Spherically Symmetric Static Solution for a Schwarzschild Black Hole with Its Hawking Radiation

Details Spherically Symmetric Static Solution for a Schwarzschild Black Hole with Its Hawking Radiation Spherically Symmetric Static Solution for a Schwarzschild Black Hole with Its Hawking Radiation

May 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000chphl..17..329h&link_type=abstract

Chinese Physics Letters, Volume 17, Issue 5, pp. 329-331 (2000).

Physics

4

Scientific paper

A black hole and its Hawking radiation may be in stable thermal equilibrium. In this letter, the static spherically symmetric numerical solution for a Schwarzschild black hole with its Hawking radiation are obtained. In the calculation, the equilibrium system is supposed to consist of a black hole, thermal radiation and a two-dimensional surface layer. The solutions obtained are compared with the York's back-reaction approach and the Zhao-Liu thermodynamic approach.

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