Hawking Radiation from a Vaidya Black Hole: A Semi-Classical Approach and Beyond
General Relativity and Quantum Cosmology
2008-11-19 v4
Abstract
We derive the Hawking radiation for Vaidya black hole in the tunneling picture from the corresponding single particle action by the use of the radial null geodesic and the Hamilton-Jacobi method (beyond semi-classical approximation). Both results are then analyzed and compared.
Keywords
Cite
@article{arxiv.0811.1132,
title = {Hawking Radiation from a Vaidya Black Hole: A Semi-Classical Approach and Beyond},
author = {Haryanto M. Siahaan and Triyanta},
journal= {arXiv preprint arXiv:0811.1132},
year = {2008}
}
Comments
Corrected version of presented talk at 2nd ICMNS (October 28, 2008), Bandung, Indonesia. 13 pages, jhep style, v4: some minor corrections, references added