dc.creatorGratton, Livio
dc.date1960
dc.date2019-04-24T12:50:45Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/74443
dc.descriptionIn 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.
dc.descriptionAsociación Argentina de Astronomía
dc.formatapplication/pdf
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectCiencias Astronómicas
dc.subjectdegenerated stellar configurations
dc.subjectGalaxias
dc.titleA comment on the equation of state for a degenerated gas
dc.typeArticulo
dc.typeArticulo


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