Novel Geometrical Models of Relativistic Stars III. The Point Particle Idealization

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dc.creatorFiziev, P. P.
dc.date2004-09-27
dc.date.accessioned2026-07-07T02:14:44Z
dc.date.available2026-07-07T02:14:44Z
dc.descriptionWe describe a novel class of geometrical models of relativistic stars. Our approach to the static spherically symmetric solutions of Einstein equations is based on a careful physical analysis of radial gauge conditions. It brings us to a two parameter family of relativistic stars without stiff functional dependence between the stelar radius and stelar mass. As a result, a point particle idealization -- a limiting case of bodies with finite dimension, becomes possible in GR, much like in Newtonian gravity. We devote this article to detailed mathematical study of this limit.
dc.description7 pages, latex file, no figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0409610
dc.identifierhttp://arxiv.org/abs/astro-ph/0409610
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8234
dc.subjectAstrophysics
dc.titleNovel Geometrical Models of Relativistic Stars III. The Point Particle Idealization
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