Spherical gravitational collapse and electromagnetic fields in radially homothetic spacetimes

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dc.creatorWagh, Sanjay M
dc.date2002-10-01
dc.date.accessioned2026-07-07T02:05:31Z
dc.date.available2026-07-07T02:05:31Z
dc.descriptionWe consider a spherically symmetric, Petrov-type D, spacetime with hyper-surface orthogonal, radial, homothetic Killing vector. In this work, some general properties of this spacetime for non-singular and non-degenerate data are presented. We also present the source-free electromagnetic fields in this spacetime. We then discuss general astrophysical relevance of the results obtained for this spacetime.
dc.descriptionRevtex4, No figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0210020
dc.identifierhttp://arxiv.org/abs/astro-ph/0210020
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5125
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleSpherical gravitational collapse and electromagnetic fields in radially homothetic spacetimes
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