Simple analysis of slowly rotating semidegenerate spheroids of fermions

Details Simple analysis of slowly rotating semidegenerate spheroids of fermions Simple analysis of slowly rotating semidegenerate spheroids of fermions

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995apj...439..846s&link_type=abstract

The Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 439, no. 2, p. 846-848

Statistics

Degenerate Matter, Fermions, Neutron Stars, Stellar Rotation, White Dwarf Stars, Fermi-Dirac Statistics, Moments Of Inertia, Oblate Spheroids

Scientific paper

The departure from sphericity of a slowly rotating partially degenerate self-gravitating cluster of fermions is calculated using the Clairaut theory. The required dimensionless moment of inertia has been computed using a recently proposed equation of state for semidegenerate fermion matter, based on a trapezoidal approximation to the Fermi-Dirac distribution function. This permits an analytic perturbative calculation of the cluster flattening around the zero-temperature limit, which simplifies considerably other previous approaches.

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