Self-consistent approximate solutions of the semiclassical Einstein equations for a Schwarzschild black hole with its Hawking evaporation

Details Self-consistent approximate solutions of the semiclassical Einstein equations for a Schwarzschild black hole with its Hawking evaporation Self-consistent approximate solutions of the semiclassical Einstein equations for a Schwarzschild black hole with its Hawking evaporation

Jul 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000phrvd..62b4029h&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 62, Issue 2, 15 July 2000, id.024029

Physics

1

Quantum Aspects Of Black Holes, Evaporation, Thermodynamics

Scientific paper

In the present paper, the self-consistent approximate formally analytic solutions of the semiclassical Einstein equations for the equilibrium of a Schwarzschild black hole with its Hawking evaporation are obtained. In the calculation, the approximation is used that the equilibrium system is supposed to consist of a black hole, thermal radiation, and a two-dimensional surface layer. The solution is compared with several related solutions, including York's back-reaction solution.

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