The hot neutron star
classification
⚛️ nucl-th
keywords
neutronstarequationparameterstemperaturecalculatedfiniteglobal
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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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