective temperature 5920 K, log [g] = 4.1, and solar metallicity, consistent with the fact that the system was observed at conjunction. Conclusions. The strength of the IR H lines is consistent with a high value of log g, and the strength of the Can triplet indicates the presence of a chromosphere, as might be expected from rapid stellar rotation. The He I absorption we observe likely arises in He excited by coronal activity in a circumstellar envelope, suggesting that the weakness of the Can triplet is also likely chromospheric in origin.
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Date Issued: 2018-07-24
Identifier: FSU_libsubv1_wos_000439936700009, 10.1051/0004-6361/201832717
Format: Citation

Title: Measurement Of The Effective Weak Mixing Angle In P(p)over-bar -> Z/gamma* -> L(+) L(-) Events.
Creator: Abazov, V. M., Abbott, B., Acharya, B. S., Adams, M., Adams, T., Agnew, J. P., Alexeev, G. D., Alkhazov, G., Alton, A., Askew, A., Atkins, S., Augsten, K., Aushev, V., Aushev, Y...
Show moreAbazov, V. M., Abbott, B., Acharya, B. S., Adams, M., Adams, T., Agnew, J. P., Alexeev, G. D., Alkhazov, G., Alton, A., Askew, A., Atkins, S., Augsten, K., Aushev, V., Aushev, Y., Avila, C., Badaud, F., Bagby, L., Baldin, B., Bandurin, D. V., Banerjee, S., Barberis, E., Baringer, P., Bartlett, J. F., Bassler, U., Bazterra, V., Bean, A., Begalli, M., Bellantoni, L., Beri, S. B., Bernardi, G., Bernhard, R., Bertram, I., Besancon, M., Beuselinck, R., Bhat, P. C., Bhatia, S., Bhatnagar, V., Blazey, G., Blessing, S., Bloom, K., Boehnlein, A., Boline, D., Boos, E. E., Borissov, G., Borysova, M., Brandt, A., Brandt, O., Brochmann, M., Brock, R., Bross, A., Brown, D., Bu, X. B., Buehler, M., Buescher, V., Bunichev, V., Burdin, S., Buszello, C. P., Camacho-Perez, E., Casey, B. C. K., Castilla-Valdez, H., Caughron, S., Chakrabarti, S., Chan, K. M., Chandra, A., Chapon, E., Chen, G., Cho, S. W., Choi, S., Choudhary, B., Cihangir, S., Claes, D., Clutter, J., Cooke, M., Cooper, W. E., Corcoran, M., Couderc, F., Cousinou, M.-C., Cuth, J., Cutts, D., Das, A., Davies, G., de Jong, S. J., De La Cruz-Burelo, E., Deliot, F., Demina, R., Denisov, D., Denisov, S. P., Desai, S., Deterre, C., DeVaughan, K., Diehl, H. T., Diesburg, M., Ding, P. F., Dominguez, A., Drutskoy, A., Dubey, A., Dudko, L. V., Duperrin, A., Dutt, S., Eads, M., Edmunds, D., Ellison, J., Elvira, V. D., Enari, Y., Evans, H., Evdokimov, A., Evdokimov, V. N., Faure, A., Feng, L., Ferbel, T., Fiedler, F., Filthaut, F., Fisher, W., Fisk, H. E., Fortner, M., Fox, H., Franc, J., Fuess, S., Garbincius, P. H., Garcia-Bellido, A., Garcia-Gonzalez, J. A., Gavrilov, V., Geng, W., Gerber, C. E., Gershtein, Y., Ginther, G., Gogota, O., Golovanov, G., Grannis, P. D., Greder, S., Greenlee, H., Grenier, G., Gris, Ph, Grivaz, J.-F., Grohsjean, A., Grunendahl, S., Grunewald, M. W., Guillemin, T., Gutierrez, G., Gutierrez, P., Haley, J., Han, L., Harder, K., Harel, A., Hauptman, J. M., Hays, J., Head, T., Hebbeker, T., Hedin, D., Hegab, H., Heinson, A. P., Heintz, U., Hensel, C., Heredia-De La Cruz, I., Herner, K., Hesketh, G., Hildreth, M. D., Hirosky, R., Hoang, T., Hobbs, J. D., Hoeneisen, B., Hogan, J., Hohlfeld, M., Holzbauer, J. L., Howley, I., Hubacek, Z., Hynek, V., Iashvili, I., Ilchenko, Y., Illingworth, R., Ito, A. S., Jabeen, S., Jaffre, M., Jayasinghe, A., Jeong, M. S., Jesik, R., Jiang, P., Johns, K., Johnson, E., Johnson, M., Jonckheere, A., Jonsson, P., Joshi, J., Jung, A. W., Juste, A., Kajfasz, E., Karmanov, D., Katsanos, I., Kaur, M., Kehoe, R., Kermiche, S., Khalatyan, N., Khanov, A., Kharchilava, A., Kharzheev, Y. N., Kiselevich, I., Kohli, J. M., Kozelov, A. V., Kraus, J., Kumar, A., Kupco, A., Kurca, T., Kuzmin, V. A., Lammers, S., Lebrun, P., Lee, H. S., Lee, S. W., Lee, W. M., Lei, X., Lellouch, J., Li, D., Li, H., Li, L., Li, Q. Z., Lim, J. K., Lincoln, D., Linnemann, J., Lipaev, V. V., Lipton, R., Liu, H., Liu, Y., Lobodenko, A., Lokajicek, M., de Sa, R. Lopes, Luna-Garcia, R., Lyon, A. L., Maciel, A. K. A., Madar, R., Magana-Villalba, R., Malik, S., Malyshev, V. L., Mansour, J., Martinez-Ortega, J., McCarthy, R., McGivern, C. L., Meijer, M. M., Melnitchouk, A., Menezes, D., Mercadante, P. G., Merkin, M., Meyer, A., Meyer, J., Miconi, F., Mondal, N. K., Mulhearn, M., Nagy, E., Narain, M., Nayyar, R., Neal, H. A., Negret, J. P., Neustroev, P., Nguyen, H. T., Nunnemann, T., Orduna, J., Osman, N., Pal, A., Parashar, N., Parihar, V., Park, S. K., Partridge, R., Parua, N., Patwa, A., Penning, B., Perfilov, M., Peters, Y., Petridis, K., Petrillo, G., Petroff, P., Pleier, M.-A., Podstavkov, V. M., Popov, A. V., Prewitt, M., Price, D., Prokopenko, N., Qian, J., Quadt, A., Quinn, B., Ratoff, P. N., Razumov, I., Ripp-Baudot, I., Rizatdinova, F., Rominsky, M., Ross, A., Royon, C., Rubinov, P., Ruchti, R., Sajot, G., Sanchez-Hernandez, A., Sanders, M. P., Santos, A. S., Savage, G., Savitskyi, M., Sawyer, L., Scanlon, T., Schamberger, R. D., Scheglov, Y., Schellman, H., Schott, M., Schwanenberger, C., Schwienhorst, R., Sekaric, J., Severini, H., Shabalina, E., Shary, V., Shaw, S., Shchukin, A. A., Shkola, O., Simak, V., Skubic, P., Slattery, P., Snow, G. R., Snow, J., Snyder, S., Soldner-Rembold, S., Sonnenschein, L., Soustruznik, K., Stark, J., Stefaniuk, N., Stoyanova, D. A., Strauss, M., Suter, L., Svoisky, P., Titov, M., Tokmenin, V. V., Tsai, Y.-T., Tsybychev, D., Tuchming, B., Tully, C., Uvarov, L., Uvarov, S., Uzunyan, S., Van Kooten, R., van Leeuwen, W. M., Varelas, N., Varnes, E. W., Vasilyev, I. A., Verkheev, A. Y., Vertogradov, L. S., Verzocchi, M., Vesterinen, M., Vilanova, D., Vokac, P., Wahl, H. D., Wang, C., Wang, M. H. L. S., Warchol, J., Watts, G., Wayne, M., Weichert, J., Welty-Rieger, L., Williams, M. R. J., Wilson, G. W., Wobisch, M., Wood, D. R., Wyatt, T. R., Xiang, Y., Xie, Y., Yamada, R., Yang, S., Yasuda, T., Yatsunenko, Y. A., Ye, W., Ye, Z., Yin, H., Yip, K., Youn, S. W., Yu, J. M., Zennamo, J., Zhao, T. G., Zhou, B., Zhu, J., Zielinski, M., Zieminska, D., Zivkovic, L.
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Abstract/Description: We present a measurement of the effective weak mixing angle parameter sin(2)theta(l)(eff) in p (p) over bar -> Z/gamma* -> mu(+)mu(-) events at a center-of-mass energy of 1.96 TeV, collected by the D0 detector at the Fermilab Tevatron Collider and corresponding to 8.6 fb(-1) of integrated luminosity. The measured value of sin(2)theta(l)(eff)[mu mu] = 0.23016 +/- 0.00064 is further combined with the result from the D0 measurement in p (p) over bar -> Z/gamma* -> e(+)e(-) events, resulting in...
Show moreWe present a measurement of the effective weak mixing angle parameter sin(2)theta(l)(eff) in p (p) over bar -> Z/gamma* -> mu(+)mu(-) events at a center-of-mass energy of 1.96 TeV, collected by the D0 detector at the Fermilab Tevatron Collider and corresponding to 8.6 fb(-1) of integrated luminosity. The measured value of sin(2)theta(l)(eff)[mu mu] = 0.23016 +/- 0.00064 is further combined with the result from the D0 measurement in p (p) over bar -> Z/gamma* -> e(+)e(-) events, resulting in sin(2)theta(l)(eff)[comb] = 0.23095 +/- 0.00040. This combined result is the most precise measurement from a single experiment at a hadron collider and is the most precise determination using the coupling of the Z/gamma* to light quarks.
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Date Issued: 2018-06-13
Identifier: FSU_libsubv1_wos_000435081500002, 10.1103/PhysRevLett.120.241802
Format: Citation

Title: Evidence For Ferromagnetic Clusters In The Colossal-magnetoresistance Material Eub6.
Creator: Pohlit, Merlin, Roessler, Sahana, Ohno, Yuzo, Ohno, Hideo, von Molnar, Stephan, Fisk, Zachary, Mueller, Jens, Wirth, Steffen
Abstract/Description: We combined scanning tunneling microscopy and locally resolved magnetic stray field measurements on the ferromagnetic semimetal EuB6, which exhibits a complex ferromagnetic order and a colossal magnetoresistance effect. In a zero magnetic field, scanning tunneling spectroscopy visualizes the existence of local inhomogeneities in the electronic density of states, which we interpret as the localization of charge carriers due to the formation of magnetic polarons. Micro-Hall magnetometry...
Show moreWe combined scanning tunneling microscopy and locally resolved magnetic stray field measurements on the ferromagnetic semimetal EuB6, which exhibits a complex ferromagnetic order and a colossal magnetoresistance effect. In a zero magnetic field, scanning tunneling spectroscopy visualizes the existence of local inhomogeneities in the electronic density of states, which we interpret as the localization of charge carriers due to the formation of magnetic polarons. Micro-Hall magnetometry measurements of the total stray field emanating from the end of a rectangular-shaped platelike sample reveals evidence for magnetic clusters also in finite magnetic fields. In contrast, the signal detected below the faces of the magnetized sample measures a local stray field indicating the formation of pronounced magnetic inhomogeneities consistent with large clusters of percolated magnetic polarons.
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Date Issued: 2018-06-19
Identifier: FSU_libsubv1_wos_000435551200004, 10.1103/PhysRevLett.120.257201
Format: Citation

Title: Search For Natural And Split Supersymmetry In Proton-proton Collisions At Root S=13 Tev In Final States With Jets And Missing Transverse Momentum.
Creator: Sirunyan, A. M., Tumasyan, A., Adam, W., Ambrogi, F., Asilar, E., Bergauer, T., Brandstetter, J., Brondolin, E., Dragicevic, M., Eroe, J., Del Valle, A. Escalante, Flechl, M.,...
Show moreSirunyan, A. M., Tumasyan, A., Adam, W., Ambrogi, F., Asilar, E., Bergauer, T., Brandstetter, J., Brondolin, E., Dragicevic, M., Eroe, J., Del Valle, A. Escalante, Flechl, M., Friedl, M., Friedl, M., Fruehwirth, R., Ghete, V. M., Grossmann, J., Hrubec, J., Jeitler, M., Koenig, A., Krammer, N., Kraetschmer, I., Liko, D., Madlener, T., Mikulec, I., Pree, E., Rad, N., Rohringer, H., Schieck, J., Schoefbeck, R., Spanring, M., Spitzbart, D., Taurok, A., Waltenberger, W., Wittmann, J., Wulz, C.-E., Zarucki, M., Chekhovsky, V., Mossolov, V., Gonzalez, J. Suarez, De Wolf, E. A., Di Croce, D., Janssen, X., Lauwers, J., Pieters, M., Van de Klundert, M., Van Haevermaet, H., Van Mechelen, P., Van Remortel, N., Abu Zeid, S., Blekman, F., D'Hondt, J., De Bruyn, I., De Clercq, J., Deroover, K., Flouris, G., Lontkovskyi, D., Lowette, S., Marchesini, I., Moortgat, S., Moreels, L., Python, Q., Skovpen, K., Tavernier, S., Van Doninck, W., Van Mulders, P., Van Parijs, I., Beghin, D., Bilin, B., Brun, H., Clerbaux, B., De Lentdecker, G., Delannoy, H., Dorney, B., Fasanella, G., Favart, L., Goldouzian, R., Grebenyuk, A., Kalsi, A. K., Lenzi, T., Luetic, J., Seva, T., Starling, E., Vander Velde, C., Vanlaer, P., Vannerom, D., Yonamine, R., Cornelis, T., Dobur, D., Fagot, A., Gul, M., Khvastunov, I., Poyraz, D., Roskas, C., Trocino, D., Tytgat, M., Verbeke, W., Vermassen, B., Vit, M., Zaganidis, N., Bakhshiansohi, H., Bondu, O., Brochet, S., Bruno, G., Caputo, C., Caudron, A., David, P., De Visscher, S., Delaere, C., Delcourt, M., Francois, B., Giammanco, A., Krintiras, G., Lemaitre, V., Magitteri, A., Mertens, A., Musich, M., Piotrzkowski, K., Quertenmont, L., Saggio, A., Marono, M. Vidal, Wertz, S., Zobec, J., Alda Junior, W. L., Alves, F. L., Alves, G. A., Brito, L., Correia Silva, G., Hensel, C., Moraes, A., Pol, M. E., Rebello Teles, P., Belchior Batista Das Chagas, E., Carvalho, W., Chinellato, J., Coelho, E., Da Costa, E. M., Da Silveira, G. G., De Jesus Damiao, D., Fonseca De Souza, S., Huertas Guativa, L. M., Malbouisson, H., Medina Jaime, M., Melo De Almeida, M., Mora Herrera, C., Mundim, L., Nogima, H., Sanchez Rosas, L. J., Santoro, A., Sznajder, A., Thiel, M., Tonelli Manganote, E. J., Torres Da Silva De Araujo, F., Vilela Pereira, A., Ahuja, S., Bernardes, C. A., Calligaris, L., Fernandez Perez Tomei, T. R., Gregores, E. M., Mercadante, P. G., Novaes, S. F., Padula, Sandra S., Romero Abad, D., Ruiz Vargas, J. C., Aleksandrov, A., Hadjiiska, R., Iaydjiev, P., Marinov, A., Misheva, M., Rodozov, M., Shopova, M., Sultanov, G., Dimitrov, A., Litov, L., Pavlov, B., Petkov, P., Fang, W., Gao, X., Yuan, L., Ahmad, M., Bian, J. G., Chen, G. M., Chen, H. S., Chen, M., Chen, Y., Jiang, C. H., Leggat, D., Liao, H., Liu, Z., Romeo, F., Shaheen, S. M., Spiezia, A., Tao, J., Wang, C., Wang, Z., Yazgan, E., Zhang, H., Zhao, J., Ban, Y., Chen, G., Li, J., Li, Q., Liu, S., Mao, Y., Qian, S. J., Wang, D., Xu, Z., Wang, Y., Avila, C., Cabrera, A., Carrillo Montoya, C. A., Chaparro Sierra, L. F., Florez, C., Gonzalez Hernandez, C. F., Segura Delgado, M. A., Courbon, B., Godinovic, N., Lelas, D., Puljak, I., Ribeiro Cipriano, P. M., Sculac, T., Antunovic, Z., Kovac, M., Brigljevic, V., Ferencek, D., Kadija, K., Mesic, B., Starodumov, A., Susa, T., Ather, M. W., Attikis, A., Mavromanolakis, G., Mousa, J., Nicolaou, C., Ptochos, F., Razis, P. A., Rykaczewski, H., Finger, M., Finger, M., Carrera Jarrin, E., Abdelalim, A. A., El-khateeb, E., Khalil, S., Bhowmik, S., Dewanjee, R. K., Kadastik, M., Perrini, L., Raidal, M., Veelken, C., Eerola, P., Kirschenmann, H., Pekkanen, J., Voutilainen, M., Havukainen, J., Heikkila, J. K., Jarvinen, T., Karimaki, V., Kinnunen, R., Lampen, T., Lassila-Perini, K., Laurila, S., Lehti, S., Linden, T., Luukka, P., Maenapaa, T., Siikonen, H., Tuominen, E., Tuominiemi, J., Tuuva, T., Besancon, M., Couderc, F., Dejardin, M., Denegri, D., Faure, J. L., Ferri, F., Ganjour, S., Ghosh, S., Givernaud, A., Gras, P., de Monchenault, G. Hamel, Jarry, P., Leloup, C., Locci, E., Machet, M., Malcles, J., Negro, G., Rander, J., Rosowsky, A., Sahin, M. O., Titov, M., Abdulsalam, A., Amendola, C., Antropov, I., Baffioni, S., Beaudette, F., Busson, P., Cadamuro, L., Charlot, C., de Cassagnac, R. Granier, Jo, M., Kucher, I., Lisniak, S., Lobanov, A., Blanco, J. Martin, Nguyen, M., Ochando, C., Ortona, G., Paganini, P., Pigard, P., Salerno, R., Sauvan, J. B., Sirois, Y., Leiton, A. G. Stahl, Yilmaz, Y., Zabi, A., Zghiche, A., Agram, J.-L., Andrea, J., Bloch, D., Brom, J.-M., Buttignol, M., Chabert, E. C., Collard, C., Conte, E., Coubez, X., Drouhin, F., Fontaine, J.-C., Gele, D., Goerlach, U., Jansova, M., Juillot, P., Le Bihan, A.-C., Tonon, N., Van Hove, P., Gadrat, S., Beauceron, S., Bernet, C., Boudoul, G., Chanon, N., Chierici, R., Contardo, D., Depasse, P., El Mamouni, H., Fay, J., Finco, L., Gascon, S., Gouzevitch, M., Grenier, G., Ille, B., Lagarde, F., Laktineh, I. B., Lattaud, H., Lethuillier, M., Mirabito, L., Pequegnot, A. L., Perries, S., Popov, A., Sordini, V., Donckt, M. Vander, Viret, S., Zhang, S., Toriashvili, T., Tsamalaidze, Z., Autermann, C., Feld, L., Kiesel, M. K., Klein, K., Lipinski, M., Preuten, M., Schomakers, C., Schulz, J., Teroerde, M., Wittmer, B., Zhukov, V., Albert, A., Duchardt, D., Endres, M., Erdmann, M., Erdweg, S., Esch, T., Fischer, R., Gueth, A., Hebbeker, T., Heidemann, C., Hoepfner, K., Knutzen, S., Merschmeyer, M., Meyer, A., Millet, P., Mukherjee, S., Pook, T., Radziej, M., Reithler, H., Rieger, M., Scheuch, F., Teyssier, D., Thuer, S., Fluegge, G., Kargoll, B., Kress, T., Kuensken, A., Mueller, T., Nehrkorn, A., Nowack, A., Pistone, C., Pooth, O., Stahl, A., Martin, M. Aldaya, Arndt, T., Asawatangtrakuldee, C., Beernaert, K., Behnke, O., Behrens, U., Martinez, A. Bermudez, Bin Anuar, A. A., Borras, K., Botta, V., Campbell, A., Connor, P., Contreras-Campana, C., Costanza, F., Danilov, V., De Wit, A., Pardos, C. Diez, Damiani, D. Dominguez, Eckerlin, G., Eckstein, D., Eichhorn, T., Eren, E., Gallo, E., Garcia, J. Garay, Geiser, A., Luyando, J. M. Grados, Grohsjean, A., Gunnellini, P., Guthoff, M., Harb, A., Hauk, J., Hempel, M., Jung, H., Kasemann, M., Keaveney, J., Kleinwort, C., Knolle, J., Korol, I., Kruecker, D., Lange, W., Lelek, A., Lenz, T., Lipka, K., Lohmann, W., Mankel, R., Melzer-Pellmann, I.-A., Meyer, A. B., Meyer, M., Missiroli, M., Mittag, G., Mnich, J., Mussgiller, A., Pitzl, D., Raspereza, A., Savitskyi, M., Saxena, P., Shevchenko, R., Stefaniuk, N., Tholen, H., Van Onsem, G. P., Walsh, R., Wen, Y., Wichmann, K., Wissing, C., Zenaiev, O., Aggleton, R., Bein, S., Blobel, V., Vignali, M. 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R., Negrete, M. Olmedo, Paneva, M. I., Si, W., Wang, L., Wei, H., Wimpenny, S., Yates, B. R., Branson, J. G., Cittolin, S., Derdzinski, M., Gerosa, R., Gilbert, D., Hashemi, B., Holzner, A., Klein, D., Kole, G., Krutelyov, V., Letts, J., Masciovecchio, M., Olivito, D., Padhi, S., Pieri, M., Sani, M., Sharma, V., Simon, S., Tadel, M., Vartak, A., Wasserbaech, S., Wood, J., Wurthwein, F., Yagil, A., Della Porta, G. Zevi, Amin, N., Bhandari, R., Bradmiller-Feld, J., Campagnari, C., Citron, M., Dishaw, A., Dutta, V., Sevilla, M. Franco, Gouskos, L., Heller, R., Incandela, J., Ovcharova, A., Qu, H., Richman, J., Stuart, D., Suarez, I., Yoo, J., Anderson, D., Bornheim, A., Bunn, J., Lawhorn, J. M., Newman, H. B., Nguyen, T. Q., Pena, C., Spiropulu, M., Vlimant, J. R., Wilkinson, R., Xie, S., Zhang, Z., Zhu, R. Y., Andrews, M. B., Ferguson, T., Mudholkar, T., Paulini, M., Russ, J., Sun, M., Vogel, H., Vorobiev, I., Weinberg, M., Cumalat, J. P., Ford, W. T., Jensen, F., Johnson, A., Krohn, M., Leontsinis, S., MacDonald, E., Mulholland, T., Stenson, K., Ulmer, K. A., Wagner, S. R., Alexander, J., Chaves, J., Cheng, Y., Chu, J., Datta, A., Mcdermott, K., Mirman, N., Patterson, J. R., Quach, D., Rinkevicius, A., Ryd, A., Skinnari, L., Ffi, L. So, Tan, S. M., Tao, Z., Thom, J., Tucker, J., Wittich, P., Zientek, M., Abdullin, S., Albrow, M., Alyari, M., Apollinari, G., Apresyan, A., Apyan, A., Banerjee, S., Bauerdick, L. A. T., Beretvas, A., Berryhill, J., Bhat, P. C., Bolla, G., Burkett, K., Butler, J. N., Canepa, A., Cerati, G. B., Cheung, H. W. K., Chlebana, F., Cremonesi, M., Duarte, J., Elvira, V. D., Freeman, J., Gecse, Z., Gottschalk, E., Gray, L., Green, D., Grunendahl, S., Gutsche, O., Hanlon, J., Harris, R. M., Hasegawa, S., Hirschauer, J., Hu, Z., Jayatilaka, B., Jindariani, S., Johnson, M., Joshi, U., Klima, B., Kortelainen, M. J., Kreis, B., Lammel, S., Lincoln, D., Lipton, R., Liu, M., Liu, T., De Sa, R. Lopes, Lykken, J., Maeshima, K., Magini, N., No, J. M. Marra Ffi, Mason, D., McBride, P., Merkel, P., Mrenna, S., Nahn, S., O'Dell, V., Pedro, K., Prokofyev, O., Rakness, G., Ristori, L., Savoy-Navarro, A., Schneider, B., Sexton-Kennedy, E., Soha, A., Spalding, W. J., Spiegel, L., Stoynev, S., Strait, J., Strobbe, N., Taylor, L., Tkaczyk, S., Tran, N. V., Uplegger, L., Vaandering, E. W., Vernieri, C., Verzocchi, M., Vidal, R., Wang, M., Weber, H. A., Whitbeck, A., Wu, W., Acosta, D., Avery, P., Bortignon, P., Bourilkov, D., Brinkerhoff, A., Carnes, A., Carver, M., Curry, D., Field, R. D., Furic, I. K., Gleyzer, S. V., Joshi, B. M., Konigsberg, J., Korytov, A., Kotov, K., Ma, P., Matchev, K., Mei, H., Mitselmakher, G., Shi, K., Sperka, D., Terentyev, N., Thomas, L., Wang, J., Wang, S., Yelton, J., Joshi, Y. R., Linn, S., Markowitz, P., Rodriguez, J. L., Ackert, A., Adams, T., Askew, A., Hagopian, S., Hagopian, V., Johnson, K. F., Kolberg, T., Martinez, G., Perry, T., Prosper, H., Saha, A., Santra, A., Sharma, V., Yohay, R., Baarmand, M. M., Bhopatkar, V., Colafranceschi, S., Hohlmann, M., Noonan, D., Roy, T., Yumiceva, F., Adams, M. R., Apanasevich, L., Berry, D., Betts, R. R., Cavanaugh, R., Chen, X., Dittmer, S., Evdokimov, O., Gerber, C. E., Hangal, D. A., Hofman, D. J., Jung, K., Kamin, J., Gonzalez, I. D. Sandoval, Tonjes, M. B., Varelas, N., Wang, H., Wu, Z., Zhang, J., Bilki, B., Clarida, W., Dilsiz, K., Durgut, S., Gandrajula, R. P., Haytmyradov, M., Khristenko, V., Merlo, J.-P., Mermerkaya, H., Mestvirishvili, A., Moeller, A., Nachtman, J., Ogul, H., Onel, Y., Ozok, F., Penzo, A., Snyder, C., Tiras, E., Wetzel, J., Yi, K., Blumenfeld, B., Cocoros, A., Eminizer, N., Fehling, D., Feng, L., Gritsan, A. V., Maksimovic, P., Roskes, J., Sarica, U., Swartz, M., Xiao, M., You, C., Al-bataineh, A., Baringer, P., Bean, A., Boren, S., Bowen, J., Castle, J., Khalil, S., Kropivnitskaya, A., Majumder, D., Mcbrayer, W., Murray, M., Rogan, C., Royon, C., Sanders, S., Schmitz, E., Takaki, J. D. Tapia, Wang, Q., Ivanov, A., Kaadze, K., Maravin, Y., Modak, A., Mohammadi, A., Saini, L. K., Skhirtladze, N., Rebassoo, F., Wright, D., Baden, A., Baron, O., Belloni, A., Eno, S. C., Feng, Y., Ferraioli, C., Hadley, N. J., Jabeen, S., Jeng, G. Y., Kellogg, R. G., Kunkle, J., Mignerey, A. C., Ricci-Tam, F., Shin, Y. H., Skuja, A., Tonwar, S. C., Abercrombie, D., Allen, B., Azzolini, V., Barbieri, R., Baty, A., Bauer, G., Bi, R., Brandt, S., Busza, W., Cali, I. A., D'Alfonso, M., Demiragli, Z., Ceballos, G. Gomez, Goncharov, M., Harris, P., Hsu, D., Hu, M., Iiyama, Y., Innocenti, G. M., Klute, M., Kovalskyi, D., Lee, Y.-J., Levin, A., Luckey, P. D., Maier, B., Marini, A. C., Mcginn, C., Mironov, C., Narayanan, S., Niu, X., Paus, C., Roland, C., Roland, G., Stephans, G. S. F., Sumorok, K., Tatar, K., Velicanu, D., Wang, J., Wang, T. W., Wyslouch, B., Zhaozhong, S., Benvenuti, A. C., Chatterjee, R. M., Evans, A., Hansen, P., Kalafut, S., Kubota, Y., Lesko, Z., Mans, J., Nourbakhsh, S., Ruckstuhl, N., Rusack, R., Turkewitz, J., Wadud, M. A., Acosta, J. G., Oliveros, S., Avdeeva, E., Bloom, K., Claes, D. R., Fangmeier, C., Golf, F., Suarez, R. Gonzalez, Kamalieddin, R., Kravchenko, I., Monroy, J., Siado, J. E., Snow, G. R., Stieger, B., Dolen, J., Godshalk, A., Harrington, C., Iashvili, I., Nguyen, D., Parker, A., Rappoccio, S., Roozbahani, B., Alverson, G., Barberis, E., Freer, C., Hortiangtham, A., Massironi, A., Morse, D. M., Orimoto, T., De Lima, R. Teixeira, Wamorkar, T., Wang, B., Wisecarver, A., Wood, D., Bhattacharya, S., Charaf, O., Hahn, K. A., Mucia, N., Odell, N., Schmitt, M. H., Sung, K., Trovato, M., Velasco, M., Bucci, R., Dev, N., Hildreth, M., Anampa, K. Hurtado, Jessop, C., Karmgard, D. J., Kellams, N., Lannon, K., Li, W., Loukas, N., Marinelli, N., Meng, F., Mueller, C., Musienko, Y., Planer, M., Reinsvold, A., Ruchti, R., Siddireddy, P., Smith, G., Taroni, S., Wayne, M., Wightman, A., Wolf, M., Woodard, A., Alimena, J., Antonelli, L., Bylsma, B., Durkin, L. S., Flowers, S., Francis, B., Hart, A., Hill, C., Ji, W., Ling, T. Y., Luo, W., Winer, B. L., Wulsin, H. W., Cooperstein, S., Driga, O., Elmer, P., Hardenbrook, J., Hebda, P., Higginbotham, S., Kalogeropoulos, A., Lange, D., Luo, J., Marlow, D., Mei, K., Ojalvo, I., Olsen, J., Palmer, C., Piroue, P., Salfeld-Nebgen, J., Stickland, D., Tully, C., Malik, S., Norberg, S., Barker, A., Barnes, V. E., Das, S., Gutay, L., Jones, M., Jung, A. W., Khatiwada, A., Miller, D. H., Neumeister, N., Peng, C. C., Qiu, H., Schulte, J. F., Sun, J., Wang, F., Xiao, R., Xie, W., Cheng, T., Parashar, N., Chen, Z., Ecklund, K. M., Freed, S., Geurts, F. J. M., Guilbaud, M., Kilpatrick, M., Li, W., Michlin, B., Padley, B. P., Roberts, J., Rorie, J., Shi, W., Tu, Z., Zabel, J., Zhang, A., Bodek, A., de Barbaro, P., Demina, R., Duh, Y. T., Ferbel, T., Galanti, M., Garcia-Bellido, A., Han, J., Hindrichs, O., Khukhunaishvili, A., Lo, K. H., Tan, P., Verzetti, M., Ciesielski, R., Goulianos, K., Mesropian, C., Agapitos, A., Chou, J. P., Gershtein, Y., Espinosa, T. A. Gomez, Halkiadakis, E., Heindl, M., Hughes, E., Kaplan, S., Elayavalli, R. Kunnawalkam, Kyriacou, S., Lath, A., Montalvo, R., Nash, K., Osherson, M., Saka, H., Salur, S., Schnetzer, S., Eld, D. She Ffi, Somalwar, S., Stone, R., Thomas, S., Thomassen, P., Walker, M., Delannoy, A. G., Heideman, J., Riley, G., Rose, K., Spanier, S., Thapa, K., Bouhali, O., Hernandez, A. Castaneda, Celik, A., Dalchenko, M., De Mattia, M., Delgado, A., Dildick, S., Eusebi, R., Gilmore, J., Huang, T., Kamon, T., Mueller, R., Pakhotin, Y., Patel, R., Perloff, A., Pernie, L., Rathjens, D., Safonov, A., Tatarinov, A., Akchurin, N., Damgov, J., De Guio, F., Dudero, P. R., Faulkner, J., Gurpinar, E., Kunori, S., Lamichhane, K., Lee, S. W., Mengke, T., Muthumuni, S., Peltola, T., Undleeb, S., Volobouev, I., Wang, Z., Greene, S., Gurrola, A., Janjam, R., Johns, W., Maguire, C., Melo, A., Ni, H., Padeken, K., Alvarez, J. D. Ruiz, Sheldon, P., Tuo, S., Velkovska, J., Xu, Q., Arenton, M. W., Barria, P., Cox, B., Hirosky, R., Joyce, M., Ledovskoy, A., Li, H., Neu, C., Sinthuprasith, T., Wang, Y., Wolfe, E., Xia, F., Harr, R., Karchin, P. E., Poudyal, N., Sturdy, J., Thapa, P., Zaleski, S., Brodski, M., Buchanan, J., Caillol, C., Carlsmith, D., Dasu, S., Dodd, L., Duric, S., Gomber, B., Grothe, M., Herndon, M., Herve, A., Hussain, U., Klabbers, P., Lanaro, A., Levine, A., Long, K., Loveless, R., Rekovic, V., Ruggles, T., Savin, A., Smith, N., Smith, W. H., Woods, N.
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Abstract/Description: A search for supersymmetry (SUSY) is performed in final states comprising one or more jets and missing transverse momentum using data from proton-proton collisions at a centre-of-mass energy of 13 TeV. The data were recorded with the CMS detector at the CERN LHC in 2016 and correspond to an integrated luminosity of 35.9 fb(-1). The number of signal events is found to agree with the expected background yields from standard model processes. The results are interpreted in the context of...
Show moreA search for supersymmetry (SUSY) is performed in final states comprising one or more jets and missing transverse momentum using data from proton-proton collisions at a centre-of-mass energy of 13 TeV. The data were recorded with the CMS detector at the CERN LHC in 2016 and correspond to an integrated luminosity of 35.9 fb(-1). The number of signal events is found to agree with the expected background yields from standard model processes. The results are interpreted in the context of simplified models of SUSY that assume the production of gluino or squark pairs and their prompt decay to quarks and the lightest neutralino. The masses of bottom, top, and mass-degenerate light-flavour squarks are probed up to 1050, 1000, and 1325 GeV, respectively. The gluino mass is probed up to 1900, 1650, and 1650 GeV when the gluino decays via virtual states of the aforementioned squarks. The strongest mass bounds on the neutralinos from gluino and squark decays are 1150 and 575 GeV, respectively. The search also provides sensitivity to simplified models inspired by split SUSY that involve the production and decay of long-lived gluinos. Values of the proper decay length CT0 from 10(-3) to 10(5) mm are considered, as well as a metastable gluino scenario. Gluino masses up to 1750 and 900 GeV are probed for CT0 = 1mm and for the metastable state, respectively. The sensitivity is moderately dependent on model assumptions for CT0 greater than or similar to 1 m. The search provides coverage of the CT0 parameter space for models involving long-lived gluinos that is complementary to existing techniques at the LHC.
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Date Issued: 2018-05-04
Identifier: FSU_libsubv1_wos_000432560700001, 10.1007/JHEP05(2018)025
Format: Citation

