Black Hole evaporation in semi-classical approach

Details Black Hole evaporation in semi-classical approach Black Hole evaporation in semi-classical approach

2011-02-15

arxiv.org/abs/1102.3095v1

Physics

General Physics

11 pages, 1 figure

Scientific paper

As well as known, the black hole evaporation problem is famous problem. Because the S.W.Hawking found the black holes emit light at the future null infinity as a thermal radiation \cite{H}, we think that the black holes may be vanish. However, to prove this problem, we should solve field equation, i.e. forth order partial differential equations \cite{Ford}\cite{BD}. However, we can find a method to solve this equation, and we could prove that the black holes finally vanish. To solve this problem we use dynamical horizons equation in the Vaidya spacetime.

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