Relativistic Model for Radiating Star
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New Solution of Einstein’s equations for spherically symmetric radiating fluid distribution has been presented. The solution is used to construct a model of radiating star. The interior space-time metric is matched with Vaidya exterior metric at zero pressure boundary.
KeywordsGeneral relativity High energy astrophysics
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- Tewari, B.C.: Indian J. Pure Appl. Phys. 32, 504 (1994)Google Scholar