The hot neutron star

Physics – Nuclear Physics – Nuclear Theory

Scientific paper

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Details

15 pages, LaTeX2e, 3 eps figures, to appear in Physica Scripta

Scientific paper

10.1238/Physica.Regular.061a0054

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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