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dc.contributor.authorHoroi, M.
dc.contributor.authorJora, R.
dc.contributor.authorZelevinsky, V.
dc.contributor.authorMurphy, A.S.
dc.contributor.authorBoyd, R.N.
dc.contributor.authorRauscher, T.
dc.date.accessioned2013-05-07T13:35:01Z
dc.date.available2013-05-07T13:35:01Z
dc.date.issued2002-07
dc.identifier.citationHoroi , M , Jora , R , Zelevinsky , V , Murphy , A S , Boyd , R N & Rauscher , T 2002 , ' V-45(p,gamma) thermonuclear reaction rate relevant to Ti-44 production in core-collapse supernovae : General estimates and shell model analysis ' , Physical Review C , vol. 66 , no. 1 , 015801 . https://doi.org/10.1103/PhysRevC.66.015801
dc.identifier.issn2469-9985
dc.identifier.otherPURE: 1633165
dc.identifier.otherPURE UUID: 42553e68-f2de-465c-947b-2a70e3821ce1
dc.identifier.otherWOS: 000177529700060
dc.identifier.otherScopus: 4243727963
dc.identifier.urihttp://hdl.handle.net/2299/10643
dc.description.abstractThe lack of knowledge of the V-45(p,gamma) reaction rate has been shown to contribute a large uncertainty to the production of Ti-44 in core-collapse supernovae. By considering likely contributions from resonances associated with Cr-46 states that are the isobaric analog of states in Ti-46, we have determined that the currently accepted value of the V-45(p,gamma) reaction rate is unlikely to be inaccurate by more than an order of magnitude. These conclusions are confirmed by the shell model calculations with the FPD6 effective interaction.en
dc.format.extent7
dc.language.isoeng
dc.relation.ispartofPhysical Review C
dc.subjectRAY LINE EMISSION
dc.subjectHALF-LIFE
dc.subjectASTROPHYSICAL REACTION-RATES
dc.subjectPROBE
dc.subjectNUCLEOSYNTHESIS
dc.titleV-45(p,gamma) thermonuclear reaction rate relevant to Ti-44 production in core-collapse supernovae : General estimates and shell model analysisen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted2002-07
rioxxterms.versionofrecordhttps://doi.org/10.1103/PhysRevC.66.015801
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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