Stress-energy tensor of a radiating sphere inclosing black hole

Abstract

We consider a uniformly luminous radiating sphere and a static black hole located in the center of that sphere. We give analytic formulas for radiation stress-energy tensor components in such a configuration, for the observer located at an arbitrary distance from the static black hole horizon.

To appear in the Proceedings of RAGtime

References in corpus (1)

• Cosmic background radiation in the vicinity of a Schwarzschild black hole: no classic firewall

Cited by in corpus (1)

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