Astrophysics and Space Science

, Volume 306, Issue 4, pp 273–277 | Cite as

Relativistic Model for Radiating Star

  • B. C. Tewari
Original Article

Abstract

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.

Keywords

General relativity High energy astrophysics 

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Copyright information

© Springer Science+Business Media B.V. 2006

Authors and Affiliations

  • B. C. Tewari
    • 1
  1. 1.Department of MathematicsKumaun UniversityAlmoraIndia

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