The hot neutron star
核理论
2016-09-08 v1
摘要
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.
引用
@article{arxiv.nucl-th/9912039,
title = {The hot neutron star},
author = {Ilona Bednarek and Ryszard Manka},
journal= {arXiv preprint arXiv:nucl-th/9912039},
year = {2016}
}
备注
15 pages, LaTeX2e, 3 eps figures, to appear in Physica Scripta