Title: Sn 2012fr: Ultraviolet, Optical, And Near-infrared Light Curves Of A Type Ia Supernova Observed Within A Day Of Explosion.
Creator: Contreras, Carlos, Phillips, M. M., Burns, Christopher R., Piro, Anthony L., Shappee, B. J., Stritzinger, Maximilian D., Baltay, C., Brown, Peter J., Conseil, Emmanuel, Klotz,...
Show moreContreras, Carlos, Phillips, M. M., Burns, Christopher R., Piro, Anthony L., Shappee, B. J., Stritzinger, Maximilian D., Baltay, C., Brown, Peter J., Conseil, Emmanuel, Klotz, Alain, Nugent, Peter E., Turpin, Damien, Parker, Stu, Rabinowitz, D., Hsiao, Eric Y., Morrell, Nidia, Campillay, Abdo, Castellon, Sergio, Corco, Carlos, Gonzalez, Consuelo, Krisciunas, Kevin, Seron, Jacqueline, Tucker, Brad E., Walker, E. S., Baron, E., Cain, C., Childress, Michael J., Folatelli, Gaston, Freedman, Wendy L., Hamuy, Mario, Hoeflich, P., Persson, S. E., Scalzo, Richard, Schmidt, Brian, Suntzeff, Nicholas B.
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Abstract/Description: We present detailed ultraviolet, optical, and near-infrared light curves of the Type Ia supernova (SN) 2012fr, which exploded in the Fornax cluster member NGC 1365. These precise high-cadence light curves provide a dense coverage of the flux evolution from -12 to +140 days with respect to the epoch of B-band maximum (t(Bmax)). Supplementary imaging at the earliest epochs reveals an initial slow and nearly linear rise in luminosity with a duration of similar to 2.5 days, followed by a faster...
Show moreWe present detailed ultraviolet, optical, and near-infrared light curves of the Type Ia supernova (SN) 2012fr, which exploded in the Fornax cluster member NGC 1365. These precise high-cadence light curves provide a dense coverage of the flux evolution from -12 to +140 days with respect to the epoch of B-band maximum (t(Bmax)). Supplementary imaging at the earliest epochs reveals an initial slow and nearly linear rise in luminosity with a duration of similar to 2.5 days, followed by a faster rising phase that is well reproduced by an explosion model with a moderate amount of Ni-56 mixing in the ejecta. From our analysis of the light curves, we conclude that: (i) the explosion occurred <22 hr before the first detection of the supernova, (ii) the rise time to peak bolometric (lambda > 1800 angstrom) luminosity was 16.5 +/- 0.6 days, (iii) the supernova suffered little or no host-galaxy dust reddening, (iv) the peak luminosity in both the optical and near-infrared was consistent with the bright end of normal Type Ia diversity, and (v) 0.60 +/- 0.15 M-circle dot of Ni-56 was synthesized in the explosion. Despite its normal luminosity, SN 2012fr displayed unusually prevalent high-velocity Ca II and Si II absorption features, and a nearly constant photospheric velocity of the Si II lambda 6355 line at similar to 12,000 km s(-1) that began similar to 5 days before t(Bmax) We also highlight some of the other peculiarities in the early phase photometry and the spectral evolution. SN 2012fr also adds to a growing number of Type Ia supernovae that are hosted by galaxies with direct Cepheid distance measurements.
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Date Issued: 2018-05-20
Identifier: FSU_libsubv1_wos_000432487700002, 10.3847/1538-4357/aabaf8
Format: Citation

Title: On The Type Ia Supernovae 2007on And 2011iv: Evidence For Chandrasekhar-mass Explosions At The Faint End Of The Luminosity-width Relationship.
Creator: Ashall, C., Mazzali, P. A., Stritzinger, M. D., Hoeflich, P., Burns, C. R., Gall, C., Hsiao, E. Y., Phillips, M. M., Morrell, N., Foley, Ryan J.
Abstract/Description: Radiative transfer models of two transitional type Ia supernova (SNe Ia) have been produced using the abundance stratification technique. These two objects - designated SN 2007on and SN 2011iv - both exploded in the same galaxy, NGC 1404, which allows for a direct comparison. SN 2007on synthesised 0.25 M-circle dot of Ni-56 and was less luminous than SN 2011iv, which produced 0.31 M-circle dot of Ni-56. SN 2007on had a lower central density (rho(c)) and higher explosion energy (E-kin similar...
Show moreRadiative transfer models of two transitional type Ia supernova (SNe Ia) have been produced using the abundance stratification technique. These two objects - designated SN 2007on and SN 2011iv - both exploded in the same galaxy, NGC 1404, which allows for a direct comparison. SN 2007on synthesised 0.25 M-circle dot of Ni-56 and was less luminous than SN 2011iv, which produced 0.31 M-circle dot of Ni-56. SN 2007on had a lower central density (rho(c)) and higher explosion energy (E-kin similar to 1.3 +/- 0.3x10(51)erg) than SN 2011iv, and it produced less nuclear statistical equilibrium (NSE) elements (0.06 M-circle dot). Whereas, SN 2011iv had a larger rho(c), which increased the electron capture rate in the lowest velocity regions, and produced 0.35 M-circle dot of stable NSE elements. SN 2011iv had an explosion energy of similar to E-kin similar to 0.9 +/- 0.2x10(51)erg. Both objects had an ejecta mass consistent with the Chandrasekhar mass (Ch-mass), and their observational properties are well described by predictions from delayed-detonation explosion models. Within this framework, comparison to the sub-luminous SN 1986G indicates SN 2011iv and SN 1986G have different transition densities (rho(tr)) but similar rho(c). Whereas, SN 1986G and SN 2007on had a similar rho(tr) but different rho(c). Finally, we examine the colour-stretch parameter sBV vs. L-max relation and determine that the bulk of SNe Ia (including the sub-luminous ones) are consistent with Ch-mass delayed-detonation explosions, where the main parameter driving the diversity is rho(tr). We also find rho(c) to be driving the second order scatter observed at the faint end of the luminosity-width relationship.
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Date Issued: 2018-06-01
Identifier: FSU_libsubv1_wos_000432660300012, 10.1093/mnras/sty632
Format: Citation

