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dc.contributor.authorRauscher, T.
dc.contributor.authorKratz, K.L.
dc.contributor.authorOberhummer, H.
dc.contributor.authorDobaczewski, J.
dc.contributor.authorMoller, P.
dc.contributor.authorSharma, M.
dc.date.accessioned2013-07-02T13:47:04Z
dc.date.available2013-07-02T13:47:04Z
dc.date.issued1997-08-04
dc.identifier.citationRauscher , T , Kratz , K L , Oberhummer , H , Dobaczewski , J , Moller , P & Sharma , M 1997 , ' Uncertainties in direct neutron capture calculations due to nuclear structure models ' , Nuclear Physics A , vol. 621 , no. 1-2 , pp. C327-C330 .
dc.identifier.issn0375-9474
dc.identifier.urihttp://hdl.handle.net/2299/11034
dc.description.abstractThe prediction of cross sections for nuclei far off stability is crucial in the field of nuclear astrophysics. For spherical nuclei close to the dripline the statistical model (Hauser-Feshbach) approach is not applicable and direct contributions may dominate the cross sections. For neutron-rich, even-even Sn targets, we compare the resulting neutron capture cross sections when consistently taking the input for the direct capture calculations from three different microscopic models. The results underline the sensitivity of cross sections calculated in the direct model to nuclear structure models which can lead to high uncertainties when lacking experimental informationen
dc.format.extent4
dc.format.extent65118
dc.language.isoeng
dc.relation.ispartofNuclear Physics A
dc.subjectPARTICLE
dc.titleUncertainties in direct neutron capture calculations due to nuclear structure modelsen
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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