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Some of the material in is restricted to members of the community. By logging in, you may be able to gain additional access to certain collections or items. If you have questions about access or logging in, please use the form on the Contact Page.
Excited states in the neutron-rich isotopes P-33 and P-34 were populated by the O-18 + O-18 fusion-evaporation reaction at E-lab = 24 MeV. The Gammasphere array was used along with the Microball particle detector array to detect gamma...
The Be-9(C-14, alpha gamma) reaction at E-Lab = 30 and 35 MeV was used to study excited states of O-19. The Florida State University (FSU) gamma detector array was used to detect gamma radiation in coincidence with charged particles...
The Ar-34(alpha, p)K-37 reaction is believed to be one of the last in a sequence of (alpha, p) and (p, gamma) reactions within the T-z = -1, sd-shell nuclei, known as the alpha p-process. This process is expected to influence the shape...
The S-30(alpha, p)Cl-33 reaction has been identified in several type-1 x-ray burst (XRB) sensitivity studies as a significant reaction within the alpha p process, possibly influencing not only the abundances of burst ashes but also the...
The emission of gamma rays from neutron-bound and neutron-unbound states in Mo-95, populated in the Mo-94(d, p) reaction, has been investigated. Charged particles and gamma radiation were detected with arrays of annular silicon and...
Background: Clustering plays an important role in the structure of Be-10. Exotic molecular-like configurations, such as alpha:2n:alpha, have been suggested at relatively low excitation energies. Purpose: To search for the high-spin...
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