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arXiv · nucl-th/9912039

The hot neutron star

Ilona Bednarek·Ryszard Manka
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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.

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Ilona Bednarek, Ryszard Manka. 1999-12-15. The hot neutron star. https://doi.org/10.1238/physica.regular.061a00544

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