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dc.contributor.authorOzkan, N.
dc.contributor.authorMurphy, A.S.J.
dc.contributor.authorBoyd, R.N.
dc.contributor.authorCole, A.L.
dc.contributor.authorFamiano, A.
dc.contributor.authorGuray, R. T.
dc.contributor.authorHoward, M.
dc.contributor.authorSahin, L.
dc.contributor.authorZach, J.J.
dc.contributor.authordeHaan, R.
dc.contributor.authorGorres, J.
dc.contributor.authorWiescher, M.
dc.contributor.authorIslam, M.S.
dc.contributor.authorRauscher, T.
dc.date.accessioned2013-09-26T09:15:09Z
dc.date.available2013-09-26T09:15:09Z
dc.date.issued2002-11-18
dc.identifier.citationOzkan , N , Murphy , A S J , Boyd , R N , Cole , A L , Famiano , A , Guray , R T , Howard , M , Sahin , L , Zach , J J , deHaan , R , Gorres , J , Wiescher , M , Islam , M S & Rauscher , T 2002 , ' Cross section measurements of the Pd-102(p, gamma)Ag-103 Sn-116(p, gamma)Sb-117, and Sn-112(alpha, gamma)Te-116 reactions relevant to the astrophysical rp- and gamma-processes ' Nuclear Physics A , vol. 710 , no. 3-4 , pp. 469-485 .
dc.identifier.issn0375-9474
dc.identifier.otherPURE: 1632779
dc.identifier.otherPURE UUID: 315f3d60-2e4f-4cc0-b12a-df7c0e31f4ff
dc.identifier.otherWOS: 000178919800011
dc.identifier.otherScopus: 18744427537
dc.identifier.urihttp://hdl.handle.net/2299/11663
dc.descriptionPII: S0375-9474(02)01134-X
dc.description.abstractTotal cross section measurements for the Pd-102(p, gamma)Ag-103 and Sn-116(p, gamma)Sb-117 reactions have been performed in the proton energy range 2.6 to 4.25 MeV, and for the Sn-112(alpha,gamma)T-116, reaction over the alpha beam energy range 7.0 to 10.5 MeV. An activation technique was used in which gamma rays from decays of the reaction products were detected off-line by two hyper-pure germanium detectors in a low background environment. Where possible, reaction rates are derived and the results compared to those of calculations generated by the NON-SMOKER and the MOST statistical model codes so as to judge their applicability for describing the cross sections needed for network calculations of nucleosynthesis in explosive astrophysical environments via the gamma- and rp-processes. (C) 2002 Elsevier Science B.V. All rights reserved.en
dc.format.extent17
dc.language.isoeng
dc.relation.ispartofNuclear Physics A
dc.subjectastrophysical S-factors
dc.subjectRATES
dc.subjectproton radiative
dc.subjectnuclear cross sections
dc.subjectgamma-process
dc.subjectcapture reactions
dc.subjectrp-process
dc.subjectP-PROCESS
dc.titleCross section measurements of the Pd-102(p, gamma)Ag-103 Sn-116(p, gamma)Sb-117, and Sn-112(alpha, gamma)Te-116 reactions relevant to the astrophysical rp- and gamma-processesen
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
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstyperestrictedAccess


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