Title: Measurement Of Quarkonium Production Cross Sections In Pp Collisions At Root S=13 Tev.
Creator: Sirunyan, A. M., Tumasyan, A., Adam, W., Ambrogi, F., Asilar, E., Bergauer, T., Brandstetter, J., Brondolin, E., Dragicevic, M., Eroe, J., Flechl, M., Friedl, M., Fruehwirth, R....
Show moreSirunyan, A. M., Tumasyan, A., Adam, W., Ambrogi, F., Asilar, E., Bergauer, T., Brandstetter, J., Brondolin, E., Dragicevic, M., Eroe, J., Flechl, M., Friedl, M., Fruehwirth, R., Ghete, V. M., Grossmann, J., Hrubec, J., Jeitler, M., Koenig, A., Krammer, N., Kraetschmer, I., Liko, D., Madlener, T., Mikulec, I., Pree, E., Rabady, D., Rad, N., Rohringer, H., Schieck, J., Schoefbeck, R., Spanring, M., Spitzbart, D., Waltenberger, W., Wittmann, J., Wulz, C.-E., Zarucki, M., Chekhovsky, V., Mossolov, V., Gonzalez, J. Suarez, De Wolf, E. A., Di Croce, D., Janssen, X., Lauwers, J., Van de Klundert, M., Van Haevermaet, H., Van Mechelen, R., Van Remortel, N., Abu Zeid, S., Blekman, F., D'Hondt, J., De Bruyn, I., De Clercq, J., Deroover, K., Flouris, G., Lontkovskyi, D., Lowette, S., Moortgat, S., Moreels, L., Python, Q., Skovpen, K., Tavernier, S., Van Doninck, W., Van Mulders, R., Van Parijs, I., Brun, H., Clerbaux, B., De Lentdecker, G., Delannoy, H., Fasanella, G., Favart, L., Goldouzian, R., Grebenyuk, A., Karapostoli, G., Lenzi, T., Luetic, J., Maerschalk, T., Marinov, A., Randle-conde, A., Seva, T., Velde, C. Vander, Vanlaer, R., Vannerom, D., Yonamine, R., Zenoni, F., Zhang, F., Cimmino, A., Cornelis, T., Dobur, D., Fagot, A., Gul, M., Khvastunov, I., Poyraz, D., Roskas, C., Salva, S., Tytgat, M., Verbeke, W., Zaganidis, N., Bakhshiansohi, H., Bondu, O., Brochet, S., Bruno, G., Caputo, C., Caudron, A., De Visscher, S., Delaere, C., Delcourt, M., Francois, B., Giammanco, A., Jafari, A., Komm, M., Krintiras, G., Lemaitre, V., Magitteri, A., Mertens, A., Musich, M., Piotrzkowski, K., Quertenmont, L., Marono, M. Vidal, Wertz, S., Beliy, N., Alda Junior, W. L., Alves, F. L., Alves, G. A., Brito, L., Correa Martins Junior, M., Hensel, C., Moraes, A., Pol, M. E., Rebello Teles, R., Belchior Batista Das Chagas, E., Carvalho, W., Chinellato, J., Custodio, A., Da Costa, E. M., Da Silveira, G. G., De Jesus Damiao, D., Fonseca De Souza, S., Huertas Guativa, L. M., Malbouisson, H., Melo De Almeida, M., Mora Herrera, C., Mundim, L., Nogima, H., Santoro, A., Sznajder, A., Tonelli Manganote, E. J., Torres Da Silva De Araujo, F., Vilela Pereira, A., Ahuja, S., Bernardes, C. A., Fernandez Perez Tomei, T. R., Gregores, E. M., Mercadante, P. G., Novaes, S. F., Padula, Sandra S., Romero Abad, D., Ruiz Vargas, J. C., Aleksandrov, A., Hadjiiska, R., Iaydjiev, R., Misheva, M., Rodozov, M., Shopova, M., Stoykova, S., Sultanov, G., Dimitrov, A., Glushkov, I., Litov, L., Pavlov, B., Petkov, R., Fang, W., Gao, X., Ahmad, M., Bian, J. G., Chen, G. M., Chen, H. S., Chen, M., Chen, Y., Jiang, C. H., Leggat, D., Liao, H., Liu, Z., Romeo, F., Shaheen, S. M., Spiezia, A., Tao, J., Wang, C., Wang, Z., Yazgan, E., Zhang, H., Zhang, S., Zhao, J., Ban, Y., Chen, G., Li, Q., Liu, S., Mao, Y., Qian, S. J., Wang, D., Xu, Z., Avila, C., Cabrera, A., Chaparro Sierra, L. F., Florez, C., Gonzalez Hernandez, C. F., Ruiz Alvarez, J. D., Courbon, B., Godinovic, N., Lelas, D., Puljak, I., Cipriano, P. M. 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A., Mersi, S., Meschi, E., Milenovic, R., Moortgat, F., Mulders, M., Neugebauer, H., Orfanelli, S., Orsini, L., Pape, L., Perez, E., Peruzzi, M., Petrilli, A., Petrucciani, G., Pfeiffer, A., Pierini, M., Racz, A., Reis, T., Rolandi, G., Rovere, M., Sakulin, H., Schafer, C., Schwick, C., Seidel, M., Selvaggi, M., Sharma, A., Silva, R., Sphicas, R., Stakia, A., Steggemann, J., Stoye, M., Tosi, M., Treille, D., Triossi, A., Tsirou, A., Veckalns, V., Verweij, M., Zeuner, W. D., Bertl, W., Caminada, L., Deiters, K., Erdmann, W., Horisberger, R., Ingram, Q., Kaestli, H. C., Kotlinski, D., Langenegger, U., Rohe, T., Wiederkehr, S. A., Bachmair, F., Bani, L., Berger, R., Bianchini, L., Casal, B., Dissertori, G., Dittmar, M., Donega, M., Grab, C., Heidegger, C., Hits, D., Hoss, J., Kasieczka, G., Klijnsma, T., Lustermann, W., Mangano, B., Marionneau, M., Meinhard, M. T., Meister, D., Micheli, F., Musella, R., Nessi-Tedaldi, F., Pandolfi, F., Pata, J., Pauss, F., Perrin, G., Perrozzi, L., Quittnat, M., Reichmann, M., Schonenberger, M., Shchutska, L., Tavolaro, V. R., Theofilatos, K., Olsson, M. L. Vesterbacka, Wallny, R., Zhu, D. H., Aarrestad, T. K., Amsler, C., Canelli, M. F., De Cosa, A., Del Burgo, R., Donato, S., Galloni, C., Hreus, T., Kilminster, B., Ngadiuba, J., Pinna, D., Rauco, G., Robmann, R., Salerno, D., Seitz, C., Takahashi, Y., Zucchetta, A., Candelise, V., Doan, T. H., Jain, Sh, Khurana, R., Kuo, C. M., Lin, W., Pozdnyakov, A., Yu, S. S., Kumar, Arun, Chang, R., Chao, Y., Chen, K. F., Chen, P. H., Fiori, F., Hou, W.-S., Hsiung, Y., Liu, Y. F., Lu, R.-S., Paganis, E., Psallidas, A., Steen, A., Tsai, J. F., Asavapibhop, B., Kovitanggoon, K., Singh, G., Srimanobhas, N., Bakirci, M. N., Boran, F., Damarseckin, S., Demiroglu, Z. S., Dozen, C., Dumanoglu, I., Eskut, E., Girgis, S., Gokbulut, G., Guler, Y., Hos, I., Kangal, E. E., Kara, O., Kiminsu, U., Oglakci, M., Onengut, G., Ozdemir, K., Ozturk, S., Topakli, H., Turkcapar, S., Zorbakir, I. S., Zorbilmez, C., Bilin, B., Karapinar, G., Ocalan, K., Yalvac, M., Zeyrek, M., Gulmez, E., Kaya, M., Kaya, O., Tekten, S., Yetkin, E. A., Agaras, M. N., Atay, S., Cakir, A., Cankocak, K., Grynyov, B., Levchuk, L., Sorokin, R., Aggleton, R., Ball, F., Beck, L., Brooke, J. J., Burns, D., Clement, E., Cussans, D., Davignon, O., Flacher, H., Goldstein, J., Grimes, M., Heath, G. P., Heath, H. F., Jacob, J., Kreczko, L., Lucas, C., Newbold, D. M., Paramesvaran, S., Poll, A., Sakuma, T., El Nasr-Storey, S. Seif, Smith, D., Smith, V. J., Bell, K. W., Belyaev, A., Brew, C., Brown, R. M., Calligaris, L., Cieri, D., Cockerill, D. J. A., Coughlan, J. A., Harder, K., Harper, S., Olaiya, E., Petyt, D., Shepherd-Themistocleous, C. H., Thea, A., Tomalin, I. R., Williams, T., Auzinger, G., Bainbridge, R., Breeze, S., Buchmuller, O., Bundock, A., Casasso, S., Citron, M., Colling, D., Corpe, L., Dauncey, R., Davies, G., De Wit, A., Della Negra, M., Di Maria, R., Elwood, A., Haddad, Y., Hall, G., Iles, G., James, T., Lane, R., Laner, C., Lyons, L., Magnan, A.-M., Malik, S., Mastrolorenzo, L., Matsushita, T., Nash, J., Nikitenko, A., Palladino, V., Pesaresi, M., Raymond, D. M., Richards, A., Rose, A., Scott, E., Seez, C., Shtipliyski, A., Summers, S., Tapper, A., Uchida, K., Acosta, M. Vazquez, Virdee, T., Wardle, N., Winterbottom, D., Wright, J., Zenz, S. C., Cole, J. E., Hobson, P. R., Khan, A., Kyberd, R., Reid, I. D., Symonds, R., Teodorescu, L., Turner, M., Borzou, A., Call, K., Dittmann, J., Hatakeyama, K., Liu, H., Pastika, N., Smith, C., Bartek, R., Dominguez, A., Buccilli, A., Cooper, S. I., Henderson, C., Rumerio, R., West, C., Arcaro, D., Avetisyan, A., Bose, T., Gastler, D., Rankin, D., Richardson, C., Rohlf, J., Sulak, L., Zou, D., Benelli, G., Cutts, D., Garabedian, A., Hakala, J., Heintz, U., Hogan, J. M., Kwok, K. H. M., Laird, E., Landsberg, G., Mao, Z., Narain, M., Pazzini, J., Piperov, S., Sagir, S., Syarif, R., Yu, D., Band, R., Brainerd, C., Breedon, R., Burns, D., Sanchez, M. Calderon De La Barca, Chertok, M., Conway, J., Conway, R., Cox, P. T., Erbacher, R., Flores, C., Funk, G., Gardner, M., Ko, W., Lander, R., Mclean, C., Mulhearn, M., Pellett, D., Pilot, J., Shalhout, S., Shi, M., Smith, J., Squires, M., Stolp, D., Tos, K., Tripathi, M., Wang, Z., Bachtis, M., Bravo, C., Cousins, R., Dasgupta, A., Florent, A., Hauser, J., Ignatenko, M., Mccoll, N., Saltzberg, D., Schnaible, C., Valuev, V., Bouvier, E., Burt, K., Clare, R., Ellison, J., Gary, J. W., Shirazi, S. M. A. Ghiasi, Hanson, G., Heilman, J., Jandir, R., Kennedy, E., Lacroix, F., Long, O. R., Negrete, M. Olmedo, Paneva, M. I., Shrinivas, A., Si, W., Wang, L., Wei, H., Wimpenny, S., Yates, B. R., Branson, J. G., Cittolin, S., Derdzinski, M., Gerosa, R., Hashemi, B., Holzner, A., Klein, D., Kole, G., Krutelyov, V., Letts, J., Macneill, I., Masciovecchio, M., Olivito, D., Padhi, S., Pieri, M., Sani, M., Sharma, V., Simon, S., Tadel, M., Vartak, A., Wasserbaech, S., Wood, J., Wurthwein, F., Yagil, A., Della Porta, G. Zevi, Amin, N., Bhandari, R., Bradmiller-Feld, J., Campagnari, C., Dishaw, A., Dutta, V., Sevilla, M. Franco, George, C., Golf, F., Gouskos, L., Gran, J., Heller, R., Incandela, J., Mullin, S. D., Ovcharova, A., Qu, H., Richman, J., Stuart, D., Suarez, I., Yoo, J., Anderson, D., Bendavid, J., Bornheim, A., Lawhorn, J. M., Newman, H. B., Nguyen, T., Pena, C., Spiropulu, M., Vlimant, J. R., Xie, S., Zhang, Z., Zhu, R. Y., Andrews, M. B., Ferguson, T., Mudholkar, T., Paulini, M., Russ, J., Sun, M., Vogel, H., Vorobiev, I., Weinberg, M., Cumalat, J. P., Ford, W. T., Jensen, F., Johnson, A., Krohn, M., Leontsinis, S., Mulholland, T., Stenson, K., Wagner, S. R., Alexander, J., Chaves, J., Chu, J., Dittmer, S., Mcdermott, K., Mirman, N., Patterson, J. R., Rinkevicius, A., Ryd, A., Skinnari, L., Soffi, L., Tan, S. M., Tao, Z., Thom, J., Tucker, J., Wittich, R., Zientek, M., Abdullin, S., Albrow, M., Apollinari, G., Apresyan, A., Apyan, A., Banerjee, S., Bauerdick, L. A. T., Beretvas, A., Berryhill, J., Bhat, P. C., Bolla, G., Burkett, K., Butler, J. N., Canepa, A., Cerati, G. B., Cheung, H. W. K., Chlebana, F., Cremonesi, M., Duarte, J., Elvira, V. D., Freeman, J., Gecse, Z., Gottschalk, E., Gray, L., Green, D., Grunendahl, S., Gutsche, O., Harris, R. M., Hasegawa, S., Hirschauer, J., Hu, Z., Jayatilaka, B., Jindariani, S., Johnson, M., Joshi, U., Klima, B., Kreis, B., Lammel, S., Lincoln, D., Lipton, R., Liu, M., Liu, T., De Sa, R. Lopes, Lykken, J., Maeshima, K., Magini, N., Marraffino, J. M., Maruyama, S., Mason, D., McBride, R., Merkel, R., Mrenna, S., Nahn, S., O'Dell, V., Pedro, K., Prokofyev, O., Rakness, G., Ristori, L., Schneider, B., Sexton-Kennedy, E., Soha, A., Spalding, W. J., Spiegel, L., Stoynev, S., Strait, J., Strobbe, N., Taylor, L., Tkaczyk, S., Tran, N. V., Uplegger, L., Vaandering, E. W., Vernieri, C., Verzocchi, M., Vidal, R., Wang, M., Weber, H. A., Whitbeck, A., Acosta, D., Avery, R., Bortignon, R., Bourilkov, D., Brinkerhoff, A., Carnes, A., Carver, M., Curry, D., Field, R. D., Furic, I. K., Konigsberg, J., Korytov, A., Kotov, K., Ma, R., Matchev, K., Mei, H., Mitselmakher, G., Rank, D., Sperka, D., Terentyev, N., Thomas, L., Wang, J., Wang, S., Yelton, J., Joshi, Y. R., Linn, S., Markowitz, R., Rodriguez, J. L., Ackert, A., Adams, T., Askew, A., Hagopian, S., Hagopian, V., Johnson, K. F., Kolberg, T., Martinez, G., Perry, T., Prosper, H., Saha, A., Santra, A., Sharma, V., Yohay, R., Baarmand, M. M., Bhopatkar, V., Colafranceschi, S., Hohlmann, M., Noonan, D., Roy, T., Yumiceva, F., Adams, M. R., Apanasevich, L., Berry, D., Betts, R. R., Cavanaugh, R., Chen, X., Evdokimov, O., Gerber, C. E., Hangal, D. A., Hofman, D. J., Jung, K., Kamin, J., Gonzalez, I. D. Sandoval, Tonjes, M. B., Trauger, H., Varelas, N., Wang, H., Wu, Z., Zhang, J., Bilki, B., Clarida, W., Dilsiz, K., Durgut, S., Gandrajula, R. P., Haytmyradov, M., Khristenko, V., Merlo, J.-R., Mermerkaya, H., Mestvirishvili, A., Moeller, A., Nachtman, J., Ogul, H., Onel, Y., Ozok, F., Penzo, A., Snyder, C., Tiras, E., Wetzel, J., Yi, K., Blumenfeld, B., Cocoros, A., Eminizer, N., Fehling, D., Feng, L., Gritsan, A. V., Maksimovic, R., Roskes, J., Sarica, U., Swartz, M., Xiao, M., You, C., Al-Bataineh, A., Baringer, R., Bean, A., Boren, S., Bowen, J., Castle, J., Khalil, S., Kropivnitskaya, A., Majumder, D., Mcbrayer, W., Murray, M., Royon, C., Sanders, S., Schmitz, E., Takaki, J. D. Tapia, Wang, Q., Ivanov, A., Kaadze, K., Maravin, Y., Mohammadi, A., Saini, L. K., Skhirtladze, N., Toda, S., Rebassoo, F., Wright, D., Anelli, C., Baden, A., Baron, O., Belloni, A., Calvert, B., Eno, S. C., Ferraioli, C., Hadley, N. J., Jabeen, S., Jeng, G. Y., Kellogg, R. G., Kunkle, J., Mignerey, A. C., Ricci-Tam, F., Shin, Y. H., Skuja, A., Tonwar, S. C., Abercrombie, D., Allen, B., Azzolini, V., Barbieri, R., Baty, A., Bi, R., Brandt, S., Busza, W., Cali, I. A., D'Alfonso, M., Demiragli, Z., Ceballos, G. Gomez, Goncharov, M., Hsu, D., Iiyama, Y., Innocenti, G. M., Klute, M., Kovalskyi, D., Lai, Y. S., Lee, Y.-J., Levin, A., Luckey, P. D., Maier, B., Marini, A. C., Mcginn, C., Mironov, C., Narayanan, S., Niu, X., Paus, C., Roland, C., Roland, G., Salfeld-Nebgen, J., Stephans, G. S. F., Tatar, K., Velicanu, D., Wang, J., Wang, T. W., Wyslouch, B., Benvenuti, A. C., Chatterjee, R. M., Evans, A., Hansen, R., Kalafut, S., Kubota, Y., Lesko, Z., Mans, J., Nourbakhsh, S., Ruckstuhl, N., Rusack, R., Turkewitz, J., Acosta, J. G., Oliveros, S., Avdeeva, E., Bloom, K., Claes, D. R., Fangmeier, C., Suarez, R. Gonzalez, Kamalieddin, R., Kravchenko, I., Monroy, J., Siado, J. E., Snow, G. R., Stieger, B., Alyari, M., Dolen, J., Godshalk, A., Harrington, C., Iashvili, I., Nguyen, D., Parker, A., Rappoccio, S., Roozbahani, B., Alverson, G., Barberis, E., Hortiangtham, A., Massironi, A., Morse, D. M., Nash, D., Orimoto, T., De Lima, R. Teixeira, Trocino, D., Wood, D., Bhattacharya, S., Charaf, O., Hahn, K. A., Mucia, N., Odell, N., Pollack, B., Schmitt, M. H., Sung, K., Trovato, M., Velasco, M., Dev, N., Hildreth, M., Anampa, K. Hurtado, Jessop, C., Karmgard, D. J., Kellams, N., Lannon, K., Loukas, N., Marinelli, N., Meng, F., Mueller, C., Musienko, Y., Planer, M., Reinsvold, A., Ruchti, R., Smith, G., Taroni, S., Wayne, M., Wolf, M., Woodard, A., Alimena, J., Antonelli, L., Bylsma, B., Durkin, L. S., Flowers, S., Francis, B., Hart, A., Hill, C., Ji, W., Liu, B., Luo, W., Puigh, D., Winer, B. L., Wulsin, H. W., Cooperstein, S., Driga, O., Elmer, R., Hardenbrook, J., Hebda, R., Higginbotham, S., Lange, D., Luo, J., Marlow, D., Mei, K., Ojalvo, I., Olsen, J., Palmer, C., Piroue, R., Stickland, D., Tully, C., Malik, S., Norberg, S., Barker, A., Barnes, V. E., Das, S., Folgueras, S., Gutay, L., Jha, M. K., Jones, M., Jung, A. W., Khatiwada, A., Miller, D. H., Neumeister, N., Peng, C. C., Schulte, J. F., Sun, J., Wang, F., Xie, W., Cheng, T., Parashar, N., Stupak, J., Adair, A., Akgun, B., Chen, Z., Ecklund, K. M., Geurts, F. J. M., Guilbaud, M., Li, W., Michlin, B., Northup, M., Padley, B. P., Roberts, J., Rorie, J., Tu, Z., Zabel, J., Bodek, A., de Barbaro, R., Demina, R., Duh, Y. T., Ferbel, T., Galanti, M., Garcia-Bellido, A., Han, J., Hindrichs, O., Khukhunaishvili, A., Lo, K. H., Tan, R., Verzetti, M., Ciesielski, R., Goulianos, K., Mesropian, C., Agapitos, A., Chou, J. P., Gershtein, Y., Espinosa, T. A. Gomez, Halkiadakis, E., Heindl, M., Hughes, E., Kaplan, S., Elayavalli, R. Kunnawalkam, Kyriacou, S., Lath, A., Montalvo, R., Nash, K., Osherson, M., Saka, H., Salur, S., Schnetzer, S., Sheffield, D., Somalwar, S., Stone, R., Thomas, S., Thomassen, R., Walker, M., Delannoy, A. G., Foerster, M., Heideman, J., Riley, G., Rose, K., Spanier, S., Thapa, K., Bouhali, O., Hernandez, A. Castaneda, Celik, A., Dalchenko, M., De Mattia, M., Delgado, A., Dildick, S., Eusebi, R., Gilmore, J., Huang, T., Kamon, T., Mueller, R., Pakhotin, Y., Patel, R., Perloff, A., Pernie, L., Rathjens, D., Safonov, A., Tatarinov, A., Ulmer, K. A., Akchurin, N., Damgov, J., De Guio, F., Dudero, P. R., Faulkner, J., Gurpinar, E., Kunori, S., Lamichhane, K., Lee, S. W., Libeiro, T., Peltola, T., Undleeb, S., Volobouev, I., Wang, Z., Greene, S., Gurrola, A., Janjam, R., Johns, W., Maguire, C., Melo, A., Ni, H., Sheldon, R., Tuo, S., Velkovska, J., Xu, Q., Arenton, M. W., Barria, R., Cox, B., Hirosky, R., Joyce, M., Ledovskoy, A., Li, H., Neu, C., Sinthuprasith, T., Wang, Y., Wolfe, E., Xia, F., Harr, R., Karchin, P. E., Sturdy, J., Zaleski, S., Brodski, M., Buchanan, J., Caillol, C., Dasu, S., Dodd, L., Duric, S., Gomber, B., Grothe, M., Herndon, M., Herve, A., Hussain, U., Klabbers, R., Lanaro, A., Levine, A., Long, K., Loveless, R., Pierro, G. A., Polese, G., Ruggles, T., Savin, A., Smith, N., Smith, W. H., Taylor, D., Woods, N.
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Abstract/Description: Differential production cross sections of prompt J/psi and psi(2S) charmonium and Upsilon(nS) (n = 1, 2, 3) bottomonium states are measured in proton-proton collisions at root s = 13 TeV, with data collected by the CMS detector at the LHC, corresponding to an integrated luminosity of 2.3 fb(-1) for the J/psi and 2.7 fb(-1) for the other mesons. The five quarkonium states are reconstructed in the dimuon decay channel, for dimuon rapidity vertical bar y vertical bar < 1.2. The double...
Show moreDifferential production cross sections of prompt J/psi and psi(2S) charmonium and Upsilon(nS) (n = 1, 2, 3) bottomonium states are measured in proton-proton collisions at root s = 13 TeV, with data collected by the CMS detector at the LHC, corresponding to an integrated luminosity of 2.3 fb(-1) for the J/psi and 2.7 fb(-1) for the other mesons. The five quarkonium states are reconstructed in the dimuon decay channel, for dimuon rapidity vertical bar y vertical bar < 1.2. The double-differential cross sections for each state are measured as a function of y and transverse momentum, and compared to theoretical expectations. In addition, ratios are presented of cross sections for prompt psi(2S) to J/psi, Upsilon(2S) to Upsilon(1S), and Upsilon(3S) to Upsilon(1S) production. (C) 2018 The Author(s). Published by Elsevier B.V.
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Date Issued: 2018-05-10
Identifier: FSU_libsubv1_wos_000432187800041, 10.1016/j.physletb.2018.02.033
Format: Citation

Title: Hard Exclusive Pion Electroproduction At Backward Angles With Clas.
Creator: Park, K., Guidal, M., Gothe, R. W., Pire, B., Semenov-Tian-Shansky, K., Laget, J.-M., Adhikari, K. P., Adhikari, S., Akbar, Z., Avakian, H., Ball, J., Balossino, I., Baltzell, N...
Show morePark, K., Guidal, M., Gothe, R. W., Pire, B., Semenov-Tian-Shansky, K., Laget, J.-M., Adhikari, K. P., Adhikari, S., Akbar, Z., Avakian, H., Ball, J., Balossino, I., Baltzell, N. A., Barion, L., Battaglieri, M., Bedlinskiy, I., Biselli, A. S., Briscoe, W. J., Brooks, W. K., Burkert, V. D., Cao, F. T., Carman, D. S., Celentano, A., Charles, G., Chetry, T., Ciullo, G., Clark, L., Cole, P. L., Contalbrigo, M., Crede, V., D'Angelo, A., Dashyan, N., De Vita, R., De Sanctis, E., Defurne, M., Deur, A., Djalali, C., Dupre, R., Egiyan, H., El Alaoui, A., El Fassi, L., Elouadrhiri, L., Eugenio, R., Fedotov, G., Fersch, R., Filippi, A., Garcon, M., Ghandilyan, Y., Gilfoyle, G. P., Girod, F. X., Golovatch, E., Griffioen, K. A., Guo, L., Hafidi, K., Hakobyan, H., Hanretty, C., Harrison, N., Hattawy, M., Heddle, D., Hicks, K., Holtrop, M., Hyde, C. E., Ilieva, Y., Ireland, D. G., Ishkhanov, B. S., Isupov, E. L., Jenkins, D., Johnston, S., Joo, K., Kabir, M. L., Keller, D., Khachatryan, G., Khachatryan, M., Khandaker, M., Kim, W., Klein, F. J., Kubarovsky, V., Kuhn, S. E., Lanza, L., Livingston, K., MacGregor, I. J. D., Markov, N., McKinnon, B., Mirazita, M., Mokeev, V., Montgomery, R. A., Camacho, C. Munoz, Nadel-Turonski, R., Niccolai, S., Niculescu, G., Osipenko, M., Paolone, M., Paremuzyan, R., Pasyuk, E., Phelps, W., Pogorelko, O., Poudel, J., Price, J. W., Prok, Y., Protopopescu, D., Ripani, M., Rizzo, A., Rossi, P., Sabatie, F., Salgado, C., Schumacher, R. A., Sharabian, Y., Skorodumina, Iu, Smith, G. D., Sokhan, D., Sparveris, N., Stepanyan, S., Strakovsky, I. I., Strauch, S., Taiuti, M., Tan, J. A., Ungar, M., Voskanyan, H., Voutier, E., Wei, X., Zachariou, N., Zhang, J.
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Abstract/Description: We report on the first measurement of cross sections for exclusive deeply virtual pion electroproduction off the proton, ep -> e'n pi(+), above the resonance region at backward pion center-of-mass angles. The phi(pi)*-dependent cross sections were measured, from which we extracted three combinations of structure functions of the proton. Our results are compatible with calculations based on nucleon-to-pion transition distribution amplitudes (TDAs). These non-perturbative objects are defined as...
Show moreWe report on the first measurement of cross sections for exclusive deeply virtual pion electroproduction off the proton, ep -> e'n pi(+), above the resonance region at backward pion center-of-mass angles. The phi(pi)*-dependent cross sections were measured, from which we extracted three combinations of structure functions of the proton. Our results are compatible with calculations based on nucleon-to-pion transition distribution amplitudes (TDAs). These non-perturbative objects are defined as matrix elements of three-quark-light-cone-operators and characterize partonic correlations with a particular emphasis on baryon charge distribution inside a nucleon. (C) 2018 The Authors. Published by Elsevier B.V.
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Date Issued: 2018-05-10
Identifier: FSU_libsubv1_wos_000432187800053, 10.1016/j.physletb.2018.03.026
Format: Citation

