From nuclear matter to Neutron Stars

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dc.creatorJha, T. K.
dc.date2009-02-02
dc.date.accessioned2026-07-07T12:36:58Z
dc.date.available2026-07-07T12:36:58Z
dc.descriptionNeutron stars are the most dense objects in the observable Universe and conventionally one uses nuclear theory to obtain the equation of state (EOS) of dense hadronic matter and the global properties of these stars. In this work, we review various aspects of nuclear matter within an effective Chiral model and interlink fundamental quantities both from nuclear saturation as well as vacuum properties and correlate it with the star properties.
dc.description10 Figures, 1 Table
dc.identifierhttps://arxiv.org/abs/0902.0262
dc.identifierhttp://arxiv.org/abs/0902.0262
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/218279
dc.subjectNuclear Theory
dc.titleFrom nuclear matter to Neutron Stars
dc.typetext

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