Physics
Scientific paper
Aug 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997phybl..53..671b&link_type=abstract
Physikalische Blätter, Jahrg. 53, Heft 7/8, p. 671 - 674
Physics
Supernovae: Explosions, Black Holes: Binaries, Black Holes: Neutron Stars, Masses: Neutron Stars
Scientific paper
In the collapse of large stars matter is formed at supranuclear densities. At a density ρ ≡ 3ρ0, where ρ0 is the nuclear matter density, K--mesons replace electrons, and go into Bose condensate. This soft equation of state gives a maximum mass for neutron stars of ≡1.5 Msun. It is argued that the last nearby supernova, SN 1987A, went into a black hole. A new scenario of binary star evolution is developed which results in the two masses in a given binary being nearly equal and all neutron star masses lying in a narrow band 1.3 Msun< MNS< 1.5 Msun.
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