Title: Study Of The X-+/-(5568) State With Semileptonic Decays Of The B-s(0) Meson.
Creator: Abazov, V. M., Abbott, B., Acharya, B. S., Adams, M., Adams, T., Agnew, J. P., Alexeev, G. D., Alkhazov, G., Alton, A., Askew, A., Atkins, S., Augsten, K., Aushev, V., Aushev, Y...
Show moreAbazov, V. M., Abbott, B., Acharya, B. S., Adams, M., Adams, T., Agnew, J. P., Alexeev, G. D., Alkhazov, G., Alton, A., Askew, A., Atkins, S., Augsten, K., Aushev, V., Aushev, Y., Avila, C., Badaud, F., Bagby, L., Baldin, B., Bandurin, D., Banerjee, S., Barberis, E., Baringer, P., Bartlett, J. F., Bassler, U., Bazterra, V., Bean, A., Begalli, M., Bellantoni, L., Beri, S. B., Bernardi, G., Bernhard, R., Bertram, I., Besancon, M., Beuselinck, R., Bhat, P. C., Bhatia, S., Bhatnagar, V., Blazey, G., Blessing, S., Bloom, K., Boehnlein, A., Boline, D., Boos, E. E., Borissov, G., Borysova, M., Brandt, A., Brandt, O., Brochmann, M., Brock, R., Bross, A., Brown, D., Bu, X. B., Buehler, M., Buescher, V., Bunichev, V., Burdin, S., Buszello, C. P., Camacho-Perez, E., Casey, B. C. K., Castilla-Vaidez, H., Caughron, S., Chakrabarti, S., Chan, K. M., Chandra, A., Chapon, E., Chen, G., Cho, S. W., Choi, S., Choudhary, B., Cihangir, S., Claes, D., Clutter, J., Cooke, M., Cooper, W. E., Corcoran, M., Couderc, F., Cousinou, M.-C., Cuth, J., Cutts, D., Das, A., Davies, G., de Jong, S. J., De La Cruz-Burelo, E., Deliot, F., Demina, R., Denisov, D., Denisov, S. P., Desai, S., Deterre, C., DeVaughan, K., Diehl, H. T., Diesburg, M., Ding, P. F., Dominguez, A., Drutskoy, A., Dubey, A., Dudko, L., Duperrin, A., Dutt, S., Eads, M., Edmunds, D., Ellison, J., Elvira, V. D., Enari, Y., Evans, H., Evdokimov, A., Evdokimov, V. N., Faure, A., Feng, L., Ferbe, T., Fiedler, F., Filthaut, F., Fisher, W., Fisk, H. E., Fortne, M., Fox, H., Franc, J., Fuess, S., Garbincius, P. H., Garcia-Bellido, A., Garcia-Gonzalez, J. A., Gavrilov, V., Geng, W., Gerber, C. E., Gershtein, Y., Ginther, G., Gogota, O., Golovanov, G., Grannis, P. D., Greder, S., Greenlee, H., Grenier, G., Gris, Ph, Grivaz, J.-F., Grohsjean, A., Grunendahl, S., Grunewald, M. W., Guillemin, T., Gutierrez, G., Gutierrez, P., Haley, J., Han, L., Harder, K., Harel, A., Hauptman, J. M., Hays, J., Head, T., Hebbeker, T., Hedin, D., Hegab, H., Heinson, A. P., Heintz, U., Hensel, C., Heredia-De La Cruz, I., Herner, K., Hesketh, G., Hildreth, M. D., Hirosky, R., Hoang, T., Hobbs, J. D., Hoeneisen, B., Hogan, J., Hohlfeld, M., Holzbauer, J. L., Howley, I., Hubacek, Z., Hynek, V., Iashvili, I., Ilchenko, Y., Illingworth, R., Ito, A. S., Jabeen, S., Jaffre, M., Jayasinghe, A., Jeong, M. S., Jesik, R., Jiang, P., Johns, K., Johnson, E., Johnson, M., Jonckheere, A., Jonsson, P., Joshi, J., Jung, A. W., Juste, A., Kajfasz, E., Karmanov, D., Katsanos, I., Kaur, M., Kehoe, R., Kermiche, S., Khalatyan, N., Khanov, A., Kharchilava, A., Kharzheev, Y. N., Kiselevich, I., Kohli, J. M., Kozelov, A., Kraus, J., Kumar, A., Kupco, A., Kurca, T., Kuzmin, V. A., Lammers, S., Lebrun, P., Lee, H. S., Lee, S. W., Lee, W. M., Lei, X., Lellouch, J., Li, D., Li, H., Li, L., Li, Q. Z., Lim, J. K., Lincoln, D., Linnemann, J., Lipaev, V. V., Lipton, R., Liu, H., Liu, Y., Lobodenko, A., Lokajicek, M., de Sa, R. Lopes, Luna-Garcia, R., Lyon, A. L., Macie, A. K. A., Madar, R., Magana-Villalba, R., Malik, S., Malyshev, V. L., Mansour, J., Martinez-Ortega, J., McCarthy, R., McGivern, C. L., Meijer, M. M., Melnitchouk, A., Menezes, D., Mercadante, P. G., Merkin, M., Meyer, A., Meyer, J., Miconi, F., Mondal, N. K., Mulhearn, M., Nagy, E., Narain, M., Nayyar, R., Neal, H. A., Negret, J. P., Neustroev, P., Nguyen, H. T., Nunnemann, T., Orduna, J., Osman, N., Pal, A., Parashar, N., Parihar, V., Park, S. K., Partridge, R., Parua, N., Patwa, A., Penning, B., Perfilov, M., Peters, Y., Petridis, K., Petrillo, G., Petroff, P., Pleier, M.-A., Podstavkov, V. M., Popov, A., Prewitt, M., Price, D., Prokopenko, N., Qian, J., Quadt, A., Quinn, B., Ratoff, P. N., Razumov, I., Ripp-Baudot, I., Rizatdinova, F., Rominsky, M., Ross, A., Royon, C., Rubinov, P., Ruchti, R., Sajot, G., Sanchez-Hernandez, A., Sanders, M. P., Santos, A. S., Savage, G., Savitskyi, M., Sawyer, L., Scanlon, T., Schamberger, R. D., Scheglov, Y., Schellman, H., Schott, M., Schwanenberger, C., Schwienhorst, R., Sekaric, J., Severini, H., Shabalina, E., Shary, V., Shaw, S., Shchukin, A. A., Shkola, O., Simak, V., Skubic, P., Slattery, P., Snow, G. R., Snow, J., Snyder, S., Soldner-Rembold, S., Sonnenschein, L., Soustruznik, K., Stark, J., Stefaniuk, N., Stoyanova, D. A., Strauss, M., Suter, L., Svoisky, P., Titov, M., Tokemenin, V. V., Tsai, Y.-T., Tsybychev, D., Tuchming, B., Tully, C., Uvarov, L., Uvarov, S., Uzunyan, S., Van Kooten, R., van Leeuwen, W. M., Varelas, N., Varnes, E. W., Vasilyev, I. A., Verkheev, A. Y., Vertogradov, L. S., Verzocchi, M., Vesterinen, M., Vilanova, D., Vokac, P., Wahl, H. D., Wang, M. H. L. S., Warchol, J., Watts, G., Wayne, M., Weichert, J., Welty-Rieger, L., Williams, M. R. J., Wilson, G. W., Wobisch, M., Wood, D. R., Wyatt, T. R., Xie, Y., Yamada, R., Yang, S., Yasuda, T., Yatsunenko, Y. A., Ye, W., Ye, Z., Yin, H., Yip, K., Youn, S. W., Yu, J. M., Zennamo, J., Zhao, T. G., Zhou, B., Zhu, J., Zielinski, M., Zieminska, D., Zivkovic, L.
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Abstract/Description: We present a study of the X-+/-(5568) using semileptonic decays of the B-s(0) meson using the full run II integrated luminosity of 10.4 fb(-1) in proton-antiproton collisions at a center of mass energy of 1.96 TeV collected with the DO detector at the Fermilab Tevatron Collider. We report evidence for a narrow structure, X-+/-(5568), in the decay sequence X-+/-(5568) -> B-s(0) pi(+/-) where B-s(0)-> mu(-/+) (DsX)-X-+/-, D-s(+/-)-> phi pi(+/-)which is consistent with the previous measurement...
Show moreWe present a study of the X-+/-(5568) using semileptonic decays of the B-s(0) meson using the full run II integrated luminosity of 10.4 fb(-1) in proton-antiproton collisions at a center of mass energy of 1.96 TeV collected with the DO detector at the Fermilab Tevatron Collider. We report evidence for a narrow structure, X-+/-(5568), in the decay sequence X-+/-(5568) -> B-s(0) pi(+/-) where B-s(0)-> mu(-/+) (DsX)-X-+/-, D-s(+/-)-> phi pi(+/-)which is consistent with the previous measurement by the DO Collaboration in the hadronic decay mode, X-+/-(5568) -> B-s(0)pi(+/-) where B-s(0 )-> J/psi phi. The mass and width of this state are measured using a combined fit of the hadronic and semileptonic data, yielding m = 5566.9(-3.1)(+3.2)(stat)(-1.2)(+0.6)(syst) MeV/c(2), Gamma = 18.6(-6.1)(+7.9)(stat)(-3.8)(+3.5) (syst) McV/c(2) with a significance of 6.7 sigma.
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Date Issued: 2018-05-18
Identifier: FSU_libsubv1_wos_000433027600002, 10.1103/PhysRevD.97.092004
Format: Citation

Title: Search For New Long-lived Particles At Root S=13 Tev.
Creator: Sirunyan, A. M., Tumasyan, A., Adam, W., Ambrogi, F., Asilar, E., Bergauer, T., Brandstetter, J., Brondolin, E., Dragicevic, M., Eroe, J., Flechl, M., Friedl, M., Fruehwirth, R....
Show moreSirunyan, A. M., Tumasyan, A., Adam, W., Ambrogi, F., Asilar, E., Bergauer, T., Brandstetter, J., Brondolin, E., Dragicevic, M., Eroe, J., Flechl, M., Friedl, M., Fruehwirth, R., Ghete, V. M., Grossmann, J., Hrubec, J., Jeitler, M., Koenig, A., Krammer, N., Kraetschmer, I., Liko, D., Madlener, T., Mikulec, I., Pree, E., Rabady, D., Rad, N., Rohringer, H., Schieck, J., Schoefbeck, R., Spanring, M., Spitzbart, D., Strauss, J., Waltenberger, W., Wittmann, J., Wulz, C.-E., Zarucki, M., Chekhovsky, V., Mossolov, V., Gonzalez, J. Suarez, De Wolf, E. A., Di Croce, D., Janssen, X., Lauwers, J., Van de Klundert, M., Van Haevermaet, H., Van Mechelen, R., Van Remortel, N., Abu Zeid, S., Blekman, F., D'Hondt, J., De Bruyn, I., De Clercq, J., Deroover, K., Flouris, G., Lontkovskyi, D., Lowette, S., Moortgat, S., Moreels, L., Olbrechts, A., Python, Q., Skovpen, K., Tavernier, S., Van Doninck, W., Van Mulders, R., Van Parijs, I., Brun, H., Clerbaux, B., De Lentdecker, G., Delannoy, H., Fasanella, G., Favart, L., Goldouzian, R., Grebenyuk, A., Karapostoli, G., Lenzi, T., Luetic, J., Maerschalk, T., Marinov, A., Randle-Conde, A., Seva, T., Vander Velde, C., Vanlaer, R., Vannerom, D., Yonamine, R., Zenoni, F., Zhang, F., Cimmino, A., Cornelis, T., Dobur, D., Fagot, A., Gul, M., Khvastunov, I., Poyraz, D., Roskas, C., Salva, S., Tytgat, M., Verbeke, W., Zaganidis, N., Bakhshiansohi, H., Bondu, O., Brochet, S., Bruno, G., Caudron, A., De Visscher, S., Delaere, C., Delcourt, M., Francois, B., Giammanco, A., Jafari, A., Komm, M., Krintiras, G., Lemaitre, V., Magitteri, A., Mertens, A., Musich, M., Piotrzkowski, K., Quertenmont, L., Marono, M. Vidal, Wertz, S., Beliy, N., Alda Junior, W. L., Alves, F. L., Alves, G. A., Brito, L., Correa Martins Junior, M., Hensel, C., Moraes, A., Pol, M. E., Rebello Teles, R., Das Chagas, E. Belchior Batista, Carvalho, W., Chinellato, J., Custodio, A., Da Costa, E. M., Da Silveira, G. G., Damiao, D. De Jesus, De Souza, S. Fonseca, Guativa, L. M. Huertas, Malbouisson, H., De Almeida, M. Melo, Herrera, C. Mora, Mundim, L., Nogima, H., Santoro, A., Sznajder, A., Manganote, E. J. Tonelli, De Araujo, F. Torres Da Silva, Vilela Pereira, A., Ahuja, S., Bernardes, C. A., Fernandez Perez Tomei, T. R., Gregores, E. M., Mercadante, P. G., Novaes, S. F., Padula, Sandra S., Romero Abad, D., Ruiz Vargas, J. C., Aleksandrov, A., Hadjiiska, R., Iaydjiev, R., Misheva, M., Rodozov, M., Shopova, M., Stoykova, S., Sultanov, G., Dimitrov, A., Glushkov, I., Litov, L., Pavlov, B., Petkov, R., Fang, W., Gao, X., Ahmad, M., Bian, J. G., Chen, G. M., Chen, H. S., Chen, M., Chen, Y., Jiang, C. H., Leggat, D., Liao, H., Liu, Z., Romeo, F., Shaheen, S. M., Spiezia, A., Tao, J., Wang, C., Wang, Z., Yazgan, E., Zhang, H., Zhao, J., Ban, Y., Chen, G., Li, Q., Liu, S., Mao, Y., Qian, S. J., Wang, D., Xu, Z., Avila, C., Cabrera, A., Chaparro Sierra, L. F., Florez, C., Gonzalez Hernandez, C. F., Ruiz Alvarez, J. D., Courbon, B., Godinovic, N., Lelas, D., Puljak, I., Cipriano, P. M. Ribeiro, Sculac, T., Antunovic, Z., Kovac, M., Brigljevic, V., Ferencek, D., Kadija, K., Mesic, B., Starodumov, A., Susa, T., Ather, M. W., Attikis, A., Mavromanolakis, G., Mousa, J., Nicolaou, C., Ptochos, F., Razis, P. A., Rykaczewski, H., Finger, M., Finger, M., Carrera Jarrin, E., El-Khateeb, E., Elgammal, S., Mohamed, A., Dewanjee, R. K., Kadastik, M., Perrini, L., Raidal, M., Tiko, A., Veelken, C., Eerola, R., Pekkanen, J., Voutilainen, M., Harkonen, J., Jarvinen, T., Karimaki, V., Kinnunen, R., Lampen, T., Lassila-Perini, K., Lehti, S., Linden, T., Luukka, R., Tuominen, E., Tuominiemi, J., Tuovinen, E., Talvitie, J., Tuuva, T., Besancon, M., Couderc, F., Dejardin, M., Denegri, D., Faure, J. L., Ferri, F., Ganjour, S., Ghosh, S., Givernaud, A., Gras, R., de Monchenault, G. Hamel, Jarry, R., Kucher, I., Locci, E., Machet, M., Malcles, J., Negro, G., Rander, J., Rosowsky, A., Sahin, M. O., Titov, M., Abdulsalam, A., Antropov, I., Baffioni, S., Beaudette, F., Busson, R., Cadamuro, L., Chariot, C., De Cassagnac, R. Granier, Jo, M., Lisniak, S., Lobanov, A., Blanco, J. Martin, Nguyen, M., Ochando, C., Ortona, G., Paganini, R., Pigard, R., Regnard, S., Salerno, R., Sauvan, J. B., Sirois, Y., Leiton, A. G. Stahl, Strebler, T., Yilmaz, Y., Zabi, A., Zghiche, A., Agram, J.-L., Andrea, J., Bloch, D., Brom, J. M., Buttignol, M., Chabert, E. C., Chanon, N., Collard, C., Conte, E., Coubez, X., Fontaine, J. C., Gele, D., Goerlach, U., Jansova, M., Le Bihan, A. C., Tonon, N., Van Hove, R., Gadrat, S., Beauceron, S., Bernet, C., Boudoul, G., Chierici, R., Contardo, D., Depasse, R., El Mamouni, H., Fay, J., Finco, L., Gascon, S., Gouzevitch, M., Grenier, G., Ille, B., Lagarde, F., Laktineh, I. B., Lethuillier, M., Mirabito, L., Pequegnot, A. L., Perries, S., Popov, A., Sordini, V., Donckt, M. Vander, Viret, S., Toriashvili, T., Bagaturia, I., Autermann, C., Beranek, S., Feld, L., Kiesel, M. K., Klein, K., Lipinski, M., Preuten, M., Schomakers, C., Schulz, J., Verlage, T., Albert, A., Dietz-Laursonn, E., Duchardt, D., Endres, M., Erdmann, M., Erdweg, S., Esch, T., Fischer, R., Giith, A., Hamer, M., Hebbeker, T., Heidemann, C., Hoepfner, K., Knutzen, S., Merschmeyer, M., Meyer, A., Millet, R., Mukherjee, S., Olschewski, M., Padeken, K., Pook, T., Radziej, M., Reithler, H., Rieger, M., Scheuch, F., Teyssier, D., Thueer, S., Fluegge, G., Kargoll, B., Kress, T., Kuensken, A., Lingemann, J., Mueller, T., Nehrkorn, A., Nowack, A., Pistone, C., Pooth, O., Stahl, A., Martin, M. Aldaya, Arndt, T., Asawatangtrakuldee, C., Beernaert, K., Behnke, O., Behrens, U., Martinez, A. Bermudez, Bin Anuar, A. A., Borras, K., Botta, V., Campbell, A., Connor, R., Contreras-Campana, C., Costanza, F., Pardos, C. Diez, Eckerlin, G., Eckstein, D., Eichhorn, T., Eren, E., Gallo, E., Garcia, J. Garay, Geiser, A., Gizhko, A., Luyando, J. M. Grados, Grohsjean, A., Gunnellini, R., Harb, A., Hauk, J., Hempel, M., Jung, H., Kalogeropoulos, A., Kasemann, M., Keaveney, J., Kleinwort, C., Korol, I., Kruecker, D., Lange, W., Lelek, A., Lenz, T., Leonard, J., Lipka, K., Lohmann, W., Mankel, R., Melzer-Pellmann, I.-A., Meyer, A. B., Mittag, G., Mnich, J., Mussgiller, A., Ntomari, E., Pitzl, D., Placakyte, R., Raspereza, A., Roland, B., Savitskyi, M., Saxena, R., Shevchenko, R., Spannagel, S., Stefaniuk, N., Van Onsem, G. P., Walsh, R., Wen, Y., Wichmann, K., Wissing, C., Zenaiev, O., Bein, S., Blobel, V., Vignali, M. Centis, Draeger, A. R., Dreyer, T., Garutti, E., Gonzalez, D., Haller, J., Hinzmann, A., Hoffmann, M., Karavdina, A., Klanner, R., Kogler, R., Kovalchuk, N., Kurz, S., Lapsien, T., Marchesini, I., Marconi, D., Meyer, M., Niedziela, M., Nowatschin, D., Pantaleo, F., Peiffer, T., Perieanu, A., Scharf, C., Schleper, R., Schmidt, A., Schumann, S., Schwandt, J., Sonneveld, J., Stadie, H., Steinbrueck, G., Stober, F. M., Stoever, M., Tholen, H., Troendle, D., Usai, E., Vanelderen, L., Vanhoefer, A., Vormwald, B., Akbiyik, M., Barth, C., Baur, S., Butz, E., Caspart, R., Chwalek, T., Colombo, F., De Boer, W., Dierlamm, A., Freund, B., Friese, R., Giffels, M., Gilbert, A., Haitz, D., Hartmann, F., Heindl, S. M., Husemann, U., Kassel, F., Kudella, S., Mildner, H., Mozer, M. U., Mueller, Th, Plagge, M., Quast, G., Rabbertz, K., Schroeder, M., Shvetsov, I., Sieber, G., Simonis, H. J., Ulrich, R., Wayand, S., Weber, M., Weiler, T., Williamson, S., Woehrmann, C., Wolf, R., Anagnostou, G., Daskalakis, G., Geralis, T., Giakoumopoulou, V. A., Kyriakis, A., Loukas, D., Topsis-Giotis, I., Kesisoglou, S., Panagiotou, A., Saoulidou, N., Evangelou, I., Foudas, C., Kokkas, R., Mallios, S., Manthos, N., Papadopoulos, I., Paradas, E., Strologas, J., Triantis, F. A., Csanad, M., Filipovic, N., Pasztor, G., Bencze, G., Hajdu, C., Horvath, D., Hunyadi, A., Sikler, F., Veszpremi, V., Vesztergombi, G., Zsigmond, A. J., Beni, N., Czellar, S., Karancsi, J., Makovec, A., Molnar, J., Szillasi, Z., Bartok, M., Raics, R., Trocsanyi, Z. L., Ujvari, B., Choudhury, S., Komaragiri, J. R., Bahinipati, S., Bhowmik, S., Mal, R., Mandal, K., Nayak, A., Sahoo, D. K., Sahoo, N., Swain, S. K., Bansal, S., Beri, S. B., Bhatnagar, V., Bhawandeep, U., Chawla, R., Dhingra, N., Kalsi, A. K., Kaur, A., Kaur, M., Kumar, R., Kumari, R., Mehta, A., Singh, J. B., Walia, G., Kumar, Ashok, Shah, Aashaq, Bhardwaj, A., Chauhan, S., Choudhary, B. C., Garg, R. B., Keshri, S., Kumar, A., Malhotra, S., Naimuddin, M., Ranjan, K., Sharma, R., Sharma, V., Bhardwaj, R., Bhattacharya, R., Bhattacharya, S., Dey, S., Dutt, S., Dutta, S., Ghosh, S., Majumdar, N., Modak, A., Mondal, K., Mukhopadhyay, S., Nandan, S., Purohit, A., Roy, A., Roy, D., Chowdhury, S. Roy, Sarkar, S., Sharan, M., Thakur, S., Behera, P. K., Chudasama, R., Dutta, D., Jha, V., Kumar, V., Mohanty, A. K., Netrakanti, P. K., Pant, L. M., Shukla, R., Topkar, A., Aziz, T., Dugad, S., Mahakud, B., Mitra, S., Mohanty, G. B., Parida, B., Sur, N., Sutar, B., Banerjee, S., Bhattacharya, S., Chatterjee, S., Das, R., Guchait, M., Jain, Sa, Kumar, S., Maity, M., Majumder, G., Mazumdar, K., Sarkar, T., Wickramage, N., Chauhan, S., Dube, S., Hegde, V., Kapoor, A., Kothekar, K., Pandey, S., Rane, A., Sharma, S., Chenarani, S., Tadavani, E. Eskandari, Etesami, S. M., Khakzad, M., Najafabadi, M. Mohammadi, Naseri, M., Mehdiabadi, S. Paktinat, Hosseinabadi, F. 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Tapia, Wang, Q., Ivanov, A., Kaadze, K., Maravin, Y., Mohammadi, A., Saini, L. K., Skhirtladze, N., Toda, S., Rebassoo, F., Wright, D., Anelli, C., Baden, A., Baron, O., Belloni, A., Calvert, B., Eno, S. C., Ferraioli, C., Hadley, N. J., Jabeen, S., Jeng, G. Y., Kellogg, R. G., Kunkle, J., Mignerey, A. C., Ricci-Tam, F., Shin, Y. H., Skuja, A., Tonwar, S. C., Abercrombie, D., Allen, B., Azzolini, V., Barbieri, R., Baty, A., Bi, R., Brandt, S., Busza, W., Cali, I. A., D'Alfonso, M., Demiragli, Z., Ceballos, G. Gomez, Goncharov, M., Hsu, D., Iiyama, Y., Innocenti, G. M., Klute, M., Kovalskyi, D., Lai, Y. S., Lee, Y.-J., Levin, A., Luckey, P. D., Maier, B., Marini, A. C., Mcginn, C., Mironov, C., Narayanan, S., Niu, X., Paus, C., Roland, C., Roland, G., Salfeld-Nebgen, J., Stephans, G. S. F., Tatar, K., Velicanu, D., Wang, J., Wang, T. W., Wyslouch, B., Benvenuti, A. C., Chatterjee, R. M., Evans, A., Hansen, R., Kalafut, S., Kubota, Y., Lesko, Z., Mans, J., Nourbakhsh, S., Ruckstuhl, N., Rusack, R., Turkewitz, J., Acosta, J. G., Oliveros, S., Avdeeva, E., Bloom, K., Claes, D. R., Fangmeier, C., Suarez, R. Gonzalez, Kamalieddin, R., Kravchenko, I., Monroy, J., Siado, J. E., Snow, G. R., Stieger, B., Alyari, M., Dolen, J., Godshalk, A., Harrington, C., Iashvili, I., Nguyen, D., Parker, A., Rappoccio, S., Roozbahani, B., Alverson, G., Barberis, E., Hortiangtham, A., Massironi, A., Morse, D. M., Nash, D., Orimoto, T., De Lima, R. Teixeira, Trocino, D., Wood, D., Bhattacharya, S., Charaf, O., Hahn, K. A., Mucia, N., Odell, N., Pollack, B., Schmitt, M. H., Sung, K., Trovato, M., Velasco, M., Dev, N., Hildreth, M., Anampa, K. Hurtado, Jessop, C., Karmgard, D. J., Kellams, N., Lannon, K., Loukas, N., Marinelli, N., Meng, F., Mueller, C., Musienko, Y., Planer, M., Reinsvold, A., Ruchti, R., Smith, G., Taroni, S., Wayne, M., Wolf, M., Woodard, A., Alimena, J., Antonelli, L., Bylsma, B., Durkin, L. S., Flowers, S., Francis, B., Hart, A., Hill, C., Ji, W., Liu, B., Luo, W., Puigh, D., Winer, B. L., Wulsin, H. W., Benaglia, A., Cooperstein, S., Driga, O., Elmer, R., Hardenbrook, J., Hebda, R., Higginbotham, S., Lange, D., Luo, J., Marlow, D., Mei, K., Ojalvo, I., Olsen, J., Palmer, C., Piroue, R., Stickland, D., Tully, C., Malik, S., Norberg, S., Barker, A., Barnes, V. E., Folgueras, S., Gutay, L., Jha, M. K., Jones, M., Jung, A. W., Khatiwada, A., Miller, D. H., Neumeister, N., Peng, C. C., Schulte, J. F., Sun, J., Wang, F., Xie, W., Cheng, T., Parashar, N., Stupak, J., Adair, A., Akgun, B., Chen, Z., Ecklund, K. M., Geurts, F. J. M., Guilbaud, M., Li, W., Michlin, B., Northup, M., Padley, B. P., Roberts, J., Rorie, J., Tu, Z., Zabel, J., Bodek, A., De Barbaro, R., Demina, R., Duh, Y. T., Ferbel, T., Galanti, M., Garcia-Bellido, A., Han, J., Hindrichs, O., Khukhunaishvili, A., Lo, K. H., Tan, R., Verzetti, M., Ciesielski, R., Goulianos, K., Mesropian, C., Agapitos, A., Chou, J. P., Gershtein, Y., Espinosa, T. A. Gomez, Halkiadakis, E., Heindl, M., Hughes, E., Kaplan, S., Elayavalli, R. Kunnawalkam, Kyriacou, S., Lath, A., Montalvo, R., Nash, K., Osherson, M., Saka, H., Salur, S., Schnetzer, S., Sheffield, D., Somalwar, S., Stone, R., Thomas, S., Thomassen, R., Walker, M., Delannoy, A. G., Foerster, M., Heideman, J., Riley, G., Rose, K., Spanier, S., Thapa, K., Bouhali, O., Hernandez, A. Castaneda, Celik, A., Dalchenko, M., De Mattia, M., Delgado, A., Dildick, S., Eusebi, R., Gilmore, J., Huang, T., Kamon, T., Mueller, R., Pakhotin, Y., Patel, R., Perloff, A., Pernie, L., Rathjens, D., Safonov, A., Tatarinov, A., Ulmer, K. A., Akchurin, N., Damgov, J., De Guio, F., Dudero, P. R., Faulkner, J., Gurpinar, E., Kunori, S., Lamichhane, K., Lee, S. W., Libeiro, T., Peltola, T., Undleeb, S., Volobouev, I., Wang, Z., Greene, S., Gurrola, A., Janjam, R., Johns, W., Maguire, C., Melo, A., Ni, H., Sheldon, R., Tuo, S., Velkovska, J., Xu, Q., Arenton, M. W., Barria, R., Cox, B., Hirosky, R., Ledovskoy, A., Li, H., Neu, C., Sinthuprasith, T., Sun, X., Wang, Y., Wolfe, E., Xia, F., Harr, R., Karchin, P. E., Sturdy, J., Zaleski, S., Brodski, M., Buchanan, J., Caillol, C., Dasu, S., Dodd, L., Duric, S., Gomber, B., Grothe, M., Herndon, M., Herve, A., Hussain, U., Klabbers, R., Lanaro, A., Levine, A., Long, K., Loveless, R., Pierro, G. A., Polese, G., Ruggles, T., Savin, A., Smith, N., Smith, W. H., Taylor, D., Woods, N.
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Abstract/Description: A search for long-lived particles was performed with data corresponding to an integrated luminosity of 2.6 fb(-1) collected at a center-of-mass energy of 13 TeV by the CMS experiment in 2015. The analysis exploits two customized topological trigger algorithms, and uses the multiplicity of displaced jets to search for the presence of a signal decay occurring at distances between 1 and 1000 mm. The results can be interpreted in a variety of different models. For pair-produced long-lived...
Show moreA search for long-lived particles was performed with data corresponding to an integrated luminosity of 2.6 fb(-1) collected at a center-of-mass energy of 13 TeV by the CMS experiment in 2015. The analysis exploits two customized topological trigger algorithms, and uses the multiplicity of displaced jets to search for the presence of a signal decay occurring at distances between 1 and 1000 mm. The results can be interpreted in a variety of different models. For pair-produced long-lived particles decaying to two b quarks and two leptons with equal decay rates between lepton flavors, cross sections larger than 2.5 fb are excluded for proper decay lengths between 70-100 mm for a long-lived particle mass of 1130 GeV at 95% confidence. For a specific model of pair-produced, long-lived top squarks with R-parity violating decays to a b quark and a lepton, masses below 550-1130 GeV are excluded at 95% confidence for equal branching fractions between lepton flavors, depending on the squark decay length. This mass bound is the most stringent to date for top squark proper decay lengths greater than 3 mm. (C) 2018 The Author(s). Published by Elsevier B.V.
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Date Issued: 2018-05-10
Identifier: FSU_libsubv1_wos_000432187800065, 10.1016/j.physletb.2018.03.019
Format: Citation

