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dc.contributor.authorHarissopulos, S.
dc.contributor.authorSkreti, E.
dc.contributor.authorTsagari, P.
dc.contributor.authorSouliotis, G.
dc.contributor.authorDemetriou, P.
dc.contributor.authorParadellis, T.
dc.contributor.authorHammer, J.W.
dc.contributor.authorKunz, R.
dc.contributor.authorAngulo, C.
dc.contributor.authorGoriely, S.
dc.contributor.authorRauscher, T.
dc.date.accessioned2013-05-09T07:55:00Z
dc.date.available2013-05-09T07:55:00Z
dc.date.issued2001-11
dc.identifier.citationHarissopulos , S , Skreti , E , Tsagari , P , Souliotis , G , Demetriou , P , Paradellis , T , Hammer , J W , Kunz , R , Angulo , C , Goriely , S & Rauscher , T 2001 , ' Cross section measurements of the Nb-93(p,gamma)Mo-94 reaction at E-p=1.4-4.9 MeV relevant to the nucleosynthetic p process ' , Physical Review C , vol. 64 , no. 5 , 055804 . https://doi.org/10.1103/PhysRevC.64.055804
dc.identifier.issn2469-9985
dc.identifier.otherPURE: 1633561
dc.identifier.otherPURE UUID: 4616c1c9-e891-4335-9235-1d64327110f5
dc.identifier.otherWOS: 000172077000063
dc.identifier.otherScopus: 14344271138
dc.identifier.urihttp://hdl.handle.net/2299/10660
dc.description.abstractIn-beam cross section measurements of the Nb-93(p,gamma)Mo-94 reaction have been carried out at E-p = 1.4-4.9 MeV, by using high efficiency high-purity Ge detectors, partly with BGO shields for Compton background suppression. From the resulting cross sections, which lie in the 0.5-300 mub range, astrophysical S factors as well as reaction rates have been obtained. By means of the statistical compound nucleus theory of Hauser and Feshbach, cross sections and reactions rates have also been calculated. A good agreement between the experimental data and the theoretical predictions has been found.en
dc.format.extent9
dc.language.isoeng
dc.relation.ispartofPhysical Review C
dc.subjectISOTOPES
dc.subjectMODEL
dc.subjectENERGIES
dc.subjectRATES
dc.subjectNUCLEAR-LEVEL DENSITY
dc.subjectLIGHT
dc.subjectASTROPHYSICS
dc.titleCross section measurements of the Nb-93(p,gamma)Mo-94 reaction at E-p=1.4-4.9 MeV relevant to the nucleosynthetic p processen
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.dateAccepted2001-11
rioxxterms.versionofrecordhttps://doi.org/10.1103/PhysRevC.64.055804
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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