Quantum tunneling and black hole spectroscopy
arXiv:0907.4271 · doi:10.1016/j.physletb.2010.02.067
Abstract
The entropy-area spectrum of a black hole has been a long-standing and unsolved problem. Based on a recent methodology introduced by two of the authors, for the black hole radiation (Hawking effect) as tunneling effect, we obtain the entropy spectrum of a black hole. In Einstein's gravity, we show that both entropy and area spectrum are evenly spaced. But in more general theories (like Einstein-Gauss-Bonnet gravity), although the entropy spectrum is equispaced, the corresponding area spectrum is not.
10 pages, LaTeX, no figures; v2: 9 pages, now, title changed, minor changes to match published version in Phys. Lett. B
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