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dc.contributor.authorSimon, A.
dc.contributor.authorSpyrou, A.
dc.contributor.authorQuinn, S.J.
dc.contributor.authorLin, L.-Y.
dc.contributor.authorStefanek, B.
dc.contributor.authorRauscher, T.
dc.contributor.authorFröhlich, C.
dc.contributor.authorBattaglia, A.
dc.contributor.authorBest, A.
dc.contributor.authorBucher, B.
dc.contributor.authorCouder, M.
dc.contributor.authorFang, X.
dc.contributor.authorGörres, J.
dc.contributor.authorKontos, A.
dc.contributor.authorLi, Q.
dc.contributor.authorLong, A.
dc.contributor.authorLyons, S.
dc.contributor.authorRoberts, A.
dc.contributor.authorRobertson, D.
dc.contributor.authorSmith, K.
dc.contributor.authorSmith, M.K.
dc.contributor.authorStech, E.
dc.contributor.authorTan, W.P.
dc.contributor.authorTang, X.D.
dc.contributor.authorWiescher, M.
dc.contributor.authorDeyoung, P.A.
dc.date.accessioned2013-06-11T13:30:48Z
dc.date.available2013-06-11T13:30:48Z
dc.date.issued2013-05-09
dc.identifier.citationSimon , A , Spyrou , A , Quinn , S J , Lin , L-Y , Stefanek , B , Rauscher , T , Fröhlich , C , Battaglia , A , Best , A , Bucher , B , Couder , M , Fang , X , Görres , J , Kontos , A , Li , Q , Long , A , Lyons , S , Roberts , A , Robertson , D , Smith , K , Smith , M K , Stech , E , Tan , W P , Tang , X D , Wiescher , M & Deyoung , P A 2013 , ' Systematic study of (p,γ) reactions on Ni isotopes ' , Physical Review C , vol. 87 , no. 5 , 055802 . https://doi.org/10.1103/PhysRevC.87.055802
dc.identifier.issn2469-9985
dc.identifier.otherPURE: 1875607
dc.identifier.otherPURE UUID: 1428a25c-0ab4-4e70-be29-ac016080d466
dc.identifier.otherScopus: 84877895532
dc.identifier.urihttp://hdl.handle.net/2299/10749
dc.description.abstractA systematic study of the radiative proton capture reaction for all stable nickel isotopes is presented. The results were obtained using 2.0-6.0 MeV protons from the 11-MV tandem Van de Graaff accelerator at the University of Notre Dame. The γ rays were detected by the NSCL-SuN detector utilizing the γ-summing technique. The results are compared to a compilation of earlier measurements and discrepancies between the previous data are resolved. The experimental results are also compared to the theoretical predictions obtained using the non-smoker and smaragd codes. Based on these comparisons an improved set of astrophysical reaction rates is proposed for the (p,γ) reactions on the stable nickel isotopes as well as for the 56Ni(p,γ)57Cu reaction.en
dc.format.extent11
dc.language.isoeng
dc.relation.ispartofPhysical Review C
dc.rightsOpen
dc.titleSystematic study of (p,γ) reactions on Ni isotopesen
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.identifier.urlhttp://www.scopus.com/inward/record.url?scp=84877895532&partnerID=8YFLogxK
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dc.description.versiontypeFinal Accepted Version
dcterms.dateAccepted2013-05-09
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1103/PhysRevC.87.055802
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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