期刊
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
卷 147, 期 2, 页码 403-408出版社
UNIV CHICAGO PRESS
DOI: 10.1086/375733
关键词
nuclear reactions, nucleosynthesis, abundances
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.
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