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dc.contributor.authorGyurky, Gy.
dc.contributor.authorFulop, Zs.
dc.contributor.authorSomorjai, E.
dc.contributor.authorKokkoris, M.
dc.contributor.authorGalanopoulos, S.
dc.contributor.authorDemetriou, P.
dc.contributor.authorHarissopulos, S.
dc.contributor.authorRauscher, T.
dc.contributor.authorGoriely, S.
dc.date.accessioned2013-07-02T10:47:04Z
dc.date.available2013-07-02T10:47:04Z
dc.date.issued2003-11
dc.identifier.citationGyurky , G , Fulop , Z , Somorjai , E , Kokkoris , M , Galanopoulos , S , Demetriou , P , Harissopulos , S , Rauscher , T & Goriely , S 2003 , ' Proton induced reaction cross section measurements on Se isotopes for the astrophysical p process ' Physical Review C , vol. 68 , no. 5 , 055803 . https://doi.org/10.1103/PhysRevC.68.055803
dc.identifier.issn2469-9985
dc.identifier.otherPURE: 1631404
dc.identifier.otherPURE UUID: bf2316ed-b5dc-4084-88b3-1c758db620e7
dc.identifier.otherWOS: 000187578300068
dc.identifier.otherScopus: 0842346955
dc.identifier.urihttp://hdl.handle.net/2299/11007
dc.description.abstractAs a continuation of a systematic study of reactions relevant to the astrophysical p process, the cross sections of the Se-74,Se-76(p,gamma) Br-75,Br-77 and Se-82(p,n) Br-82 reactions have been measured at energies from 1.3 to 3.6 MeV using an activation technique. The results are compared to the predictions of Hauser-Feshbach statistical model calculations using the NON-SMOKER andMOST codes. The sensitivity of the calculations to variations in the optical proton potential and the nuclear level density was studied. Good agreement between theoretical and experimental reaction rates was found for the reactions Se-74(p,gamma) Br-75 and Se-82(p,n) Br-82 .en
dc.format.extent9
dc.language.isoeng
dc.relation.ispartofPhysical Review C
dc.rights/dk/atira/pure/core/openaccesspermission/open
dc.subjectNUCLEAR
dc.subjectSTARS
dc.subjectSTATISTICAL-MODEL CALCULATIONS
dc.subjectENERGIES
dc.subjectII SUPERNOVAE
dc.subjectRELEVANT
dc.subjectRP
dc.subjectNUCLEOSYNTHESIS
dc.subjectGAMMA-PROCESSES
dc.subjectREACTION-RATES
dc.titleProton induced reaction cross section measurements on Se isotopes for the astrophysical 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
dc.description.versiontypeSubmitted Version
rioxxterms.versionSMUR
rioxxterms.versionofrecordhttps://doi.org/10.1103/PhysRevC.68.055803
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstyperestrictedAccess


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