Structure of the Star with Ideal Gases

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dc.creatorGu, Ying-Qiu
dc.date2007-12-03
dc.date.accessioned2026-07-07T08:46:51Z
dc.date.available2026-07-07T08:46:51Z
dc.descriptionIn this paper, we provide a simplified stellar structure model for ideal gases, in which the particles are only driven by gravity. According to the model, the structural information of the star can be roughly solved by the total mass and radius of a star. To get more accurate results, the model should be modified by introducing other interaction among particles and rotation of the star.
dc.description9 pages, 5 figures
dc.identifierhttps://arxiv.org/abs/0712.0219
dc.identifierhttp://arxiv.org/abs/0712.0219
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/143394
dc.subjectGeneral Physics
dc.titleStructure of the Star with Ideal Gases
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