Physics – Nuclear Physics – Nuclear Theory
Scientific paper
1998-02-18
Physics
Nuclear Physics
Nuclear Theory
8 pages, Latex, 3 figures included. To appear in "Hirschegg '98: Nuclear Astrophysics", Proceedings of Int. Workshop XXVI on G
Scientific paper
We study the properties of static and rotating neutron stars adopting non-relativistic equations of state (EOS) for asymmetric nuclear matter based on the Brueckner-Hartree-Fock (BHF) scheme. The BHF calculation, with the continuous choice for the single particle potential, appears to be very close to the full EOS, which includes the three-hole line contribution calculated by solving the Bethe-Fadeev equations within the gap choice for the single particle potential. Three-body forces are included in order to reproduce the correct saturation point for nuclear matter. A comparison with fully relativistic many-body calculations of nuclear matter EOS is made.
Baldo Marcello
Burgio G. F.
Song Hong-Qiang
Weber Fridolin
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