Hawking Radiation as Tunnelling in Static Black Holes
General Relativity and Quantum Cosmology
2007-05-23 v1
Abstract
Hawking radiation can usefully be viewed as a semi-classical tunnelling process that originates at the black hole horizon. The conservation of energy implies the effect of self-gravitation. For a static black hole, a generalized Painleve coordinate system is introduced, and Hawking radiation as tunnelling under the effect of self-gravitation is investigated. The corrected radiation is consistent with the underlying unitary theory.
Cite
@article{arxiv.gr-qc/0512098,
title = {Hawking Radiation as Tunnelling in Static Black Holes},
author = {Wenbiao Liu},
journal= {arXiv preprint arXiv:gr-qc/0512098},
year = {2007}
}