The hot neutron star
arXiv:nucl-th/9912039 · doi:10.1238/Physica.Regular.061a00544
Abstract
In this paper the equation of state of hot neutron matter is calculated. Involving the Oppenheimer-Volkov-Tolman equation global parameters of a neutron star at the finite temperature are obtained. The objective of our work was to study the influence of the temperature on the main parameters of a neutron star.
15 pages, LaTeX2e, 3 eps figures, to appear in Physica Scripta