Title: Multistability In An Unusual Phase Diagram Induced By The Competition Between Antiferromagnetic-like Short-range And Ferromagnetic-like Long-range Interactions.
Creator: Nishino, Masamichi, Rikvold, Per Arne, Omand, Conor, Miyashita, Seiji
Abstract/Description: The interplay between competing short-range (SR) and long-range (LR) interactions can cause nontrivial structures in phase diagrams. Recently, horn-shaped unusual structures were found by Monte Carlo simulations in the phase diagram of the Ising antiferromagnet (IA) with infinite-range ferromagnetic-like (F) interactions [Phys. Rev. B 93, 064109 (2016); 96, 174428 (2017)], and also in an IA with LR interactions of elastic origin modeling spin-crossover materials [Phys. Rev. B 96, 144425 (2017...
Show moreThe interplay between competing short-range (SR) and long-range (LR) interactions can cause nontrivial structures in phase diagrams. Recently, horn-shaped unusual structures were found by Monte Carlo simulations in the phase diagram of the Ising antiferromagnet (IA) with infinite-range ferromagnetic-like (F) interactions [Phys. Rev. B 93, 064109 (2016); 96, 174428 (2017)], and also in an IA with LR interactions of elastic origin modeling spin-crossover materials [Phys. Rev. B 96, 144425 (2017)]. To clarify the nature of the phases associated with the horn structures, we study the phase diagram of the IA model with infinite-range F interactions by applying a variational free energy in a cluster mean-field (CMF) approximation. While the simple Bragg-Williams mean-field theory for each sublattice does not produce a horn structure, we find such structures with the CMF method. This confirms that the local thermal fluctuations enabled by the multisite clusters are essential for this phenomenon. We investigate in detail the structure of metastable phases in the phase diagram. In contrast to the phase diagram obtained by the Monte Carlo studies, we find a triple point, at which ferromagnetic-like, antiferromagnetic-like, and disordered phases coexist, and also six tristable regions accompanying the horn structure. We also point out that several characteristic endpoints of first-order transitions appear in the phase diagram. We propose three possible scenarios for the transitions related to the tristable regions. Finally, we discuss the relation between the triple point in this phase diagram and that of a possible lattice-gas model, in which solid, liquid, and gas phases can coexist.
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Date Issued: 2018-10-02
Identifier: FSU_libsubv1_wos_000446296400003, 10.1103/PhysRevB.98.144402
Format: Citation

Title: Magnetohydrodynamical Effects On Nuclear Deflagration Fronts In Type Ia Supernovae.
Creator: Hristov, Boyan, Collins, David C., Hoeflich, Peter, Weatherford, Charles A., Diamond, Tiara R.
Abstract/Description: This article presents a study of the effects of magnetic fields on non-distributed nuclear burning fronts as a possible solution to a fundamental problem for the thermonuclear explosion of a Chandrasekhar mass (M-Ch) white dwarf (WD), the currently favored scenario for the majority of Type Ia SNe. All existing 3D hydrodynamical simulations predict strong global mixing of the burning products due to Rayleigh-Taylor (RT) instabilities, which contradicts observations. As a first step toward...
Show moreThis article presents a study of the effects of magnetic fields on non-distributed nuclear burning fronts as a possible solution to a fundamental problem for the thermonuclear explosion of a Chandrasekhar mass (M-Ch) white dwarf (WD), the currently favored scenario for the majority of Type Ia SNe. All existing 3D hydrodynamical simulations predict strong global mixing of the burning products due to Rayleigh-Taylor (RT) instabilities, which contradicts observations. As a first step toward studying the flame physics, we present a set of computational magnet-hydrodynamic models in rectangular flux tubes, resembling a small inner region of a WD. We consider initial magnetic fields up to 10(12) G of various orientations. We find an increasing suppression of RT instabilities starting at about 10(9) G. The front speed tends to decrease with increasing magnitude up to about 1011 G. For even higher fields new small-scale, finger-like structures develop, which increase the burning speed by a factor of 3 to 4 above the fieldfree RT-dominated regime. We suggest that the new instability may provide sufficiently accelerated energy production during the distributed burning regime to go over the Chapman-Jougey limit and trigger a detonation. Finally, we discuss the possible origins of high magnetic fields during the final stage of the progenitor evolution or the explosion.
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Date Issued: 2018-05-01
Identifier: FSU_libsubv1_wos_000431051500004, 10.3847/1538-4357/aab7f2
Format: Citation

Title: Liquid-liquid Phase Separation Of Patchy Particles Illuminates Diverse Effects Of Regulatory Components On Protein Droplet Formation.
Creator: Nguemaha, Valery, Zhou, Huan-Xiang
Abstract/Description: Recently many cellular functions have been associated with membraneless organelles, or protein droplets, formed by liquid-liquid phase separation (LLPS). Proteins in these droplets often contain RNA-binding domains, but the effects of RNA on LLPS have been controversial. To gain better understanding on the roles of RNA and other macromolecular regulators, here we used Gibbs-ensemble simulations to determine phase diagrams of two-component patchy particles, as models for mixtures of proteins...
Show moreRecently many cellular functions have been associated with membraneless organelles, or protein droplets, formed by liquid-liquid phase separation (LLPS). Proteins in these droplets often contain RNA-binding domains, but the effects of RNA on LLPS have been controversial. To gain better understanding on the roles of RNA and other macromolecular regulators, here we used Gibbs-ensemble simulations to determine phase diagrams of two-component patchy particles, as models for mixtures of proteins with regulatory components. Protein-like particles have four patches, with attraction strength epsilon(PP); regulatory particles experience mutual steric repulsion but have two attractive patches toward proteins, with the strength epsilon(PR) tunable. At low epsilon(PR), the regulator, due to steric repulsion, preferentially partitions in the dispersed phase, thereby displacing the protein into the droplet phase and promoting LLPS. At moderate epsilon(PR), the regulator starts to partition and displace the protein in the droplet phase, but only to weaken bonding networks and thereby suppress LLPS. At epsilon(PR) > epsilon(PP), the enhanced bonding ability of the regulator initially promotes LLPS, but at higher amounts, the resulting displacement of the protein suppresses LLPS. These results illustrate how RNA can have disparate effects on LLPS, thus able to perform diverse functions in different organelles.
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Date Issued: 2018-04-30
Identifier: FSU_libsubv1_wos_000431104900029, 10.1038/s41598-018-25132-1
Format: Citation

Title: Neutron Skins And Neutron Stars In The Multimessenger Era.
Creator: Fattoyev, F. J., Piekarewicz, J., Horowitz, C. J.
Abstract/Description: The historical first detection of a binary neutron star merger by the LIGO-Virgo Collaboration [B. P. Abbott et al., Phys. Rev. Lett. 119, 161101 (2017)] is providing fundamental new insights into the astrophysical site for the r process and on the nature of dense matter. A set of realistic models of the equation of state (EOS) that yield an accurate description of the properties of finite nuclei, support neutron stars of two solar masses, and provide a Lorentz covariant extrapolation to...
Show moreThe historical first detection of a binary neutron star merger by the LIGO-Virgo Collaboration [B. P. Abbott et al., Phys. Rev. Lett. 119, 161101 (2017)] is providing fundamental new insights into the astrophysical site for the r process and on the nature of dense matter. A set of realistic models of the equation of state (EOS) that yield an accurate description of the properties of finite nuclei, support neutron stars of two solar masses, and provide a Lorentz covariant extrapolation to dense matter are used to confront its predictions against tidal polarizabilities extracted from the gravitational-wave data. Given the sensitivity of the gravitational-wave signal to the underlying EOS, limits on the tidal polarizability inferred from the observation translate into constraints on the neutron-star radius. Based on these constraints, models that predict a stiff symmetry energy, and thus large stellar radii, can be ruled out. Indeed, we deduce an upper limit on the radius of a 1.4M circle dot neutron star of R1.4. < 13.76 km. Given the sensitivity of the neutron-skin thickness of Pb-208 to the symmetry energy, albeit at a lower density, we infer a corresponding upper limit of about R-skin(208) less than or similar to 0.25 fm. However, if the upcoming PREX-II experiment measures a significantly thicker skin, this may be evidence of a softening of the symmetry energy at high densities-likely indicative of a phase transition in the interior of neutron stars.
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Date Issued: 2018-04-25
Identifier: FSU_libsubv1_wos_000430822000003, 10.1103/PhysRevLett.120.172702
Format: Citation

Title: Photoproduction Of K+ K- Meson Pairs On The Proton.
Creator: Lombardo, S., Battaglieri, M., Celentano, A., D'Angelo, A., De Vita, R., Filippi, A., Glazier, D. I., Hughes, S. M., Mathieu, V., Rizzo, A., Santopinto, E., Stankovic, I.,...
Show moreLombardo, S., Battaglieri, M., Celentano, A., D'Angelo, A., De Vita, R., Filippi, A., Glazier, D. I., Hughes, S. M., Mathieu, V., Rizzo, A., Santopinto, E., Stankovic, I., Szczepaniak, A. P., Watts, D., Zana, L., Adhikari, S., Akbar, Z., Avakian, H., Ball, J., Baltzell, N. A., Barion, L., Bashkanov, M., Batourine, V., Bedlinskiy, I., Biselli, A. S., Boiarinov, S., Briscoe, W. J., Burkert, V. D., Cao, F., Carman, D. S., Chatagnon, P., Chetry, T., Ciullo, G., Clark, L., Clary, B. A., Cole, P. L., Contalbrigo, M., Crede, V., Dashyan, N., De Sanctis, E., Defurne, M., Deur, A., Diehl, S., Djalali, C., Dugger, M., Dupre, R., Egiyan, H., Ehrhart, M., El Alaoui, A., El Fassi, L., Eugenio, P., Fedotov, G., Gavalian, G., Ghandilyan, Y., Gilfoyle, G. P., Giovanetti, K. L., Girod, F. X., Golovatch, E., Gothe, R. W., Griffioen, K. A., Guidal, M., Guo, L., Hafidi, K., Hakobyan, H., Harrison, N., Hattawy, M., Heddle, D., Hicks, K., Holtrop, M., Ilieva, Y., Ireland, D. G., Ishkhanov, B. S., Isupov, E. L., Jenkins, D., Jo, H. S., Johnston, S., Joo, K., Kabir, M. L., Keller, D., Khachatryan, G., Khachatryan, M., Khandaker, M., Kim, A., Kim, W., Klein, A., Klein, F. J., Kubarovsky, V., Lanza, L., Lenisa, P., Livingston, K., MacGregor, I. J. D., Marchand, D., Markov, N., McKinnon, B., Mestayer, M. D., Meyer, C. A., Meziani, Z. E., Mirazita, M., Mokeev, V., Montgomery, R. A., Camacho, C. Munoz, Nadel-Turonski, P., Niccolai, S., Niculescu, G., Osipenko, M., Ostrovidov, A. I., Paolone, M., Paremuzyan, R., Park, K., Pasyuk, E., Pogorelko, O., Price, J. W., Prok, Y., Protopopescu, D., Ripani, M., Riser, D., Ritchie, B. G., Rosner, G., Sabatie, F., Salgado, C., Schumacher, R. A., Sharabian, Y. G., Skorodumina, Iu, Smith, G. D., Sober, D. I., Sokhan, D., Sparveris, N., Strakovsky, I. I., Strauch, S., Taiuti, M., Tan, J. A., Ungaro, M., Voskanyan, H., Voutier, E., Wang, R., Wei, X., Wood, M. H., Zachariou, N., Zhang, J., Zhao, Z. W.
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Abstract/Description: The exclusive reaction gamma p -> pK(+) K- was studied in the photon energy range 3.0-3.8 GeV and momentum transfer range 0.6 < -t < 1.3 GeV2. Data were collected with the CLAS detector at the Thomas Jefferson National Accelerator Facility. In this kinematic range the integrated luminosity was approximately 20 pb(-1). The reaction was isolated by detecting the K+ and the proton in CLAS, and reconstructing the K- via the missing-mass technique. Moments of the dikaon decay angular distributions...
Show moreThe exclusive reaction gamma p -> pK(+) K- was studied in the photon energy range 3.0-3.8 GeV and momentum transfer range 0.6 < -t < 1.3 GeV2. Data were collected with the CLAS detector at the Thomas Jefferson National Accelerator Facility. In this kinematic range the integrated luminosity was approximately 20 pb(-1). The reaction was isolated by detecting the K+ and the proton in CLAS, and reconstructing the K- via the missing-mass technique. Moments of the dikaon decay angular distributions were extracted from the experimental data. Besides the dominant contribution of the phi meson in the P wave, evidence for S - P interference was found. The differential production cross sections d sigma/dt for individual waves in the mass range of the phi resonance were extracted and compared to predictions of a Regge-inspired model. This is the first time the t-dependent cross section of the S-wave contribution to the elastic K+ K- photoproduction has been measured.
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Date Issued: 2018-09-27
Identifier: FSU_libsubv1_wos_000445969800001, 10.1103/PhysRevD.98.052009
Format: Citation

Title: Quantum Anomalous Hall Insulator Stabilized By Competing Interactions.
Creator: Sur, Shouvik, Gong, Shou-Shu, Yang, Kun, Vafek, Oskar
Abstract/Description: We study the quantum phases driven by interaction in a semimetal with a quadratic band touching at the Fermi level. By combining the density matrix renormalization group (DMRG), analytical power expanded Gibbs potential method, and the weak coupling renormalization group, we study a spinless fermion system on a checkerboard lattice at half-filling, which has a quadratic band touching in the absence of interaction. In the presence of strong nearest-neighbor (V-1) and next-nearest-neighbor (V-2...
Show moreWe study the quantum phases driven by interaction in a semimetal with a quadratic band touching at the Fermi level. By combining the density matrix renormalization group (DMRG), analytical power expanded Gibbs potential method, and the weak coupling renormalization group, we study a spinless fermion system on a checkerboard lattice at half-filling, which has a quadratic band touching in the absence of interaction. In the presence of strong nearest-neighbor (V-1) and next-nearest-neighbor (V-2) interactions, we identify a site nematic insulator phase, a stripe insulator phase, and a phase separation region, in agreement with the phase diagram obtained analytically in the strong coupling limit (i.e., in the absence of fermion hopping). In the intermediate interaction regime we establish a quantum anomalous Hall phase in the DMRG as evidenced by the spontaneous time-reversal symmetry breaking and the appearance of a quantized Chern number C = 1. For weak interaction we utilize the power expanded Gibbs potential method that treats V-1 and V-2 on equal footing, as well as the weak coupling renormalization group. Our analytical results reveal that not only the repulsive V-1 interaction, but also the V-2 interaction (both repulsive and attractive), can drive the quantum anomalous Hall phase. We also determine the phase boundary in the V-1-V-2 plane that separates the semimetal from the quantum anomalous Hall state. Finally, we show that the nematic semimetal, which was proposed for vertical bar V-2 vertical bar >> V-1 at weak coupling in a previous study, is absent, and the quantum anomalous Hall state is the only weak coupling instability of the spinless quadratic band touching semimetal.
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Date Issued: 2018-09-26
Identifier: FSU_libsubv1_wos_000445726500005, 10.1103/PhysRevB.98.125144
Format: Citation

Title: A Conserved Glycine Harboring Disease-associated Mutations Permits Nmda Receptor Slow Deactivation And High Ca2+ Permeability.
Creator: Amin, Johansen B., Leng, Xiaoling, Gochman, Aaron, Zhou, Huan-Xiang, Wollmuth, Lonnie P.
Abstract/Description: A variety of de novo and inherited missense mutations associated with neurological disorders are found in the NMDA receptor M4 transmembrane helices, which are peripheral to the pore domain in eukaryotic ionotropic glutamate receptors. Subsets of these mutations affect receptor gating with dramatic effects, including in one instance halting it, occurring at a conserved glycine near the extracellular end of M4. Functional experiments and molecular dynamic simulations of constructs with and...
Show moreA variety of de novo and inherited missense mutations associated with neurological disorders are found in the NMDA receptor M4 transmembrane helices, which are peripheral to the pore domain in eukaryotic ionotropic glutamate receptors. Subsets of these mutations affect receptor gating with dramatic effects, including in one instance halting it, occurring at a conserved glycine near the extracellular end of M4. Functional experiments and molecular dynamic simulations of constructs with and without substitutions at this glycine indicate that it acts as a hinge, permitting the intracellular portion of the ion channel to laterally expand. This expansion stabilizes long-lived open states leading to slow deactivation and high Ca2+ permeability. Our studies provide a functional and structural framework for the effect of missense mutations on NMDARs at central synapses and highlight how the M4 segment may represent a pathway for intracellular modulation of NMDA receptor function.
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Date Issued: 2018-09-14
Identifier: FSU_libsubv1_wos_000444554800005, 10.1038/s41467-018-06145-w
Format: Citation

