Properties of rapidly rotating hot neutron stars within Brueckner theory
Hong-Ming Liu, Bo-Xiu Zhou, Zeng-Hua Li, Jin-Biao Wei, H. -J. Schulze
Abstract
We study the properties of hot rapidly rotating neutron stars using various equations of state based on the Brueckner-Hartree-Fock approach at finite temperature. The temperature dependence of gravitational mass, equatorial radius, Kepler frequency, moment of inertia are analysed in detail and universal relations are examined.
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