Nuclear Partition Functions at Temperatures Exceeding 10 10 K | Zendy

T. Rauscher | Zendy

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Nuclear Partition Functions at Temperatures Exceeding 10 ¹⁰ K

Author(s) -

T. Rauscher

Publication year - 2003

Publication title -

the astrophysical journal supplement series

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 3.546

H-Index - 277

eISSN - 1538-4365

pISSN - 0067-0049

DOI - 10.1086/375733

Subject(s) - nuclide , nuclear physics , partition (number theory) , neutron , physics , proton , fermi gamma ray space telescope , atomic physics , mathematics , condensed matter physics , combinatorics

Nuclear partition functions were calculated for a grid of temperatures from1.2x10^10 K to 2.75x10^11 K (1<=kT<=24 MeV) within a Fermi-gas approach,including all nuclides from the proton-dripline to the neutron-dripline withproton number 9<=Z<=85. The calculation is based on a nuclear level densitydescription published elsewhere, thus extending the previous tables ofpartition functions beyond 10^10 K. Additional high temperature corrections hadto be applied.

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