A comment on the equation of state for a degenerated gas
- Autores
- Gratton, Livio
- Año de publicación
- 1960
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- 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 - Materia
-
Ciencias Astronómicas
degenerated stellar configurations
Galaxias - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/74443
Ver los metadatos del registro completo
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A comment on the equation of state for a degenerated gasGratton, LivioCiencias Astronómicasdegenerated stellar configurationsGalaxiasIn 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 Astronomía1960info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/74443enginfo:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-22T16:53:40Zoai:sedici.unlp.edu.ar:10915/74443Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-22 16:53:40.516SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
A comment on the equation of state for a degenerated gas |
| title |
A comment on the equation of state for a degenerated gas |
| spellingShingle |
A comment on the equation of state for a degenerated gas Gratton, Livio Ciencias Astronómicas degenerated stellar configurations Galaxias |
| 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 |
A comment on the equation of state for a degenerated gas |
| dc.creator.none.fl_str_mv |
Gratton, Livio |
| author |
Gratton, Livio |
| author_facet |
Gratton, Livio |
| author_role |
author |
| dc.subject.none.fl_str_mv |
Ciencias Astronómicas degenerated stellar configurations Galaxias |
| topic |
Ciencias Astronómicas degenerated stellar configurations Galaxias |
| dc.description.none.fl_txt_mv |
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 |
| 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. |
| publishDate |
1960 |
| dc.date.none.fl_str_mv |
1960 |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
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http://sedici.unlp.edu.ar/handle/10915/74443 |
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eng |
| language |
eng |
| dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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openAccess |
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http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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SEDICI (UNLP) - Universidad Nacional de La Plata |
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