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dc.contributor.authorMocelj, D.
dc.contributor.authorRauscher, T.
dc.contributor.authorMartinez-Pinedo, G.
dc.contributor.authorAlhassid, Y.
dc.identifier.citationMocelj , D , Rauscher , T , Martinez-Pinedo , G & Alhassid , Y 2003 , ' Influence of parity-dependence in the nuclear level density on the prediction of astrophysical reaction rates ' , Nuclear Physics A , vol. 718 , pp. 650C-652C .
dc.identifier.otherPURE: 1632419
dc.identifier.otherPURE UUID: 2e069df2-adf4-49ed-95b2-8325140dfc42
dc.identifier.otherWOS: 000182314300143
dc.identifier.otherScopus: 0037910264
dc.description.abstractA simple description for obtaining the parity distribution of nuclear levels in the pf + g(9/2) shell as a function of excitation energy was recently derived. We implement this in a global nuclear level density model. In the framework of the statistical model, cross sections and astrophysical reaction rates are calculated in the Fe region and compared to rates obtained with the common assumption of an equal distribution of parities. We find considerable differences, especially for reactions involving particles in the exit channel.en
dc.relation.ispartofNuclear Physics A
dc.titleInfluence of parity-dependence in the nuclear level density on the prediction of astrophysical reaction ratesen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.typeJournal Article/Review

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