A comment on the equation of state for a degenerated gas

In current literature on degenerated stellar configurations there seems to exist a strange misconception concerning the equations for relativistic degeneracv. As it is well known in a non-relativistic degenerated gas we can neglect the partial pressure of heavy particles due to the fact that in the...

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Autor principal: Gratton, Livio
Formato: Articulo
Lenguaje:Inglés
Publicado: 1960
Materias:
Ciencias Astronómicas
degenerated stellar configurations
Galaxias
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/74443
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata
id I19-R120-10915-74443
record_format dspace
spelling I19-R120-10915-744432024-04-29T17:15:20Z http://sedici.unlp.edu.ar/handle/10915/74443 A comment on the equation of state for a degenerated gas Gratton, Livio 1960 2019-04-24T12:50:45Z en Ciencias Astronómicas degenerated stellar configurations Galaxias In current literature on degenerated stellar configurations there seems to exist a strange misconception concerning the equations for relativistic degeneracv. As it is well known in a non-relativistic degenerated gas we can neglect the partial pressure of heavy particles due to the fact that in the equation of state for non-relativistic degeneracy the mass of the particles is contained in the denominator: with the usual notation. Asociación Argentina de Astronomía Articulo Articulo http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application/pdf
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
degenerated stellar configurations
Galaxias
spellingShingle Ciencias Astronómicas
degenerated stellar configurations
Galaxias
Gratton, Livio
A comment on the equation of state for a degenerated gas
topic_facet Ciencias Astronómicas
degenerated stellar configurations
Galaxias
description In current literature on degenerated stellar configurations there seems to exist a strange misconception concerning the equations for relativistic degeneracv. As it is well known in a non-relativistic degenerated gas we can neglect the partial pressure of heavy particles due to the fact that in the equation of state for non-relativistic degeneracy the mass of the particles is contained in the denominator: with the usual notation.
format Articulo
Articulo
author Gratton, Livio
author_facet Gratton, Livio
author_sort Gratton, Livio
title A comment on the equation of state for a degenerated gas
title_short A comment on the equation of state for a degenerated gas
title_full A comment on the equation of state for a degenerated gas
title_fullStr A comment on the equation of state for a degenerated gas
title_full_unstemmed A comment on the equation of state for a degenerated gas
title_sort comment on the equation of state for a degenerated gas
publishDate 1960
url http://sedici.unlp.edu.ar/handle/10915/74443
work_keys_str_mv AT grattonlivio acommentontheequationofstateforadegeneratedgas
AT grattonlivio commentontheequationofstateforadegeneratedgas
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