Title: Tevatron Run Ii Combination Of The Effective Leptonic Electroweak Mixing Angle.
Creator: Aaltonen, T., Abazov, V. M., Abbott, B., Acharya, B. S., Adams, M., Adams, T., Agnew, J. P., Alexeev, G. D., Alkhazov, G., Alton, A., Amerio, S., Amidei, D., Anastassov, A.,...
Show moreAaltonen, T., Abazov, V. M., Abbott, B., Acharya, B. S., Adams, M., Adams, T., Agnew, J. P., Alexeev, G. D., Alkhazov, G., Alton, A., Amerio, S., Amidei, D., Anastassov, A., Annovi, A., Antos, J., Apollinari, G., Appel, J. A., Arisawa, T., Artikov, A., Asaadi, J., Ashmanskas, W., Askew, A., Atkins, S., Auerbach, B., Augsten, K. K., Aurisano, A., Aushev, V., Aushev, Y., Avila, C., Azfar, F., Badaud, F., Badgett, W., Bae, T., Bagby, L., Baldin, B., Bandurin, D. V., Banerjee, S., Barbaro-Galtieri, A., Barberis, E., Baringer, P., Barnes, V. E., Barnett, B. A., Barria, P., Bartlett, J. F., Bartos, P., Bassler, U., Bauce, M., Bazterra, V., Bean, A., Bedeschi, F., Begalli, M., Behari, S., Bellantoni, L., Bellettini, G., Bellinger, J., Benjamin, D., Beretvas, A., Beri, S. B., Bernardi, G., Bernhard, R., Bertram, I., Besancon, M., Beuselinck, R., Bhat, P. C., Bhatia, S., Bhatnagar, V., Bhatti, A., Bland, K. R., Blazey, G., Blessing, S., Bloom, K., Blumenfeld, B., Bocci, A., Bodek, A., Boehnlein, A., Boline, D., Boos, E. E., Borisov, G., Bonoletto, D., Borysova, M., Boudreau, J., Boveia, A., Brandt, A., Brandt, O., Brigliadori, L., Brochmann, M., Brock, R., Bromberg, C., Bross, A., Brown, D., Brucken, E., Bu, X. B., Budagov, J. J., Budd, H. S., Buehler, M., Buescher, V., Bunichev, V., Burdin, S., Burkett, K., Busetto, G., Bussey, P., Buszello, C. P., Butti, P., Buzatu, A., Calamba, A., Camacho-Perez, E., Camarda, S., Campanelli, M., Canelli, F., Carls, B., Carlsmith, D., Carosi, R., Carrillo, S., Casal, B., Casarsa, M., Casey, B. C. K., Castilla-Valdez, H., Castro, A., Catastini, P., Caughron, S., Cauz, D., Cavaliere, V., Cerri, A., Cerrito, L., Chakrabarti, S., Chan, K. M., Chandra, A., Chapon, E., Chen, G., Chen, Y. C., Chertok, M., Chiarelli, G., Chlachidze, G., Cho, K., Cho, S. W., Choi, S., Chokheli, D., Choudhary, B., Cihangir, S., Claes, D., Clark, A., Clarke, C., Clutter, J., Convery, M. M. E., Conway, J., Cooke, M. M., Cooper, W. E., Corbo, M., Corcoran, M., Cordelli, M., Couderc, F., Cousinou, M.-C., Cox, C. A., Cox, D. J., Cremonesi, M., Cruz, D., Cuevas, J., Culbertson, R., Cuth, J., Cutts, D., Das, A., d'Ascenzo, N., Datta, M., Davies, G., de Barbaro, P., de Jong, S. J., De La Cruz-Burelo, E., Deliot, F., Demina, R., Demortier, L., Deninno, M., Denisov, D., Denisov, S. P., D'Errico, M., Desai, S., Deterre, C., DeVaughan, K., Devoto, F., Di Canto, A., Di Ruzza, B., Diehl, H. T., Diesburg, M., Ding, P. F., Dittmann, J. R., Dominguez, A., Donati, S., D'Onofrio, M., Dorigo, M., Driutti, A., Drutskoy, A., Dubey, A., Dudko, L. V., Duperrin, A., Dutt, S., Eads, M., Ebina, K., Edgar, R., Edmunds, D., Elagin, A., Ellison, J., Elvira, V. D., Enari, Y., Erbacher, R., Errede, S., Esham, B., Evans, H., Evdokimov, A., Evdokimov, V. N., Farrington, S., Faure, A., Feng, L., Ferbel, T., Ramos, J. P. Fernandez, Fiedler, F., Field, R., Filthaut, F., Fisher, W., Fisk, H. E., Flanagan, G., Forrest, R., Fortner, M., Fox, H., Franc, J. J., Franklin, M., Freeman, J. C., Frisch, H. H., Fuess, S., Funakoshi, Y. Y., Galloni, C., Garbincius, P. H., Garcia-Bellido, A., Garcia-Gonzalez, J. A., Garfinkel, A. F., Garosi, P., Gavrilov, V., Geng, W., Gerber, C. E., Gerberich, H., Gerchtein, E., Gershtein, Y., Giagu, S., Giakoumopoulou, V., Gibson, K., Ginsburg, C. M., Ginther, G., Giokaris, N., Giromini, P., Glagolev, V., Glenzinski, D., Gogota, O., Gold, M., Goldin, D., Golossanov, A., Golovanov, G., Gomez, G., Gomez-Ceballos, G., Goncharov, M., Lopez, O. Gonzalez, Gorelov, I., Goshaw, A. T., Goulianos, K., Gramellini, E., Grannis, P. D., Greder, S., Greenlee, H., Grenier, G., Gris, Ph, Grivaz, J.-F., Grohscjean, A., Grosso-Pilcher, C., Gruenendahl, S., Gruenewald, M. W., Guillemin, T., da Costa, J. Guimaraes, Gutierrez, G., Gutierrez, P., Hahn, S. R., Haley, J., Han, J. Y., Han, L. L., Happacher, F., Hara, K., Harder, K., Hare, M., Harel, A., Harr, R. F., Harrington-Taber, T., Hatakeyama, K., Hauptman, J. M., Hays, C., Hays, J., Head, T., Hebbeker, T., Hedin, D., Hegab, H., Heinrich, J., Heinson, A. P., Heintz, U., Hensel, C., Heredia-De La Cruz, I., Hendon, M., Herner, K., Hesketh, G., Hildreth, M. D., Hirosky, R., Huang, T., Hobbs, J. D., Hocker, A., Hoeneisen, B., Hogan, J., Hohlfeld, M., Holzbauer, J. L., Hong, Z., Hopkins, W., Hou, S., Howley, I., Hubacek, Z., Hughes, R. E., Husemann, U., Hussein, M., Huston, J., Hynek, V., Iashvili, I., Ilchenko, Y., Illingworth, R., Introzzi, G., Iori, M., Ito, A. S., Ivanov, A., Jabeen, S., Jaffre, M., James, E., Jang, D., Jayasinghe, A., Jayatilaka, B., Jeon, E. J., Jeong, M. S., Jesik, R., Jiang, P., Jindariani, S., Johns, K., Johnson, E. E., Johnson, M., Jonckheere, A. A., Jones, M., Jonsson, P., Joo, K. K., Joshi, J., Jun, S. Y., Jung, A. W., Junk, T. R., Juste, A., Kajfasz, E., Kambeitz, M., Kamon, T., Karchin, P. E., Karmanov, D., Kasmi, A., Kato, Y., Katsanos, I., Kaur, M., Kehoe, R., Kermiche, S., Ketchum, W., Keung, J., Khalatyan, N., Khanov, A., Kharchilava, A., Kharzheev, Y. N., Kilminster, B., Kim, D. H., Kim, H. S., Kim, J. E., Kim, M. J., Kim, S. H., Kim, S. B., Kim, Y. J., Kim, Y. K., Kimura, N., Kirby, M., Kiselevich, I., Kohli, J. M., Kondo, K., Kong, D. J., Konigsberg, J. J., Kotwa, A. V., Kozelov, A. V., Kraus, J., Kreps, M., Kroll, J., Kruse, M., Kuhr, T., Kumar, A., Kupco, A., Kurata, M., Kurca, T., Kuzmin, V. A., Laasanen, A. T., Lammel, S., Lammers, S., Lancaster, M., Lannon, K., Latino, G., Lebrun, P., Lee, H. S., Lee, H. S., Lee, J. S., Lee, S. W., Lee, W. M., Lei, X., Lellouch, J., Leo, S., Leone, S., Lewis, J. D., Li, D., Li, H., Li, L., Li, Q. Z., Lim, J. K., Limosani, A., Lincoln, D., Linnemann, J., Lipaev, V. V., Lipeles, E., Lipton, R., Lister, A., Liu, H., Liu, Q., Liu, T., Liu, Y., Lobodenko, A., Lockwitz, S., Loginov, A., Lokajicek, M., de Sa, R. Lopes, Lucchesi, D., Luca, A., Lueck, J., Lujan, P., Lukens, P., Luna-Garcia, R., Lungu, G., Lyon, A. L., Lys, J., Lysak, R., Maciel, A. K. A., Madar, R., Madrak, R., Maestro, P., Magana-Villalba, R., Malik, S., Malik, S., Malyshev, V. L., Manca, G., Manousakis-Katsikakis, A., Mansour, J., Marchese, L., Margaroli, F., Marino, P., Martinez-Ortega, J., Matera, K., Mattson, M. E., Mazzacane, A., Mazzanti, P., McCarthy, R., McGivern, C. L., McNulty, R., Mehta, A., Mehtala, P., Meijer, M. M., Melnitchouk, A., Menezes, D., Mercadante, P. G., Merkin, M., Mesropian, C., Meyer, A., Meyer, J., Miao, T., Miconi, F., Mietlicki, D., Mitra, A., Miyake, H., Moed, S., Moggi, N., Mondal, N. K., Moon, C. S., Moore, R., Morello, M. J., Mukherjee, A., Mulhearn, M., Muller, Th, Murat, P., Mussini, M., Nachtman, J., Nagai, Y., Naganoma, J., Nagy, E., Nakano, I., Napier, A., Narain, M., Nayyar, R., Neal, H. A., Negret, J. P., Nett, J., Neustroev, P., Nguyen, H. T., Nigmanov, T., Nodulman, L., Noh, S. Y., Nomiella, O., Nunnemann, T., Oakes, L., Oh, S. H., Oh, Y. D., Okusawa, T., Orava, R., Orduna, J., Ortolan, L., Osman, N., Pagliarone, C., Pal, A., Palencia, E., Palni, P., Papadimitriou, V., Parashar, N., Parihar, V., Park, S. K., Parker, W., Partridge, R., Parua, N., Patwa, A., Pauletta, G., Paulini, M., Paus, C., Penning, B., Perfilov, M., Peters, Y., Petridis, K., Petrillo, G., Petroff, P., Phillips, T. J., Piacentino, G., Pianori, E., Pilot, J., Pitts, K., Plager, C., Pleier, M.-A., Podstavkov, V. M., Pondrom, L., Popov, A. V., Poprocki, S. S., Potamianos, K., Pranko, A., Prewitt, M., Price, D., Prokopenko, N., Prokoshin, F., Ptohos, F., Punzi, G., Qian, J., Quadt, A., Quinn, B., Ratoff, P. 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H. L. S., Wang, S. M., Warchol, J., Waters, D., Watts, G., Wayne, M., Weichert, J., Welty-Rieger, L., Wester, W. C., Whiteson, D., Wicklund, A. B., Wilbur, S., Williams, H. H., Williams, M. R. J., Wilson, G. W., Wilson, J. S., Wilson, P., Winer, B. L., Wittich, P., Wobisch, M., Wolbers, S., Wolfmeister, H., Wood, D. R., Wright, T., Wu, X., Wu, Z., Wyatt, T. R., Xiang, Y., Xie, Y., Yamada, R., Yamamoto, K., Yamato, D., Yang, S., Yang, T., Yang, U. K., Yang, Y. C., Yao, W.-M., Yasuda, T., Yatsunenko, Y. A., Ye, W., Ye, Z., Yeh, C. P., Yi, K., Yin, H., Yip, K., Yoh, J., Yorita, K., Yoshida, T., Youn, S. W., Yu, G. B., Yu, I., Yu, J. J. M., Zanetti, A. M., Zeng, Y., Zennamo, J., Zhao, T. G., Zhou, B., Zhou, C., Zhu, J., Zielinski, M., Zieminska, D., Zivkovic, L., Zucchelli, S.
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Abstract/Description: Drell-Yan lepton pairs produced in the process p (p) over bar -> l(+)l(-) + X through an intermediate gamma*/Z boson have an asymmetry in their angular distribution related to the spontaneous symmetry breaking of the electroweak force and the associated mixing of its neutral gauge bosons. The CDF and D0 experiments have measured the effective-leptonic electroweak mixing parameter sin(2) theta(lept)(eff) using electron and muon pairs selected from the full Tevatron proton-antiproton data sets...
Show moreDrell-Yan lepton pairs produced in the process p (p) over bar -> l(+)l(-) + X through an intermediate gamma*/Z boson have an asymmetry in their angular distribution related to the spontaneous symmetry breaking of the electroweak force and the associated mixing of its neutral gauge bosons. The CDF and D0 experiments have measured the effective-leptonic electroweak mixing parameter sin(2) theta(lept)(eff) using electron and muon pairs selected from the full Tevatron proton-antiproton data sets collected in 2001-2011, corresponding to 9-10 fb(-1) of integrated luminosity. The combination of these measurements yields the most precise result from hadron colliders, sin(2)theta(lept)(eff) = 0.23148 +/- 0.00033. This result is consistent with, and approaches in precision, the best measurements from electron-positron colliders. The standard model inference of the on-shell electroweak mixing parameter sin(2) theta(W), or equivalently the W-boson mass M-W, using the ZFITTER software package yields sin(2) theta(W) = 0.22324 +/- 0.00033 or equivalently, M-W = 80.367 +/- 0.017 GeV/c(2).
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Date Issued: 2018-06-28
Identifier: FSU_libsubv1_wos_000436628000001, 10.1103/PhysRevD.97.112007
Format: Citation

Title: Static And Dynamic Signatures Of Anisotropic Electronic Phase Separation In La2/3ca1/3mno3 Thin Films Under Anisotropic Strain.
Creator: Hu, L., Yu, L. Q., Xiong, P., Wang, X. L., Zhao, J. H., Wang, L. F., Huang, Z., Wu, W. B.
Abstract/Description: The electronic phase separation (EPS) of optimally doped La2/3Ca1/3MnO3 (LCMO) thin films under various degrees of anisotropic strain is investigated by static magnetotransport and dynamic relaxation measurements. Three LCMO films were grown simultaneously on (001) NdGaO3 substrates by pulsed laser deposition, and then postgrowth annealed at 780 degrees C in O-2 for different durations of time. With increasing annealing time, the films developed significant strains of opposite signs along the...
Show moreThe electronic phase separation (EPS) of optimally doped La2/3Ca1/3MnO3 (LCMO) thin films under various degrees of anisotropic strain is investigated by static magnetotransport and dynamic relaxation measurements. Three LCMO films were grown simultaneously on (001) NdGaO3 substrates by pulsed laser deposition, and then postgrowth annealed at 780 degrees C in O-2 for different durations of time. With increasing annealing time, the films developed significant strains of opposite signs along the two orthogonal in-plane directions. The static temperature-dependent resistivity, p(T), was measured simultaneously along the two orthogonal directions. With increasing annealing time, both zero-field-cooled and field-cooled p(T) show significant increases, suggesting strain-triggered EPS and appearance of antiferromagnetic insulating (AFI) phases in a ferromagnetic metallic (FMM) ground state. Meanwhile, p(T) along the tensile-strained [010] direction becomes progressively larger than that along the compressive-strained [100]. The enhanced resistivity anisotropy indicates that the EPS is characterized by phase-separated FMM entities with a preferred orientation along [100], possibly due to the cooperative deformation and rotation/tilting of the MnO6 octahedra under the enhanced anisotropic strain. The anisotropic EPS can also be tuned by an external magnetic field. During a field cycle at several fixed temperatures, the AFI phases are melted at high fields and recovered at low fields, resulting in sharp resistance changes of ratio as high as 10(4). Furthermore, the resistivity was found to exhibit glasslike behavior, relaxing logarithmically in the phase-separated states. Fitting the data to a phenomenological model, the resulting resistive viscosity and characteristic relaxation time are found to evolve with temperature, showing a close correlation with the static measurements in the EPS states.
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Date Issued: 2018-06-25
Identifier: FSU_libsubv1_wos_000436190900003, 10.1103/PhysRevB.97.214428
Format: Citation

Title: Quench Dynamics Across Topological Quantum Phase Transitions.
Creator: Liou, Shiuan-Fan, Yang, Kun
Abstract/Description: We study the dynamics of systems quenched through topological quantum phase transitions and investigate the behavior of the bulk and edge excitations with various quench rates. Specifically, we consider the Haldane model and checkerboard model in slow quench processes with distinct band-touching structures leading to topology changes. The generation of bulk excitations is found to obey the power-law relation Kibble-Zurek and Landau-Zener theories predict. However, an anti-Kibble-Zurek...
Show moreWe study the dynamics of systems quenched through topological quantum phase transitions and investigate the behavior of the bulk and edge excitations with various quench rates. Specifically, we consider the Haldane model and checkerboard model in slow quench processes with distinct band-touching structures leading to topology changes. The generation of bulk excitations is found to obey the power-law relation Kibble-Zurek and Landau-Zener theories predict. However, an anti-Kibble-Zurek behavior is observed in the edge excitations. The mechanism of excitation generation on edge states is revealed, which explains the anti-Kibble-Zurek behavior.
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Date Issued: 2018-06-25
Identifier: FSU_libsubv1_wos_000436192300003, 10.1103/PhysRevB.97.235144
Format: Citation

Title: Topological Phase Transition In A Two-species Fermion System: Effects Of A Rotating Trap Potential Or A Synthetic Gauge Field.
Creator: Liou, Shiuan-Fan, Hu, Zi-Xiang, Yang, Kun
Abstract/Description: We numerically investigate the quantum phases and phase transition in a system made of two species of fermionic atoms that interact with each other via s-wave Feshbach resonance and are subject to rotation or a synthetic gauge field that puts the fermions at Landau level filling factor v(f) = 2. We show that the system undergoes a continuous quantum phase transition from a v(f) = 2 fermionic integer quantum Hall state formed by atoms to a v(b) = 1/2 bosonic fractional quantum Hall state...
Show moreWe numerically investigate the quantum phases and phase transition in a system made of two species of fermionic atoms that interact with each other via s-wave Feshbach resonance and are subject to rotation or a synthetic gauge field that puts the fermions at Landau level filling factor v(f) = 2. We show that the system undergoes a continuous quantum phase transition from a v(f) = 2 fermionic integer quantum Hall state formed by atoms to a v(b) = 1/2 bosonic fractional quantum Hall state formed by bosonic diatomic molecules. In the disk geometry we use, these two different topological phases are distinguished by their different gapless edge excitation spectra, and the quantum phase transition between them is signaled by the closing of the energy gap in the bulk. Comparisons will be made with field-theoretical predictions and the case of p-wave pairing.
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Date Issued: 2018-06-25
Identifier: FSU_libsubv1_wos_000436192800006, 10.1103/PhysRevB.97.245140
Format: Citation

