Junction Conditions and Consequences of Quasi-Spherical Space-Time with Electro-Magnetic Field and Vaidya Matric

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dc.creatorNath, Soma
dc.creatorDebnath, Ujjal
dc.creatorChakraborty, Subenoy
dc.date2007-11-07
dc.date.accessioned2026-07-07T11:12:59Z
dc.date.available2026-07-07T11:12:59Z
dc.descriptionIn this work the junction conditions between the exterior Reissner-Nordstrom-Vaidya space-time with the interior quasi-spherical Szekeres space-time have been studied for analyzing gravitational collapse in the presence of a magneto-hydrodynamic fluid undergoing dissipation in the form of heat flow. We have discussed about the apparent horizon and have evaluated the time difference between the formation of apparent horizon and central singularity.
dc.description8 latex pages, RevTex style, no figures
dc.identifierhttps://arxiv.org/abs/0711.1057
dc.identifierhttp://arxiv.org/abs/0711.1057
dc.identifierAstrophys.SpaceSci.313:431-436,2008
dc.identifierdoi:10.1007/s10509-007-9713-3
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/191565
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleJunction Conditions and Consequences of Quasi-Spherical Space-Time with Electro-Magnetic Field and Vaidya Matric
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