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.
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Tewari, B.C. Relativistic Model for Radiating Star. Astrophys Space Sci 306, 273–277 (2006). https://doi.org/10.1007/s10509-006-9273-y
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DOI: https://doi.org/10.1007/s10509-006-9273-y