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dc.contributor.authorRauscher, T.
dc.date.accessioned2013-07-02T11:02:03Z
dc.date.available2013-07-02T11:02:03Z
dc.date.issued2003-08
dc.identifier.citationRauscher , T 2003 , ' Nuclear partition functions at temperatures exceeding 10(10) K ' , Astrophysical Journal, Supplement Series , vol. 147 , no. 2 , pp. 403-408 .
dc.identifier.issn0067-0049
dc.identifier.otherPURE: 1631536
dc.identifier.otherPURE UUID: 7e730627-5faa-401c-88bf-b147f9eda346
dc.identifier.otherWOS: 000184318900008
dc.identifier.otherScopus: 0041571896
dc.identifier.urihttp://hdl.handle.net/2299/11009
dc.description.abstractNuclear partition functions were calculated for a grid of temperatures from 1.2 x 10(10) to 2.75 x 10(11) K (1 MeV less than or equal to kT less than or equal to 24 MeV) within a Fermi-gas approach, including all nuclides from the proton-dripline to the neutron-dripline with proton number 9 less than or equal to Z less than or equal to 85. The calculation is based on a nuclear level density description published elsewhere, thus extending the previous tables of partition functions beyond 10(10) K. Additional high-temperature corrections had to be applied.en
dc.format.extent6
dc.language.isoeng
dc.relation.ispartofAstrophysical Journal, Supplement Series
dc.rightsOpen
dc.subjectSTATISTICAL-MODEL CALCULATIONS
dc.subjectASTROPHYSICAL REACTION-RATES
dc.subjectnuclear reactions, nucleosynthesis, abundances
dc.titleNuclear partition functions at temperatures exceeding 10(10) Ken
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
dcterms.dateAccepted2003-08
rioxxterms.versionSMUR
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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