Supernova and neutron stars with relativistic equations of state

Details Supernova and neutron stars with relativistic equations of state Supernova and neutron stars with relativistic equations of state

Feb 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992phlb..276..393s&link_type=abstract

Physics Letters B, Volume 276, Issue 4, p. 393-397.

Physics

18

Scientific paper

We study the properties of supernova hot stars and neutron stars using equations of state at finite temperature with arbitrary proton-to-neutron ratios derived from the relativistic mean field theory. The coupling strengths and masses of the relativistic mean field theory are fixed by the known nuclear properties and describe also unstable nuclei. We calculate also the star profiles with equations of state obtained by the relativistic Brueckner-Hartree-Fock theory, which reproduces the nuclear matter saturation property.
On leave of absence from University of Mainz, W-6500 Mainz, FRG.

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