Hot Neutron Stars at Birth and Related Problems

Details Hot Neutron Stars at Birth and Related Problems Hot Neutron Stars at Birth and Related Problems

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996pthph..95..901t&link_type=abstract

Progress of Theoretical Physics, Vol. 95, No. 5, pp. 901-912

Physics

9

Scientific paper

On the basis of a realistic supernova equation of state which has been obtained by solving a set of finite-temperature Hartree-Fock equations with effective nucleon interaction, hot neutron stars at birth are constructed. They are compared with the usual cold neutron stars with regard to composition, equation of state and profile, and are discussed concerning the energy release and the spin-up in the subsequent cooling stage. Also, it is stressed that new constraints are imposed on the critical mass and the maximum rotation rate of cold neutron stars by consideration of their hot stage. A comment is given concerning the effect of pion condensation on this critical mass problem.

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