Physics
Scientific paper
Jan 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991srtoh..11..171t&link_type=abstract
Sci. Rep. Tôhoku Univ., Eighth Ser., Vol. 11, Nos. 2/3, p. 171 - 174
Physics
Scientific paper
The equation of state (EOS) of dense supernova matter is constructed by
the finite-temperature Hartree-Fock approach with the effective
two-nucleon interaction. On the basis of the EOS, characteristic
features of neutron stars at the birth are demonstrated.
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