Title: Measurement Of Angular Parameters From The Decay B-0 -> K*(0)mu(+)mu(-) In Proton-proton Collisions At Root S=8 Tev.
Creator: Sirunyan, A. M., Tumasyan, A., Adam, W., Ambrogi, F., Asilar, E., Bergauer, T., Brandstetter, J., Brondolin, E., Dragicevic, M., Eroe, J., Flechl, M., Friedl, M., Fruehwirth, R....
Show moreSirunyan, A. M., Tumasyan, A., Adam, W., Ambrogi, F., Asilar, E., Bergauer, T., Brandstetter, J., Brondolin, E., Dragicevic, M., Eroe, J., Flechl, M., Friedl, M., Fruehwirth, R., Ghete, V. M., Grossmann, J., Hrubec, J., Jeitler, M., Koenig, A., Krammer, N., Kraetschmer, I., Liko, D., Madlener, T., Mikulec, I., Pree, E., Rad, N., Rohringer, H., Schieck, J., Schoefbeck, R., Spanring, M., Spitzbart, D., Waltenberger, W., Wittmann, J., Wulz, C.-E., Zarucki, M., Chekhovsky, V., Mossolov, V., Gonzalez, J. Suarez, Abu Zeid, S., Blekman, F., D'Hondt, J., De Bruyn, I., De Clercq, J., Deroover, K., Flouris, G., Lontkovskyi, D., Lowette, S., Moortgat, S., Moreels, L., Python, Q., Skovpen, K., Tavernier, S., Van Doninck, W., Van Mulders, R., Van Parijs, I., Beghin, D., Brun, H., Clerbaux, B., De Lentdecker, G., Delannoy, H., Dorney, B., Fasanella, G., Favart, L., Goldouzian, R., Grebenyuk, A., Karapostoli, G., Lenzi, T., Luetic, J., Maerschalk, T., Marinov, A., Randle-conde, A., Seva, T., Starling, E., Vander Velde, C., Vanlaer, R., Vannerom, D., Yonamine, R., Zenoni, F., Zhang, F., Cimmino, A., Cornelis, T., Dobur, D., Fagot, A., Gul, M., Khvastunov, I., Poyraz, D., Roskas, C., Salva, S., Tytgat, M., Verbeke, W., Zaganidis, N., Bakhshiansohi, H., Bondu, O., Brochet, S., Bruno, G., Caputo, C., Caudron, A., David, R., De Visscher, S., Delaere, C., Delcourt, M., Francois, B., Giammanco, A., Komm, M., Krintiras, G., Lemaitre, V., Magitteri, A., Mertens, A., Musich, M., Piotrzkowski, K., Quertenmont, L., Saggio, A., Marono, M. Vidal, Wertz, S., Zobec, J., Beliy, N., Alda Junior, W. L., Alves, F. L., Alves, G. A., Brito, L., Correa Martins Junior, M., Hensel, C., Moraes, A., Pol, M. E., Rebello Teles, R., Belchior Batista Das Chagas, E., Carvalho, W., Chinellato, J., Coelho, E., Da Costa, E. M., Da Silveira, G. G., De Jesus Damiao, D., Fonseca De Souza, S., Huertas Guativa, L. M., Malbouisson, H., Melo De Almeida, M., Mora Herrera, C., Mundim, L., Nogima, H., Sanchez Rosas, L. J., Santoro, A., Sznajder, A., Thiel, M., Tonelli Manganote, E. J., Torres Da Silva De Araujo, F., Vilela Pereira, A., Ahuja, S., Bernardes, C. A., Fernandez Perez Tomei, T. R., Gregores, E. M., Mercadante, P. G., Novaes, S. F., Padula, Sandra S., Romero Abad, D., Ruiz Vargas, J. C., Aleksandrov, A., Hadjiiska, R., Iaydjiev, R., Misheva, M., Rodozov, M., Shopova, M., Sultanov, G., Dimitrov, A., Glushkov, I., Litov, L., Pavlov, B., Petkov, R., Fang, W., Gao, X., Yuan, L., Ahmad, M., Bian, J. G., Chen, G. M., Chen, H. S., Chen, M., Chen, Y., Jiang, C. H., Leggat, D., Liao, H., Liu, Z., Romeo, F., Shaheen, S. M., Spiezia, A., Tao, J., Wang, C., Wang, Z., Yazgan, E., Zhang, H., Zhang, S., Zhao, J., Ban, Y., Chen, G., Li, Q., Linwei, L., Liu, S., Mao, Y., Qian, S. J., Wang, D., Xu, Z., Avila, C., Cabrera, A., Chaparro Sierra, L. F., Florez, C., Gonzalez Hernandez, C. F., Ruiz Alvarez, J. D., Segura Delgado, M. A., Courbon, B., Godinovic, N., Lelas, D., Puljak, I., Cipriano, P. M. Ribeiro, Sculac, T., Antunovic, Z., Kovac, M., Brigljevic, V., Ferencek, D., Kadija, K., Mesic, B., Starodumov, A., Susa, T., Ather, M. W., Attikis, A., Mavromanolakis, G., Mousa, J., Nicolaou, C., Ptochos, F., Razis, P. A., Rykaczewski, H., Fingers, M., Finger, M., Jarrin, E. Carrera, Assran, Y., Elgammal, S., Mahrous, A., Dewanjee, R. K., Kadastik, M., Perrini, L., Raidal, M., Tiko, A., Veelken, C., Eerola, R., Kirschenmann, H., Pekkanen, J., Voutilainen, M., Havukainen, J., Heikkila, J. K., Jarvinen, T., Karimaki, V., Kinnunen, R., Lampen, T., Lassila-Perini, K., Laurila, S., Lehti, S., Linden, T., Luukka, R., Siikonen, H., Tuominen, E., Tuominiemi, J., Talvitie, J., Tuuva, T., Besancon, M., Couderc, F., Dejardin, M., Denegri, D., Faure, J. L., Ferri, F., Ganjour, S., Ghosh, S., Givernaud, A., Gras, R., de Monchenault, G. Hamel, Jarry, R., Kucher, I., Leloup, C., Locci, E., Machet, M., Malcles, J., Negro, G., Rander, J., Rosowsky, A., Sahin, M. O., Titov, M., Abdulsalam, A., Amendola, C., Antropov, I., Baffioni, S., Beaudette, F., Busson, R., Cadamuro, C., Charlot, C., de Cassagnac, R. Granier, Lisniak, M. Jo S., Lobanov, A., Blanco, J. Martin, Nguyen, M., Ochando, C., Ortona, G., Paganini, R., Pigard, R., Salerno, R., Sauvan, J. B., Sirois, Y., Leiton, A. G. Stahl, Strebler, T., Yilmaz, Y., Zabi, A., Zghiche, A., Agram, J.-L., Andrea, J., Bloch, D., Brom, J.-M., Buttignol, M., Chabert, E. 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T., Meister, D., Micheli, F., Musella, R., Nessi-Tedaldi, F., Pandolfi, F., Pata, J., Pauss, F., Perrin, G., Perrozzi, L., Quittnat, M., Reichmann, M., Becerra, D. A. Sanz, Schonenberger, M., Shchutska, L., Tavolaro, V. R., Theofilatos, K., Olsson, M. L. Vesterbacka, Wallny, R., Zhu, D. H., Aarrestad, T. K., Amsler, C., Canelli, M. F. a, De Cosa, A., Del Burgo, R., Donato, S., Galloni, C., Hreus, T., Kilminster, B., Pinna, D., Rauco, G., Robmann, R., Salerno, D., Schweiger, K., Seitz, C., Takahashi, Y., Zucchetta, A., Candelise, V., Doan, T. H., Jain, Sh, Khurana, R., Kilo, C. M., Lin, W., Pozdnyakov, A., Yu, S. S., Kumar, Arun, Chang, R., Chao, Y., Chen, K. F., Chen, P. H., Fiori, F., Hou, W.-S., Hsiung, Y., Liu, Y. F., Lu, R.-S., Paganis, E., Psallidas, A., Steen, A., Tsai, J. F., Asavapibhop, B., Kovitanggoon, K., Singh, G., Srimanobhas, N., Bakirci, M. N., Bat, A., Boran, F., Damarseckin, S., Demiroglu, Z. S., Dozen, C., Eskut, E., Girgis, S., Gokbulut, G., Guler, Y., Hos, I., Kanga, E. E., Kara, O., Kiminsu, U., Oglakci, M., Onengut, G., Ozdemir, K., Ozturk, S., Tali, B., Tok, U. G., Topakli, H., Turkcapar, S., Zorbakir, I. S., Zorbilmez, C., Bilin, B., Karapinar, G., Ocalan, K., Yalvac, M., Zeyrek, M., Gulmez, E., Kaya, M., Kaya, O., Tekten, S., Yetkin, E. A., Agaras, M. N., Atay, S., Cakir, A., Cankocak, K., Grynyov, B., Levchuk, L., Ball, F., Beck, L., Brooke, J. J., Burns, D., Clement, E., Cussans, D., Davignon, O., Flacher, H., Goldstein, J., Heath, G. P., Heath, H. F., Kreczko, L., Newbold, D. M., Paramesvaran, S., Sakuma, T., El Nasr-Storey, S. Seif, Smith, D., Smith, V. J., Bell, K. W., Belyaev, A., Brew, C., Brown, R. M., Calligaris, L., Cieri, D., Cockerill, D. J. A., Coughlan, J. A., Harder, K., Harper, S., Olaiya, E., Petyt, D., Shepherd-Themistocleous, C. H., Thea, A., Tomalin, I. R., Williams, T., Auzinger, G., Bainbridge, R., Borg, J., Breeze, S., Buchmuller, O., Bundock, A., Casasso, S., Citron, M., Colling, D., Corpe, L., Dauncey, R., Davies, G., De Wit, A., Della Negra, M., Di Maria, R., Elwood, A., Haddad, Y., Hall, G., Iles, G., James, T., Lane, R., Laner, C., Lyons, L., Magnan, A.-M., Malik, S., Mastrolorenzo, L., Matsushita, T., Nash, J., Nikitenko, A., Palladino, V., Pesaresi, M., Raymond, D. M., Richards, A., Rose, A., Scott, E., Seez, C., Shtipliyski, A., Summers, S., Tapper, A., Uchida, K., Acosta, M. Vazquez, Virdee, T., Wardle, N., Winterbottom, D., Wright, J., Zenz, S. C., Cole, J. E., Hobson, P. R., Khan, A., Kyberd, R., Reid, I. D., Symonds, R., Teodorescu, L., Turner, M., Zahid, S., Borzou, A., Call, K., Dittmann, J., Hatakeyama, K., Liu, H., Pastika, N., Smith, C., Bartek, R., Dominguez, A., Buccilli, A., Cooper, S. I., Henderson, C., Rumerio, R., West, C., Arcaro, D., Avetisyan, A., Bose, T., Gastler, D., Rankin, D., Richardson, C., Rohlf, J., Sulak, L., Zou, D., Benelli, G., Cutts, D., Garabedian, A., Hadley, M., Hakala, J., Heintz, U., Hogan, J. M., Kwok, K. H. M., Laird, E., Landsberg, G., Lee, J., Mao, Z., Narain, M., Pazzini, J., Piperov, S., Sagir, S., Syarif, R., Yu, D., Band, R., Brainerd, C., Burns, D., Sanchez, M. Calderon De La Barca, Chertok, M., Conway, J., Conway, R., Cox, P. T., Erbacher, R., Flores, C., Funk, G., Gardner, M., Ko, W., Lander, R., Mclean, C., Mulhearn, M., Pellett, D., Pilot, J., Shalhout, S., Shi, M., Smith, J., Stolp, D., Tos, K., Tripathi, M., Wang, Z., Bachtis, M., Bravo, C., Cousins, R., Dasgupta, A., Florent, A., Hauser, J., Ignatenko, M., Mccoll, N., Regnard, S., Saltzberg, D., Schnaible, C., Valuev, V., Bouvier, E., Burt, K., Clare, R., Ellison, J., Gary, J. W., Shirazi, S. M. A. Ghiasi, Hanson, G., Heilman, J., Kennedy, E., Lacroix, F., Long, O. R., Negrete, M. Olmedo, Paneva, M. I., Si, W., Wang, L., Wei, H., Wimpenny, S., Yates, B. R., Branson, J. G., Cittolin, S., Derdzinski, M., Gerosa, R., Gilbert, D., Hashemi, B., Holzner, A., Klein, D., Kole, G., Krutelyov, V., Letts, J., Macneill, I., Masciovecchio, M., Olivito, D., Padhi, S., Pieri, M., Sani, M., Sharma, V., Simon, S., Tadel, M., Vartak, A., Wasserbaech, S., Wood, J., Wurthwein, F., Yagil, A., Della Porta, G. Zevi, Amin, N., Bhandari, R., Bradmiller-Feld, J., Campagnari, C., Dishaw, A., Dutta, V., Sevilla, M. Franco, George, C., Golf, F., Gouskos, L., Gran, J., Heller, R., Incandela, J., Mullin, S. D., Ovcharova, A., Qu, H., Richman, J., Stuart, D., Suarez, I., Yoo, J., Anderson, D., Bornheim, A., Lawhorn, J. M., Newman, H. B., Nguyen, T., Pena, C., Spiropulu, M., Vlimant, J. R., Xie, S., Zhang, Z., Zhu, R. Y., Andrews, M. B., Ferguson, T., Mudholkar, T., Paulini, M., Russ, J., Sun, M., Vogel, H., Vorobiev, I., Weinberg, M., Cumalat, J. P., Ford, W. T., Jensen, F., Johnson, A., Krohn, M., Leontsinis, S., Mulholland, T., Stenson, K., Wagner, S. R., Alexander, J., Chaves, J., Chu, J., Dittmer, S., Mcdermott, K., Mirman, N., Patterson, J. R., Quach, D., Rinkevicius, A., Ryd, A., Skinnari, L., Soffi, L., Tan, S. M., Tao, Z., Thom, J., Tucker, J., Wittich, R., Zientek, M., Abdullin, S., Albrow, M., Alyari, M., Apollinari, G., Apresyan, A., Apyan, A., Banerjee, S., Bauerdick, L. A. T., Beretvas, A., Berryhill, J., Bhat, P. C., Bolla, G., Burkett, K., Butler, J. N., Canepa, A., Cerati, G. B., Cheung, H. W. K., Chlebana, F., Cremonesi, M., Duarte, J., Elvira, V. D., Freeman, J., Gecse, Z., Gottschalk, E., Gray, L., Green, D., Grunendahl, S., Gutsche, O., Harris, R. M., Hasegawa, S., Hirschauer, J., Hu, Z., Jayatilaka, B., Jindariani, S., Johnson, M., Joshi, U., Klima, B., Kreis, B., Lammel, S., Lincoln, D., Lipton, R., Liu, M., Liu, T., De Sa, R. Lopes, Lykken, J., Maeshima, K., Magini, N., Marraffino, J. M., Mason, D., McBride, R., Merkel, R., Mrenna, S., Nahn, S., O'Dell, V., Pedro, K., Prokofyev, O., Rakness, G., Ristori, L., Schneider, B., Sexton-Kennedy, E., Soha, A., Spalding, W. J., Spiegel, L., Stoynev, S., Strait, J., Strobbe, N., Taylor, L., Tkaczyk, S., Tran, N. V., Uplegger, L., Vaandering, E. W., Vernieri, C., Verzocchi, M., Vidal, R., Wang, M., Weber, H. A., Whitbeck, A., Acosta, D., Avery, R., Bortignon, R., Bourilkov, D., Brinkerhoff, A., Carnes, A., Carver, M., Curry, D., Field, R. D., Furic, I. K., Gleyzer, S. V., Joshi, B. M., Konigsberg, J., Korytov, A., Kotov, K., Ma, R., Matchev, K., Mei, H., Mitselmakher, G., Rank, D., Shi, K., Sperka, D., Terentyev, N., Thomas, L., Wang, J., Wang, S., Yelton, J., Joshi, Y. R., Linn, S., Markowitz, R., Rodriguez, J. L., Ackert, A., Adams, T., Askew, A., Hagopian, S., Hagopian, V., Johnson, K. F., Kolberg, T., Martinez, G., Perry, T., Prosper, H., Saha, A., Santra, A., Sharma, V., Yohay, R., Baarmand, M. M., Bhopatkar, V., Colafranceschi, S., Hohlmann, M., Noonan, D., Roy, T., Yumiceva, F., Adams, M. R., Apanasevich, L., Berry, D., Betts, R. R., Cavanaugh, R., Chen, X., Evdokimov, O., Gerber, C. E., Hangal, D. A., Hofman, D. J., Jung, K., Kamin, J., Gonzalez, I. D. Sandoval, Tonjes, M. B., Trauger, H., Varelas, N., Wang, H., Wu, Z., Zhang, J., Bilki, B., Clarida, W., Dilsiz, K., Durgut, S., Gandrajula, R. P., Haytmyradov, M., Khristenko, V., Merlo, J.-R., Mermerkaya, H., Mestvirishvili, A., Moeller, A., Nachtman, J., Ogul, H., Onel, Y., Ozok, F., Penzo, A., Snyder, C., Tiras, E., Wetzel, J., Yi, K., Blumenfeld, B., Cocoros, A., Eminizer, N., Fehling, D., Feng, L., Gritsan, A. V., Maksimovic, R., Roskes, J., Sarica, U., Swartz, M., Xiao, M., You, C., Al-bataineh, A., Baringer, P., Bean, A., Boren, S., Bowen, J., Castle, J., Khalil, S., Kropivnitskaya, A., Majumder, D., Mcbrayer, W., Murray, M., Royon, C., Sanders, S., Schmitz, E., Takaki, J. D. Tapia, Wang, Q., Ivanov, A., Kaadze, K., Maravin, Y., Mohammadi, A., Saini, L. K., Skhirtladze, N., Toda, S., Rebassoo, F., Wright, D., Anelli, C., Baden, A., Baron, O., Belloni, A., Calvert, B., Eno, S. C., Feng, Y., Ferraioli, C., Hadley, N. J., Jabeen, S., Jeng, G. Y., Kellogg, R. G., Kunkle, J., Mignerey, A. C., Ricci-Tam, F., Shin, Y. H., Skuja, A., Tonwar, S. C., Abercrombie, D., Allen, B., Azzolini, V., Barbieri, R., Baty, A., Bi, R., Brandt, S., Busza, W., Cali, I. A., D'Alfonso, M., Demiragli, Z., Ceballos, G. Gomez, Goncharov, M., Hsu, D., Hu, M., Iiyama, Y., Innocenti, G. M., Klute, M., Kovalskyi, D., Lai, Y. S., Lee, Y.-J., Levin, A., Luckey, P. D., Maier, B., Marini, A. C., Mcginn, C., Mironov, C., Narayanan, S., Niu, X., Paus, C., Roland, C., Roland, G., Salfeld-Nebgen, J., Stephans, G. S. F., Tatar, K., Velicanu, D., Wang, J., Wang, T. W., Wyslouch, B., Benvenuti, A. C., Chatterjee, R. M., Evans, A., Hansen, R., Hiltbrand, J., Kalafut, S., Kubota, Y., Lesko, Z., Mans, J., Nourbakhsh, S., Ruckstuhl, N., Rusack, R., Turkewitz, J., Wadud, M. A., Acosta, J. G., Oliveros, S., Avdeeva, E., Bloom, K., Claes, D. R., Fangmeier, C., Suarez, R. Gonzalez, Kamalieddin, R., Kravchenko, I., Monroy, J., Siado, J. E., Snow, G. R., Stieger, B., Dolen, J., Godshalk, A., Harrington, C., Iashvili, I., Nguyen, D., Parker, A., Rappoccio, S., Roozbahani, B., Alverson, G., Barberis, E., Hortiangtham, A., Massironi, A., Morse, D. M., Orimoto, T., De Lima, R. Teixeira, Trocino, D., Wood, D., Bhattacharya, S., Charaf, O., Hahn, K. A., Mucia, N., Odell, N., Pollack, B., Schmitt, M. H., Sung, K., Trovato, M., Velasco, M., Dev, N., Hildreth, M., Anampa, K. Hurtado, Jessop, C., Karmgard, D. J., Kellams, N., Lannon, K., Loukas, N., Marinelli, N., Meng, F., Mueller, C., Musienko, Y., Planer, M., Reinsvold, A., Ruchti, R., Smith, G., Taroni, S., Wayne, M., Wolf, M., Woodard, A., Alimena, J., Antonelli, L., Bylsma, B., Durkin, L. S., Flowers, S., Francis, B., Hart, A., Hill, C., Ji, W., Liu, B., Luo, W., Puigh, D., Winer, B. L., Wulsin, H. W., Cooperstein, S., Driga, O., Elmer, R., Hardenbrook, J., Hebda, R., Higginbotham, S., Lange, D., Luo, J., Marlow, D., Mei, K., Ojalvo, I., Olsen, J., Palmer, C., Piroue, R., Stickland, D., Tully, C., Malik, S., Norberg, S., Barker, A., Barnes, V. E., Das, S., Folgueras, S., Gutay, L., Jha, M. K., Jones, M., Jung, A. W., Khatiwada, A., Miller, D. H., Neumeister, N., Peng, C. C., Qiu, H., Schulte, J. F., Sun, J., Wang, F., Xie, W., Cheng, T., Parashar, N., Stupak, J., Adair, A., Chen, Z., Ecklund, K. M., Freed, S., Geurts, F. J. M., Guilbaud, M., Kilpatrick, M., Li, W., Michlin, B., Northup, M., Padley, B. P., Roberts, J., Rorie, J., Shi, W., Tu, Z., Zabel, J., Zhang, A., Bodek, A., de Barbaro, R., Demina, R., Duh, Y. T., Ferbel, T., Galanti, M., Garcia-Bellido, A., Han, J., Hindrichs, O., Khukhunaishvili, A., Lo, K. H., Tan, R., Verzetti, M., Ciesielski, R., Goulianos, K., Mesropian, C., Agapitos, A., Chou, J. P., Gershtein, Y., Espinosa, T. A. Gomez, Halkiadakis, E., Heindl, M., Hughes, E., Kaplan, S., Elayavalli, R. Kunnawalkam, Kyriacou, S., Lath, A., Montalvo, R., Nash, K., Osherson, M., Saka, H., Salur, S., Schnetzer, S., Sheffield, D., Somalwar, S., Stone, R., Thomas, S., Thomassen, R., Walker, M., Delannoy, A. G., Foerster, M., Heideman, J., Riley, G., Rose, K., Spanier, S., Thapa, K., Bouhali, O., Hernandez, A. Castaneda, Celik, A., Dalchenko, M., De Mattia, M., Delgado, A., Dildick, S., Eusebi, R., Gilmore, J., Huang, T., Kamon, T., Mueller, R., Pakhotin, Y., Patel, R., Perloff, A., Pernie, L., Rathjens, D., Safonov, A., Tatarinov, A., Ulmer, K. A., Akchurin, N., Damgov, J., De Guio, F., Dudero, P. R., Faulkner, J., Gurpinar, E., Kunori, S., Lamichhane, K., Lee, S. W., Libeiro, T., Mengke, T., Muthumuni, S., Peltola, T., Undleeb, S., Volobouev, I., Wang, Z., Greene, S., Gurrola, A., Janjam, R., Johns, W., Maguire, C., Melo, A., Ni, H., Padeken, K., Sheldon, R., Tuo, S., Velkovska, J., Xu, Q., Arenton, M. W., Barria, R., Cox, B., Hirosky, R., Joyce, M., Ledovskoy, A., Li, H., Neu, C., Sinthuprasith, T., Wang, Y., Wolfe, E., Xia, F., Harr, R., Karchin, P. E., Poudyal, N., Sturdy, J., Thapa, R., Zaleski, S., Brodski, M., Buchanan, J., Caillol, C., Dasu, S., Dodd, L., Duric, S., Gomber, B., Grothe, M., Herndon, M., Herve, A., Hussain, U., Klabbers, R., Lanaro, A., Levine, A., Long, K., Loveless, R., Polese, G., Ruggles, T., Savin, A., Smith, N., Smith, W. H., Taylor, D., Woods, N.
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Abstract/Description: Angular distributions of the decay B-0 -> K*(0)mu(+)mu(-) are studied using a sample of proton-proton collisions at root s = 8 TeV collected with the CMS detector at the LHC, corresponding to an integrated luminosity of 20.5 fb(-1). An angular analysis is performed to determine the P-1 and P-5' parameters, where the P-5' parameter is of particular interest because of recent measurements that indicate a potential discrepancy with the standard model predictions. Based on a sample of 1397 signal...
Show moreAngular distributions of the decay B-0 -> K*(0)mu(+)mu(-) are studied using a sample of proton-proton collisions at root s = 8 TeV collected with the CMS detector at the LHC, corresponding to an integrated luminosity of 20.5 fb(-1). An angular analysis is performed to determine the P-1 and P-5' parameters, where the P-5' parameter is of particular interest because of recent measurements that indicate a potential discrepancy with the standard model predictions. Based on a sample of 1397 signal events, the P-1 and P-5' parameters are determined as a function of the dimuon invariant mass squared. The measurements are in agreement with predictions based on the standard model. (C) 2018 The Author(s). Published by Elsevier B.V.
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Date Issued: 2018-06-10
Identifier: FSU_libsubv1_wos_000435653100067, 10.1016/j.physletb.2018.04.030
Format: Citation

Title: Constraints For The Progenitor Masses Of Historic Core-collapse Supernovae.
Creator: Williams, Benjamin F., Hillis, Tristan J., Murphy, Jeremiah W., Gilbert, Karoline, Dalcanton, Julianne J., Dolphin, Andrew E.
Abstract/Description: We age-date the stellar populations associated with 12 historic nearby core-collapse supernovae (CCSNe) and two supernova impostors; from these ages, we infer their initial masses and associated uncertainties. To do this, we have obtained new Hubble Space Telescope imaging covering these CCSNe. Using these images, we measure resolved stellar photometry for the stars surrounding the locations of the SNe. We then fit the color-magnitude distributions of this photometry with stellar evolution...
Show moreWe age-date the stellar populations associated with 12 historic nearby core-collapse supernovae (CCSNe) and two supernova impostors; from these ages, we infer their initial masses and associated uncertainties. To do this, we have obtained new Hubble Space Telescope imaging covering these CCSNe. Using these images, we measure resolved stellar photometry for the stars surrounding the locations of the SNe. We then fit the color-magnitude distributions of this photometry with stellar evolution models to determine the ages of any young existing populations present. From these age distributions, we infer the most likely progenitor masses for all of the SNe in our sample. We find ages between 4 and 50 Myr, corresponding to masses from 7.5 to 59 solar masses. There were no SNe that lacked a local young population. Our sample contains four SNe Ib/c; their masses have a wide range of values, suggesting that the progenitors of stripped-envelope SNe are binary systems. Both impostors have masses constrained to be less than or similar to 7.5 solar masses. In cases with precursor imaging measurements, we find that agedating and precursor imaging give consistent progenitor masses. This consistency implies that, although the uncertainties for each technique are significantly different, the results of both are reliable to the measured uncertainties. We combine these new measurements with those from our previous work and find that the distribution of 25 core-collapse SNe progenitor masses is consistent with a standard Salpeter power-law mass function, no upper mass cutoff, and an assumed minimum mass for core-collapse of 7.5 M-circle dot. The distribution is consistent with a minimum mass < 9.5. M-circle dot.
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Date Issued: 2018-06-10
Identifier: FSU_libsubv1_wos_000434675500011, 10.3847/1538-4357/aaba7d
Format: Citation

Title: Classification Of Symmetry Derived Pairing At The M Point In Fese.
Creator: Eugenio, P. Myles, Vafek, Oskar
Abstract/Description: Using the constraints imposed by the crystalline symmetry of FeSe and the experimentally observed phenomenology, we analyze the possible pairing symmetry of the superconducting order parameter focusing on intercalated and monolayer FeSe compounds. Such analysis leads to three possible pairing symmetry states-s wave, d wave, and helical p wave. Despite the differences in the pairing symmetry, each of these states is fully gapped with gap minimum centered above the normal state Fermi surface,...
Show moreUsing the constraints imposed by the crystalline symmetry of FeSe and the experimentally observed phenomenology, we analyze the possible pairing symmetry of the superconducting order parameter focusing on intercalated and monolayer FeSe compounds. Such analysis leads to three possible pairing symmetry states-s wave, d wave, and helical p wave. Despite the differences in the pairing symmetry, each of these states is fully gapped with gap minimum centered above the normal state Fermi surface, in agreement with photoemission data of Zhang et al. [Phys. Rev. Lett. 117, 117001 (2016)]. The analysis provides additional insights into the possible pairing mechanism for each of these states, highlighting the detrimental role of the renormalized repulsive intraorbital Hubbard U and interorbital U' and the beneficial role of the pair hopping J' and the Hund's J terms, as well as the spin-orbit coupling in the effective low-energy Hamiltonian.
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Date Issued: 2018-07-06
Identifier: FSU_libsubv1_wos_000437735000001, 10.1103/PhysRevB.98.014503
Format: Citation

Title: Sn 2017ein And The Possible First Identification Of A Type Ic Supernova Progenitor.
Creator: Van Dyk, Schuyler D., Zheng, WeiKang, Brink, Thomas G., Filippenko, Alexei V., Milisavljevic, Dan, Andrews, Jennifer E., Smith, Nathan, Cignoni, Michele, Fox, Ori D., Kelly,...
Show moreVan Dyk, Schuyler D., Zheng, WeiKang, Brink, Thomas G., Filippenko, Alexei V., Milisavljevic, Dan, Andrews, Jennifer E., Smith, Nathan, Cignoni, Michele, Fox, Ori D., Kelly, Patrick L., Adamo, Angela, Yunus, Sameen, Zhang, Keto, Kumar, Sahana
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Abstract/Description: We have identified a progenitor candidate in archival Hubble Space Telescope (HST) images for the Type Ic supernova (SN Ic) SN 2017ein in NGC 3938, pinpointing the candidate's location via HST Target of Opportunity imaging of the SN itself. This would be the first identification of a stellar-like object as a progenitor candidate for any SN Ic to date. We also present observations of SN 2017ein during the first similar to 49 days since explosion. We find that SN 2017ein most resembles the well...
Show moreWe have identified a progenitor candidate in archival Hubble Space Telescope (HST) images for the Type Ic supernova (SN Ic) SN 2017ein in NGC 3938, pinpointing the candidate's location via HST Target of Opportunity imaging of the SN itself. This would be the first identification of a stellar-like object as a progenitor candidate for any SN Ic to date. We also present observations of SN 2017ein during the first similar to 49 days since explosion. We find that SN 2017ein most resembles the well-studied SN Ic SN 2007gr. We infer that SN 2017ein experienced a total visual extinction of A(V)approximate to 1.0-1.9 mag, predominantly because of dust within the host galaxy. Although the distance is not well known, if this object is the progenitor, it was likely of high initial mass, similar to 47-48M(circle dot) if a single star, or similar to 60-80M(circle dot) if in a binary system. However, we also find that the progenitor candidate could be a very blue and young compact cluster, further implying a very massive (>65M(circle dot)) progenitor. Furthermore, the actual progenitor might not be associated with the candidate at all and could be far less massive. From the immediate stellar environment, we find possible evidence for three different populations; if the SN progenitor was a member of the youngest population, this would be consistent with an initial mass of similar to 57M(circle dot). After it has faded, the SN should be reobserved at high spatial resolution and sensitivity, to determine whether the candidate is indeed the progenitor.
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Date Issued: 2018-06-20
Identifier: FSU_libsubv1_wos_000435374600004, 10.3847/1538-4357/aac32c
Format: Citation

Title: The Progenitor Age And Mass Of The Black Hole Formation Candidate N6946-bh1.
Creator: Murphy, Jeremiah W., Khan, Rubab, Williams, Benjamin, Dolphin, Andrew E., Dalcanton, Julianne, Diaz-Rodriguez, Mariangelly
Abstract/Description: The failed supernova N6946-BH1 likely formed a black hole (BH); we age-date the surrounding population and infer an age and initial mass for the progenitor of this BH formation candidate. First, we use archival Hubble Space Telescope imaging to extract broadband photometry of the resolved stellar populations surrounding this event. Using this photometry, we fit stellar evolution models to the color-magnitude diagrams to measure the recent star formation history (SFH). Modeling the photometry...
Show moreThe failed supernova N6946-BH1 likely formed a black hole (BH); we age-date the surrounding population and infer an age and initial mass for the progenitor of this BH formation candidate. First, we use archival Hubble Space Telescope imaging to extract broadband photometry of the resolved stellar populations surrounding this event. Using this photometry, we fit stellar evolution models to the color-magnitude diagrams to measure the recent star formation history (SFH). Modeling the photometry requires an accurate distance; therefore, we measure the tip of the red giant branch and infer a distance modulus of 29.47 +/- 0.079 to NGC. 6946, or a metric distance of 7.83 +/- 0.29 Mpc. To estimate the stellar population's age, we convert the SFH and uncertainties into a probabilistic distribution for the progenitor's age. The region in the immediate vicinity of N6946-BH1 exhibits the youngest and most vigorous star formation for several hundred pc. This suggests that the progenitor is not a runaway star. From these measurements, we infer an age for the BH progenitor of 10.6(-5.9)(+14.5) Myr. Assuming that the progenitor evolved effectively as a single star, this corresponds to an initial mass of 17.9(-7.6)(+29.9) M-circle dot. Previous spectral energy distribution (SED) modeling of the progenitor suggests a mass of similar to 27M(circle dot). Formally, the SED-derived mass falls within our narrowest 68% confidence interval; however, 91% of the probability distribution function we measure lies below that mass, putting some tension between the age and the direct-imaging results.
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Date Issued: 2018-06-20
Identifier: FSU_libsubv1_wos_000435654900007, 10.3847/1538-4357/aac2be
Format: Citation

