Physics
Scientific paper
Sep 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pthph..82..475t&link_type=abstract
Progress of Theoretical Physics, Vol. 82, No. 3, pp. 475-480
Physics
14
Scientific paper
Based on the equation of state for supernova matter suitably constructed, the characteristicfeatures of hot neutron stars at the birth era, such as a "fat density profile", are demonstrated. Also,energies releasable in the formation and the cooling stages are estimated for the case with andwithout pion condensations and are discussed in connection with SN1987A.
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