arXiv:nucl-th/9912039·v1·Nuclear Theory
The hot neutron star
Ilona Bednarek🇵🇱 · Ryszard Manka (University of Silesia, Katowice, Poland)🇵🇱
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.
Comments: 15 pages, LaTeX2e, 3 eps figures, to appear in Physica Scripta