Black Hole evaporation in semi-classical approach
General Physics
2011-02-16 v1
Abstract
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.
Cite
@article{arxiv.1102.3095,
title = {Black Hole evaporation in semi-classical approach},
author = {Shintaro Sawayama},
journal= {arXiv preprint arXiv:1102.3095},
year = {2011}
}
Comments
11 pages, 1 figure