Shell-model studies of the astrophysical rp reaction 29P(p, y)30 S

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dc.contributor.authorRichter, W. A.
dc.contributor.authorBrown, B. Alex
dc.date.accessioned2017-07-25T10:17:57Z
dc.date.available2017-07-25T10:17:57Z
dc.date.issued2013
dc.description.abstractWe present results for levels in 30S (the mirror nucleus of 30Si) that are used for the 29P(p,γ ) rp reaction rate calculations. The resonance energies used in the reaction rate calculations are based on recent measurements which extend the excitation energy spectrum. The levels are checked against results from the isobaric mass multiplet equation and the binding energies of the T = 1 analog states. Where the analog states are not known the levels are calculated with two-body interactions that use the sd-shell interactions USDA and USDB as the charge-independent parts, with a Coulomb, charge-dependent, and charge-asymmetric Hamiltonian added. The γ -decay lifetimes and 29P to 30S spectroscopic factors are also calculated with the same interactions, and together with experimental information on the levels of excited states are used to determine the 29P(p,γ )30S reaction rates.en_US
dc.description.accreditationWeb of Science
dc.identifier.citationRichter, W. A. & Brown, B. A. (2013). Shell-model studies of the astrophysical rp reaction 29P(p, y)30 S. Physical Review C, 87 (065803): 1-7en_US
dc.identifier.issn0556-2813
dc.identifier.urihttp://hdl.handle.net/10566/3107
dc.language.isoenen_US
dc.publisherAmerican Physical Societyen_US
dc.rightsPublisher retains copyright. Authors may archive the published version in their institutional repository.
dc.source.urihttp://dx.doi.org/10.1103/PhysRevC.87.065803
dc.subjectShell-model studiesen_US
dc.subjectAstrophysicalen_US
dc.subjectReactionen_US
dc.subjectUSDAen_US
dc.subjectUSDBen_US
dc.titleShell-model studies of the astrophysical rp reaction 29P(p, y)30 Sen_US
dc.typeArticleen_US

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