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NON-SPHERICAL COLLAPSE OF A RADIATING STAR

S. G. GHOSH

Centre for Mathematical Physics, Science College, Congress Nagar, Nagpur-440 012, India

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and

D. W. DESHKAR

Centre for Mathematical Physics, Science College, Congress Nagar, Nagpur-440 012, India

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https://doi.org/10.1142/S0218271803002433Cited by:24 (Source: Crossref)

Abstract

We study the junction conditions for non-spherical (plane symmetric) collapsing radiating star consisting of a shearing fluid undergoing radial heat flow with outgoing radiation. Radiation of the system is described by plane symmetric Vaidya solution. Physical quantities relating to the local conservation of momentum and surface red-shift are also obtained.

PACS: 04.20.-q, 04.40.Dg, 97.10.Cv

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