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dc.contributor.authorDillmann, I.
dc.contributor.authorRauscher, T.
dc.contributor.authorHeil, M.
dc.contributor.authorKaeppeler, F.
dc.contributor.authorRapp, W.
dc.contributor.authorThielemann, F-K
dc.date.accessioned2013-09-26T09:00:11Z
dc.date.available2013-09-26T09:00:11Z
dc.date.issued2008-01
dc.identifier.citationDillmann , I , Rauscher , T , Heil , M , Kaeppeler , F , Rapp , W & Thielemann , F-K 2008 , ' p-Process simulations with a modified reaction library ' , Journal of Physics G: Nuclear and Particle Physics , vol. 35 , no. 1 , 014029 . https://doi.org/10.1088/0954-3899/35/1/014029
dc.identifier.issn0954-3899
dc.identifier.otherPURE: 1622455
dc.identifier.otherPURE UUID: 9f7ceca0-cb22-4090-8896-972bfcfadaeb
dc.identifier.otherWOS: 000252019800030
dc.identifier.otherScopus: 38849086765
dc.identifier.urihttp://hdl.handle.net/2299/11659
dc.description.abstractWe have performed p-process simulations with the most recent stellar (n, gamma) cross sections from the Karlsruhe Astrophysical Database of Nucleosynthesis in Stars project (version v0.2, http://nuclear-astrophysics.fzk.de/kadonis). The simulations were carried out with a parametrized supernova type II shock front model ('gamma-process') of a 25 solar mass star and compared to recently published results. A decrease in the normalized overproduction factor could be attributed to lower cross sections of a significant fraction of seed nuclei located in Bi and Pb regions around the N = 126 shell closure.en
dc.format.extent5
dc.language.isoeng
dc.relation.ispartofJournal of Physics G: Nuclear and Particle Physics
dc.rightsOpen
dc.subjectNUCLEAR
dc.subjectISOTOPES
dc.subjectSTARS
dc.subjectSTATISTICAL-MODEL CALCULATIONS
dc.subjectPROCESS NUCLEOSYNTHESIS
dc.subjectCROSS-SECTIONS
dc.subjectELEMENTS
dc.subjectASTROPHYSICAL REACTION-RATES
dc.subjectRP-PROCESS
dc.subjectNEUTRON-CAPTURE
dc.titlep-Process simulations with a modified reaction libraryen
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.versiontypeFinal Accepted Version
dcterms.dateAccepted2008-01
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1088/0954-3899/35/1/014029
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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