Relativistic Gravitational mass in Tolman-VI type solution

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dc.creatorRay, Saibal
dc.creatorDas, Basanti
dc.date2004-09-22
dc.date2007-10-31
dc.date.accessioned2026-07-07T11:29:27Z
dc.date.available2026-07-07T11:29:27Z
dc.descriptionSome known solutions for static charged fluid spheres of Tolman-VI type in general relativity are reexamined. The gravitational mass that appears in the Pant and Sah \cite{pan79} and Tikekar \cite{tik84} solutions is shown to be of electromagnetic origin in the sense that the gravitational mass, along with all other physical quantities, depends on the electromagnetic field alone. The energy condition, singularity and stability problems of the models are discussed thoroughly.
dc.description7 pages, no figure
dc.identifierhttps://arxiv.org/abs/astro-ph/0409527
dc.identifierhttp://arxiv.org/abs/astro-ph/0409527
dc.identifierGrav.Cosmol.13:224-230,2007
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/196716
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleRelativistic Gravitational mass in Tolman-VI type solution
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