Kiro Miyazaki
Hot neutron star in generalized thermo-statistics
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ABSTRACT.  The hot neutron star (NS) is investigated for the first time in the generalized thermo-statistics so as to take into account the breaking of the standard Boltzmann-Gibbs thermo-statistics under the long-ranged gravitational potential. It is found that at sub-saturation density in hot NS matter the gravitation leads to a stiffer equation of state than the standard thermo-statistics. The hot NSs in the generalized thermo-statistics are therefore much more massive and larger than those in the standard thermo-statistics.