Entropy and thermodynamical stability of white dwarfs

Fuente: arXiv
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Autori principali: Adam, Jr., Jiří, Truhlík, Emil
Natura: Preprint
Pubblicazione: 2024
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author Adam, Jr., Jiří
Truhlík, Emil
author_facet Adam, Jr., Jiří
Truhlík, Emil
contents A structure of spherical white dwarfs is calculated for a non-zero temperature. It is shown that the thermodynamical stability of the white dwarf stars can be described naturally within the concept of the Helmholtz free energy of the Coulomb fully ionized electron-ion plasma.
format Preprint
id arxiv_https___arxiv_org_abs_2406_07010
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Entropy and thermodynamical stability of white dwarfs
Adam, Jr., Jiří
Truhlík, Emil
Solar and Stellar Astrophysics
A structure of spherical white dwarfs is calculated for a non-zero temperature. It is shown that the thermodynamical stability of the white dwarf stars can be described naturally within the concept of the Helmholtz free energy of the Coulomb fully ionized electron-ion plasma.
title Entropy and thermodynamical stability of white dwarfs
topic Solar and Stellar Astrophysics
url https://arxiv.org/abs/2406.07010