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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.accessioned2013-07-02T12:47:08Z
dc.date.available2013-07-02T12:47:08Z
dc.date.issued2003-05-05
dc.identifier.citationHoroi , M , Jora , R , Zelevinsky , V , Murphy , A S , Boyd , R N & Rauscher , T 2003 , ' The V-45(p,gamma) thermonuclear reaction rate relevant to Ti-44 production rate in core-collapsed supernovae : a shell model analysis ' , Nuclear Physics A , vol. 718 , pp. 502C-504C . https://doi.org/10.1016/S0375-9474(03)00870-4
dc.identifier.issn0375-9474
dc.identifier.otherPURE: 1632115
dc.identifier.otherPURE UUID: e1403358-332b-4e96-9e7e-9c5e7809eae5
dc.identifier.otherWOS: 000182314300096
dc.identifier.otherScopus: 0038586450
dc.identifier.urihttp://hdl.handle.net/2299/11018
dc.format.extent3
dc.language.isoeng
dc.relation.ispartofNuclear Physics A
dc.subjectNUCLEOSYNTHESIS
dc.titleThe V-45(p,gamma) thermonuclear reaction rate relevant to Ti-44 production rate in core-collapsed supernovae : a 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.dateAccepted2003-05-05
rioxxterms.versionofrecordhttps://doi.org/10.1016/S0375-9474(03)00870-4
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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