Title: Search For Excited Quarks Of Light And Heavy Flavor In Gamma Plus Jet Final States In Proton-proton Collisions At Root S=13 Tev.
Creator: Sirunyan, A. M., Tumasyan, A., Adam, W., Ambrogi, F., Asilar, E., Bergauer, T., Brandstetter, J., Brondolin, E., Dragicevic, M., Eroe, J., Flechl, M., Friedl, M., Fruehwirth, R....
Show moreSirunyan, A. M., Tumasyan, A., Adam, W., Ambrogi, F., Asilar, E., Bergauer, T., Brandstetter, J., Brondolin, E., Dragicevic, M., Eroe, J., Flechl, M., Friedl, M., Fruehwirth, R., Ghete, V. M., Grossmann, J., Hrubec, J., Jeitler, M., Koenig, A., Krammer, N., Kraetschmer, I., Liko, D., Madlener, T., Mikulec, I., Pree, E., Rad, N., Rohringer, H., Schieck, J., Schoefbeck, R., Spanring, M., Spitzbart, D., Waltenberger, W., Wittmann, J., Wulz, C.-E., Zarucki, M., Chekhovsky, V., Mossolov, V., Gonzalez, J. Suarez, De Wolf, E. A., Di Croce, D., Janssen, X., Lauwers, J., de Klundert, M. Van, Van Haevermaet, H., Van Mechelen, R., Van Remortel, N., Abu Zeid, S., Blekman, F., D'Hondt, J., De Bruyn, I., De Clercq, J., Deroover, K., Flouris, G., Lontkovskyi, D., Lowette, S., Marchesini, I., Moortgat, S., Moreels, L., Python, Q., Skovpen, K., Tavernier, S., Van Doninck, W., Van Mulders, R., Van Parijs, I., Beghin, D., Brun, H., Clerbaux, B., De Lentdecker, G., Delannoy, H., Dorney, B., Fasanella, G., Favart, L., Goldouzian, R., Grebenyuk, A., Lenzi, T., Luetic, J., Maerschalk, T., Marinov, A., Seva, T., Starling, E., Vander Velde, C., Vanlaer, R., Vannerom, D., Yonamine, R., Zenoni, F., Zhang, F., Cimmino, A., Cornelis, T., Dobur, D., Fagot, A., Gul, M., Khvastunov, I., Poyraz, D., Roskas, C., Salva, S., Tytgat, M., Verbeke, W., Zaganidis, N., Bakhshiansohi, H., Bondu, O., Brochet, S., Bruno, G., Caputo, C., Caudron, A., David, P., De Visscher, S., Delaere, C., Delcourt, M., Francois, B., Giammanco, A., Komm, M., Krintiras, G., Lemaitre, V., Magitteri, A., Mertens, A., Musich, M., Piotrzkowski, K., Quertenmont, L., Saggio, A., Marono, M. Vidal, Wertz, S., Zobec, J., Alda Junior, W. L., Alves, F. L., Alves, G. A., Brito, L., Correa Martins Junior, M., Hensel, C., Moraes, A., Pol, M. E., Rebello Teles, R., Belchior Batista Das Chagas, E., Carvalho, W., Chinellato, J., Coelho, E., Da Costa, E. M., Da Silveira, G. G., De Jesus Damiao, D., Fonseca De Souza, S., Huertas Guativa, L. M., Malbouisson, H., Melo De Almeida, M., Mora Herrera, C., Mundim, L., Nogima, H., Sanchez Rosas, L. J., Santoro, A., Sznajder, A., Thiel, M., Tonelli Manganote, E. J., Torres Da Silva De Araujo, F., Vilela Pereira, A., Ahuja, S., Bernardes, C. A., Fernandez Perez Tomei, T. R., Gregores, E. M., Mercadante, P. G., Novaes, S. F., Padula, Sandra S., Romero Abad, D., Ruiz Vargas, J. C., Aleksandrov, A., Hadjiiska, R., Iaydjiev, R., Misheva, M., Rodozov, M., Shopova, M., Sultanov, G., Dimitrov, A., Litov, L., Pavlov, B., Petkov, R., Fang, W., Gao, X., Yuan, L., Ahmad, M., Bian, J. G., Chen, G. M., Chen, H. S., Chen, M., Chen, Y., Jiang, C. H., Leggat, D., Liao, H., Liu, Z., Romeo, F., Shaheen, S. M., Spiezia, A., Tao, J., Wang, C., Wang, Z., Yazgan, E., Zhang, H., Zhang, S., Zhao, J., Ban, Y., Chen, G., Li, J., Li, Q., Liu, S., Mao, Y., Qian, S. J., Wang, D., Xu, Z., Avila, C., Cabrera, A., Chaparro Sierra, L. F., Florez, C., Gonzalez Hernandez, C. F., Ruiz Alvarez, J. D., Segura Delgado, M. A., Courbon, B., Godinovic, N., Lelas, D., Puljak, I., Cipriano, P. M. Ribeiro, Sculac, T., Antunovic, Z., Kovac, M., Brigljevic, V., Ferencek, D., Kadija, K., Mesic, B., Starodumov, A., Susa, T., Ather, M. W., Attikis, A., Mavromanolakis, G., Mousa, J., Nicolaou, C., Ptochos, F., Razis, P. A., Rykaczewski, H., Finger, M., Finger, M., Carrera Jarrin, E., El-khateeb, E., Elgammal, S., Kamel, A. Ellithi, Dewanjee, R. K., Kadastik, M., Perrini, L., Raidal, M., Tiko, A., Veelken, C., Eerola, R., Kirschenmann, H., Pekkanen, J., Voutilainen, M., Havukainen, J., Heikkila, J. K., Jarvinen, T., Karimaki, V., Kinnunen, R., Lampen, T., Lassila-Perini, K., Laurila, S., Lehti, S., Linden, T., Luukka, R., Siikonen, H., Tuominen, E., Tuominiemi, J., Tuuva, T., Besancon, M., Couderc, F., Dejardin, M., Denegri, D., Faure, J. L., Ferri, F., Ganjour, S., Ghosh, S., Gras, R., de Monchenault, G. Hamel, Jarry, P., Kucher, I., Leloup, C., Locci, E., Machet, M., Malcles, J., Negro, G., Rander, J., Rosowsky, A., Sahin, M. O., Titov, M., Abdulsalam, A., Amendola, C., Antropov, I., Baffioni, S., Beaudette, F., Busson, R., Cadamuro, L., Charlot, C., de Cassagnac, R. Granier, Jo, M., Lisniak, S., Lobanov, A., Blanco, J. Martin, Nguyen, M., Ochando, C., Ortona, G., Paganini, R., Pigard, R., Salerno, R., Sauvan, J. B., Sirois, Y., Leiton, A. G. Stahl, Strebler, T., Yilmaz, Y., Zabi, A., Zghiche, A., Agram, J.-L., Andrea, J., Bloch, D., Brom, J.-M., Buttignol, M., Chabert, E. C., Chanon, N., Collard, C., Conte, E., Coubez, X., Fontaine, J.-C., Gele, D., Goerlach, U., Jansova, M., Le Bihan, A.-C., Tonon, N., Van Hove, P., Gadrat, S., Beauceron, S., Bernet, C., Boudoul, G., Chierici, R., Contardo, D., Depasse, R., El Mamouni, H., Fay, J., Finco, L., Gascon, S., Gouzevitch, M., Grenier, G., Ille, B., Lagarde, F., Laktineh, I. B., Lethuillier, M., Mirabito, L., Pequegnot, A. L., Perries, S., Popov, A., Sordini, V., Vander Donckt, M., Viret, S., Khvedelidze, A., Tsamalaidze, Z., Autermann, C., Feld, L., Kiesel, M. K., Klein, K., Lipinski, M., Preuten, M., Schomakers, C., Schulz, J., Zhukov, V., Albert, A., Dietz-Laursonn, E., Duchardt, D., Endres, M., Erdmann, M., Erdweg, S., Esch, T., Fischer, R., Gueth, A., Hamer, M., Hebbeker, T., Heidemann, C., Hoepfner, K., Knutzen, S., Merschmeyer, M., Meyer, A., Millet, R., Mukherjee, S., Pook, T., Radziej, M., Reithler, H., Rieger, M., Scheuch, F., Teyssier, D., Thueer, S., Fluegge, G., Kargoll, B., Kress, T., Kuensken, A., Mueller, T., Nehrkorn, A., Nowack, A., Pistone, C., Pooth, O., Stahl, A., Martin, M. Aldaya, Arndt, T., Asawatangtrakuldee, C., Beernaert, K., Behnke, O., Behrens, U., Martinez, A. Bermudez, Bin Anuar, A. A., Borras, K., Botta, V., Campbell, A., Connor, P., Contreras-Campana, C., Costanza, F., Pardos, C. Diez, Eckerlin, G., Eckstein, D., Eichhorn, T., Eren, E., Gallo, E., Garcia, J. Garay, Geiser, A., Luyando, J. M. Grados, Grohsjean, A., Gunnellini, R., Guthoff, M., Harb, A., Hauk, J., Hempel, M., Jung, H., Kasemann, M., Keaveney, J., Kleinwort, C., Korol, I., Kruecker, D., Lange, W., Lelek, A., Lenz, T., Leonard, J., Lipka, K., Lohmann, W., Mankel, R., Melzer-Pellmann, I.-A., Meyer, A. B., Mittag, G., Mnich, J., Mussgiller, A., Ntomari, E., Pitzl, D., Raspereza, A., Savitskyi, M., Saxena, R., Shevchenko, R., Spannagel, S., Stefaniuk, N., Van Onsem, G. P., Walsh, R., Wen, Y., Wichmann, K., Wissing, C., Zenaiev, O., Aggleton, R., Bein, S., Blobel, V., Vignali, M. Centis, Dreyer, T., Garutti, E., Gonzalez, D., Haller, J., Hinzmann, A., Hoffmann, M., Karavdina, A., Klanner, R., Kogler, R., Kovalchuk, N., Kurz, S., Lapsien, T., Marconi, D., Meyer, M., Niedziela, M., Nowatschin, D., Pantaleo, E., Peiffer, T., Perieanu, A., Scharf, C., Schleper, R., Schmidt, A., Schumann, S., Schwandt, J., Sonneveld, J., Stadie, H., Steinbrueck, G., Stober, F. M., Stoever, M., Tholen, H., Troendle, D., Usai, E., Vanhoefer, A., Vormwald, B., Akbiyik, M., Barth, C., Baselga, M., Baur, S., Butz, E., Caspart, R., Chwalek, T., Colombo, E., De Boer, W., Dierlamm, A., Faltermann, N., Freund, B., Friese, R., Giffels, M., Harrendorf, M. A., Hartmann, F., Heindl, S. M., Husemann, U., Kassel, F., Kudella, S., Mildner, H., Mozer, M. U., Mueller, Th, Plagge, M., Quast, G., Rabbertz, K., Schroeder, M., Shvetsov, I., Sieber, G., Simonis, H. J., Ulrich, R., Wayand, S., Weber, M., Weiler, T., Williamson, S., Woehrmann, C., Wolf, R., Anagnostou, G., Daskalakis, G., Geralis, T., Kyriakis, A., Loukas, D., Topsis-Giotis, I., Karathanasis, G., Kesisoglou, S., Panagiotou, A., Saoulidou, N., Kousouris, K., Evangelou, I., Foudas, C., Gianneios, R., Katsoulis, R., Kokkas, R., Mallios, S., Manthos, N., Papadopoulos, I., Paradas, E., Strologas, J., Triantis, F. A., Tsitsonis, D., Csanad, M., Filipovic, N., Pasztor, G., Suranyi, O., Veres, G. I., Bencze, G., Hajdu, C., Horvath, D., Hunyadi, A., Sikler, F., Veszpremi, V., Beni, N., Czellar, S., Karancsi, J., Makovec, A., Molnar, J., Szillasi, Z., Bartok, M., Raics, R., Trocsanyi, Z. L., Ujvari, B., Choudhury, S., Komaragiri, J. R., Bahinipati, S., Bhowmik, S., Mal, P., Mandal, K., Nayak, A., Sahoo, D. K., Sahoo, N., Swain, S. K., Bansal, S., Beri, S. B., Bhatnagar, V., Chawla, R., Dhingra, N., Kalsi, A. K., Kaur, A., Kaur, M., Kaur, S., Kumar, R., Kumari, R., Mehta, A., Singh, J. B., Walia, G., Kumar, Ashok, Shah, Aashaq, Bhardwaj, A., Chauhan, S., Choudhary, B. C., Garg, R. B., Keshri, S., Kumar, A., Malhotra, S., Naimuddin, M., Ranjan, K., Sharma, R., Bhardwaj, R., Bhattacharya, R., Bhattacharya, S., Bhawandeep, U., Dey, S., Dutt, S., Dutta, S., Ghosh, S., Majumdar, N., Modak, A., Mondal, K., Mukhopadhyay, S., Nandan, S., Purohit, A., Roy, A., Chowdhury, S. Roy, Sarkar, S., Sharan, M., Thakur, S., Behera, P. K., Chudasama, R., Dutta, D., Jha, V., Kumar, V., Mohanty, A. K., Netrakanti, P. K., Pant, L. M., Shukla, R., Topkar, A., Aziz, T., Dugad, S., Mahakud, B., Mitra, S., Mohanty, G. B., Sur, N., Sutar, B., Banerjee, S., Bhattacharya, S., Chatterjee, S., Das, P., Guchait, M., Jain, Sa, Kumar, S., Maity, M., Majumder, G., Mazumdar, K., Sarkar, T., Wickramage, N., Chauhan, S., Dube, S., Hegde, V., Kapoor, A., Kothekar, K., Pandey, S., Rane, A., Sharma, S., Chenarani, S., Tadavani, E. Eskandari, Etesami, S. M., Khakzad, M., Najafabadi, M. Mohammadi, Naseri, M., Mehdiabadi, S. Paktinat, Hosseinabadi, F. Rezaei, Safarzadeh, B., Zeinali, M., Felcini, M., Grunewald, M., Abbrescia, M., Calabria, C., Colaleo, A., Creanza, D., Cristella, L., De Filippis, N., De Palma, M., Errico, F., Fiore, L., Iaselli, G., Lezki, S., Maggi, G., Maggi, M., Miniello, G., My, S., Nuzzo, S., Pompili, A., Pugliese, G., Radogna, R., Ranieri, A., Selvaggi, G., Sharma, A., Silvestris, L., Venditti, R., Verwilligen, R., Abbiendi, G., Battilana, C., Bonacorsi, D., Borgonovi, L., Braibant-Giacomelli, S., Campanini, R., Capiluppi, P., Castro, A., Cavallo, F. R., Chhibra, S. S., Codispoti, G., Cuffiani, M., Dallavalle, G. M., Fabbri, F., Fanfani, A., Fasanella, D., Giacomelli, R., Grandi, C., Guiducci, L., Marcellini, S., Masetti, G., Montanari, A., Navarria, F. L., Perrotta, A., Rossi, A. M., Rovelli, T., Siroli, G. P., Tosi, N., Albergo, S., Costa, S., Di Mattia, A., Giordano, F., Potenza, R., Tricomi, A., Tuve, C., Barbagli, G., Chatterjee, K., Ciulli, V., Civinini, C., D'Alessandro, R., Focardi, E., Lenzi, P., Meschini, M., Paoletti, S., Russo, L., Sguazzoni, G., Strom, D., Viliani, L., Benussi, L., Bianco, S., Fabbri, F., Piccolo, D., Primavera, F., Calvelli, V., Ferro, F., Ravera, E., Robutti, E., Tosi, S., Benaglia, A., Beschi, A., Brianza, L., Brivio, E., Ciriolo, V., Dinardo, M. E., Fiorendi, S., Gennai, S., Ghezzi, A., Govoni, R., Malberti, M., Malvezzi, S., Manzoni, R. A., Menasce, D., Moroni, L., Paganoni, M., Pauwels, K., Pedrini, D., Pigazzini, S., Ragazzi, S., de Fatis, T. Tabarelli, Buontempo, S., Cavallo, N., Di Guida, S., Fabozzi, F., Fienga, E., Iorio, A. O. M., Khan, W. A., Lista, L., Meola, S., Paolucci, R., Sciacca, C., Thyssen, F., Azzi, P., Bacchetta, N., Benato, L., Bisello, D., Boletti, A., Carlin, R., De Oliveira, A. Carvalho Antunes, Checchia, P., Manzano, P. 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A., Shoaib, M., Waqas, M., Bialkowska, H., Bluj, M., Boimska, B., Frueboes, T., Gorski, M., Kazana, M., Nawrocki, K., Szleper, M., Zalewski, R., Bunkowski, K., Byszuk, A., Doroba, K., Kalinowski, A., Konecki, M., Krolikowski, J., Misiura, M., Olszewski, M., Pyskir, A., Walczak, M., Bargassa, R., Beira Da Cruz E Silva, C., Di Francesco, A., Faccioli, R., Galinhas, B., Gallinaro, M., Hollar, J., Leonardo, N., Iglesias, L. Lloret, Nemallapudi, M. V., Seixas, J., Strong, G., Toldaiev, O., Vadruccio, D., Varela, J., Alexakhin, V., Bunin, R., Golunov, A., Golutvin, I., Gorbounov, N., Kamenev, A., Karjavin, V., Lanev, A., Malakhov, A., Matveev, V., Palichik, V., Perelygin, V., Savina, M., Shmatov, S., Shulha, S., Skatchkov, N., Smirnov, V., Zarubin, A., Ivanov, Y., Kim, V., Kuznetsova, E., Levchenko, R., Murzin, V., Oreshkin, V., Smirnov, I., Sosnov, D., Sulimov, V., Uvarov, L., Vavilov, S., Vorobyev, A., Andreev, Yu, Dermenev, A., Gninenko, S., Golubev, N., Karneyeu, A., Kirsanov, M., Krasnikov, N., Pashenkov, A., Tlisov, D., Toropin, A., Epshteyn, V., Gavrilov, V., Lychkovskaya, N., Popov, V., Pozdnyakov, I., Safronov, G., Spiridonov, A., Stepennov, A., Toms, M., Vlasov, E., Zhokin, A., Aushev, T., Bylinkin, A., Chistov, R., Danilov, M., Parygin, R., Philippov, D., Polikarpov, S., Tarkovskii, E., Andreev, V., Azarkin, M., Dremin, I., Kirakosyan, M., Terkulov, A., Baskakov, A., Belyaev, A., Boos, E., Bunichev, V., Dubinin, M., Dudko, L., Ershov, A., Gribushin, A., Klyukhin, V., Kodolova, O., Lokhtin, I., Miagkov, I., Obraztsov, S., Petrushanko, S., Savrin, V., Blinov, V., Skovpen, Y., Shtol, D., Azhgirey, I., Bayshev, I., Bitioukov, S., Elumakhov, D., Godizov, A., Kachanov, V., Kalinin, A., Konstantinov, D., Mandrik, P., Petrov, V., Ryutin, R., Sobol, A., Troshin, S., Tyurin, N., Uzunian, A., Volkov, A., Adzic, R., Cirkovic, R., Devetak, D., Dordevic, M., Milosevic, J., Rekovic, V., Alcaraz Maestre, J., Bachiller, I., Barrio Luna, M., Cerrada, M., Colino, N., De La Cruz, B., Delgado Peris, A., Escalante Del Valle, A., Fernandez Bedoya, C., Fernandez Ramos, J. P., Flix, J., Fouz, M. C., Gonzalez Lopez, O., Goy Lopez, S., Hernandez, J. M., Josa, M. I., Moran, D., Perez-Calero Yzquierdo, A., Puerta Pelayo, J., Quintario Olmeda, A., Redondo, I., Romero, L., Soares, M. S., Alvarez Fernandez, A., Albajar, C., de Troconiz, J. F., Missiroli, M., Cuevas, J., Erice, C., Fernandez Menendez, J., Gonzalez Caballero, I., Gonzalez Fernandez, J. R., Palencia Cortezon, E., Sanchez Cruz, S., Vischia, P., Vizan Garcia, J. M., Cabrillo, I. J., Calderon, A., Chazin Quero, B., Curras, E., Duarte Campderros, J., Fernandez, M., Garcia-Ferrero, J., Gomez, G., Lopez Virto, A., Marco, J., Martinez Rivero, C., Martinez Ruiz del Arbol, R., Matorras, F., Piedra Gomez, J., Rodrigo, T., Ruiz-Jimeno, A., Scodellaro, L., Trevisani, N., Vila, I., Vilar Cortabitarte, R., Abbaneo, D., Akgun, B., Auffray, E., Baillon, P., Ball, A. H., Barney, D., Bendavid, J., Bianco, M., Bloch, P., Bocci, A., Botta, C., Camporesi, T., Castello, R., Cepeda, M., Cerminara, G., Chapon, E., Chen, Y., d'Enterria, D., Dabrowski, A., Daponte, V., David, A., De Gruttola, M., De Roeck, A., Deelen, N., Dobson, M., du Pree, T., Duenser, M., Dupont, N., Elliott-Peisert, A., Everaerts, R., Fallavollita, F., Franzoni, G., Fulcher, J., Funk, W., Gigi, D., Gilbert, A., Gill, K., Glege, F., Gulhan, D., Harris, P., Hegeman, J., Innocente, V., Jafari, A., Janot, P., Karacheban, O., Kieseler, J., Knunz, V., Kornmayer, A., Kortelainen, M. J., Krammer, M., Lange, C., Lecoq, P., Lourenco, C., Lucchini, M. T., Malgeri, L., Mannelli, M., Martelli, A., Meijers, F., Merlin, J. A., Mersi, S., Meschi, E., Milenovic, R., Moortgat, F., Mulders, M., Neugebauer, H., Ngadiuba, J., Orfanelli, S., Orsini, L., Pape, L., Perez, E., Peruzzi, M., Petrilli, A., Petrucciani, G., Pfeiffer, A., Pierini, M., Rabady, D., Racz, A., Reis, T., Rolandi, G., Rovere, M., Sakulin, H., Schafer, C., Schwick, C., Seidel, M., Selvaggi, M., Sharma, A., Silva, P., Sphicas, P., Stakia, A., Steggemann, J., Stoye, M., Tosi, M., Treille, D., Triossi, A., Tsirou, A., Veckalns, V., Verweij, M., Zeuner, W. D., Bertl, W., Caminada, L., Deiters, K., Erdmann, W., Horisberger, R., Ingram, Q., Kaestli, H. C., Kotlinski, D., Langenegger, U., Rohe, T., Wiederkehr, S. A., Backhaus, M., Bani, L., Berger, P., Bianchini, L., Casal, B., Dissertori, G., Dittmar, M., Donega, M., Dorfer, C., Grab, C., Heidegger, C., Hits, D., Hoss, J., Kasieczka, G., Klijnsma, T., Lustermann, W., Mangano, B., Marionneau, M., Meinhard, M. 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M., Hasegawa, S., Hirschauer, J., Hu, Z., Jayatilaka, B., Jindariani, S., Johnson, M., Joshi, U., Klima, B., Kreis, B., Lammel, S., Lincoln, D., Lipton, R., Liu, M., Liu, T., De Sa, R. Lopes, Lykken, J., Maeshima, K., Magini, N., Marraffino, J. M., Mason, D., McBride, R., Merkel, R., Mrenna, S., Nahn, S., O'Dell, V., Pedro, K., Prokofyev, O., Rakness, G., Ristori, L., Schneider, B., Sexton-Kennedy, E., Soha, A., Spalding, W. J., Spiegel, L., Stoynev, S., Strait, J., Strobbe, N., Taylor, L., Tkaczyk, S., Tran, N. V., Uplegger, L., Vaandering, E. W., Vernieri, C., Verzocchi, M., Vidal, R., Wang, M., Weber, H. A., Whitbeck, A., Acosta, D., Avery, P., Bortignon, P., Bourilkov, D., Brinkerhoff, A., Carnes, A., Carver, M., Curry, D., Field, R. D., Furic, I. K., Gleyzer, S. V., Joshi, B. M., Konigsberg, J., Korytov, A., Kotov, K., Ma, P., Matchev, K., Mei, H., Mitselmakher, G., Shi, K., Sperka, D., Terentyev, N., Thomas, L., Wang, J., Wang, S., Yelton, J., Joshi, Y. 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E., Poudyal, N., Sturdy, J., Thapa, P., Zaleski, S., Brodski, M., Buchanan, J., Caillol, C., Dasu, S., Dodd, L., Duric, S., Gomber, B., Grothe, M., Herndon, M., Herve, A., Hussain, U., Klabbers, P., Lanaro, A., Levine, A., Long, K., Loveless, R., Ruggles, T., Savin, A., Smith, N., Smith, W. H., Taylor, D., Woods, N.
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Abstract/Description: A search is presented for excited quarks of light and heavy flavor that decay to gamma + jet final states. The analysis is based on data corresponding to an integrated luminosity of 35.9 fb(-1) collected by the CMS experiment in proton-proton collisions at root s = 13 TeV at the LHC. A signal would appear as a resonant contribution to the invariant mass spectrum of the gamma + jet system, above the background expected from standard model processes. No resonant excess is found, and upper...
Show moreA search is presented for excited quarks of light and heavy flavor that decay to gamma + jet final states. The analysis is based on data corresponding to an integrated luminosity of 35.9 fb(-1) collected by the CMS experiment in proton-proton collisions at root s = 13 TeV at the LHC. A signal would appear as a resonant contribution to the invariant mass spectrum of the gamma + jet system, above the background expected from standard model processes. No resonant excess is found, and upper limits are set on the product of the excited quark cross section and its branching fraction as a function of its mass. These are the most stringent limits to date in the gamma + jet final state, and exclude excited light quarks with masses below 5.5 TeV and excited b quarks with masses below 1.8 TeV, assuming standard model like coupling strengths. (C) 2018 The Author(s). Published by Elsevier B.V.
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Date Issued: 2018-06-10
Identifier: FSU_libsubv1_wos_000435653100051, 10.1016/j.physletb.2018.04.007
Format: Citation

Title: Effects Of Stuffing On The Atomic And Electronic Structure Of The Pyrochlore Yb2ti2o7.
Creator: Ghosh, Soham S., Manousakis, Efstratios
Abstract/Description: There are reasons to believe that the ground state of the magnetic rare-earth pyrochlore Yb(2)Ti2O(7) is on the boundary between competing ground states. We have carried out ab initio density functional calculations to determine the most stable chemical formula as a function of the oxygen chemical potential and the likely location of the oxygen atoms in the unit cell of the "stuffed" system. We find that it is energetically favorable in the stuffed crystal (with an Yb replacement on a Ti site...
Show moreThere are reasons to believe that the ground state of the magnetic rare-earth pyrochlore Yb(2)Ti2O(7) is on the boundary between competing ground states. We have carried out ab initio density functional calculations to determine the most stable chemical formula as a function of the oxygen chemical potential and the likely location of the oxygen atoms in the unit cell of the "stuffed" system. We find that it is energetically favorable in the stuffed crystal (with an Yb replacement on a Ti site) to contain oxygen vacancies which dope the Yb 4f orbitals and qualitatively change the electronic properties of the system. In addition, with the inclusion of the contribution of spin-orbit coupling (SOC) on top of the GGA + U approach, we investigated the electronic structure and the magnetic moments of the most stable stuffed system. In our determined stuffed structure the valence bands as compared to those of the pure system are pushed down and a change in hybridization between the O 2p orbitals and the metal ion states is found. Our first-principle findings should form a foundation for effective models describing the low-temperature properties of this material whose true ground state remains controversial.
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Date Issued: 2018-06-11
Identifier: FSU_libsubv1_wos_000434762500006, 10.1103/PhysRevB.97.245117
Format: Citation

National High Magnetic Field Laboratory (55)	+ -
Institute of Molecular Biophysics (14)	+ -
Department of Chemical and Biomedical Engineering (3)	+ -
Department of Chemistry and Biochemistry (3)	+ -
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Gershtein, Y. (23)	+ -
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