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dc.contributor.authorMocelj, D.
dc.contributor.authorRauscher, T.
dc.contributor.authorThielemann, Friedrich-Karl
dc.contributor.authorMartinez-Pinedo, G.
dc.contributor.authorLanganke, K.
dc.contributor.authorPacearescu, L.
dc.contributor.authorFassler, A.
dc.identifier.citationMocelj , D , Rauscher , T , Thielemann , F-K , Martinez-Pinedo , G , Langanke , K , Pacearescu , L & Fassler , A 2005 , ' Towards a parity-dependent level density for astrophysics ' , Journal of Physics G: Nuclear and Particle Physics , vol. 31 , no. 10 , pp. S1927-S1930 .
dc.identifier.otherPURE: 1628010
dc.identifier.otherPURE UUID: bc3589f1-d1d0-49da-ab6a-e57af6e9efba
dc.identifier.otherWOS: 000232575600105
dc.identifier.otherScopus: 25444492871
dc.description.abstractAstrophysical reaction rates are sensitive to the parity distribution at low excitation energies. We combine a formula for the energy-dependent parity distribution with a microscopic-macroscopic nuclear level density. This approach describes well the transition from low excitation energies where a single parity dominates to high excitations where the two densities are equal.en
dc.relation.ispartofJournal of Physics G: Nuclear and Particle Physics
dc.titleTowards a parity-dependent level density for astrophysicsen
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.typeJournal Article/Review

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