dc.contributor.author | Rauscher, T. | |
dc.date.accessioned | 2013-07-02T11:02:03Z | |
dc.date.available | 2013-07-02T11:02:03Z | |
dc.date.issued | 2003-08 | |
dc.identifier.citation | Rauscher , T 2003 , ' Nuclear partition functions at temperatures exceeding 10(10) K ' , Astrophysical Journal, Supplement Series , vol. 147 , no. 2 , pp. 403-408 . | |
dc.identifier.issn | 0067-0049 | |
dc.identifier.uri | http://hdl.handle.net/2299/11009 | |
dc.description.abstract | Nuclear 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.extent | 6 | |
dc.format.extent | 124968 | |
dc.language.iso | eng | |
dc.relation.ispartof | Astrophysical Journal, Supplement Series | |
dc.subject | STATISTICAL-MODEL CALCULATIONS | |
dc.subject | ASTROPHYSICAL REACTION-RATES | |
dc.subject | nuclear reactions, nucleosynthesis, abundances | |
dc.title | Nuclear partition functions at temperatures exceeding 10(10) K | en |
dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
dc.description.status | Peer reviewed | |
rioxxterms.type | Journal Article/Review | |
herts.preservation.rarelyaccessed | true | |