Quantum spectrum of black holes

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The black hole as the thermodynamical system in equilibrium possesses the periodicity of motion in imaginary time, that allows us to formulate the quasi-classical rule of quantization. The rule yields the equidistant spectrum for the entropy of non-rotating black holes as well as for the appropriately scaled entropy in the case of rotation. We clarify and discuss a role of quasi-normal modes.
5 pages, RevTeX4 class; v2, v3: references added

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General Relativity and Quantum Cosmology, High Energy Physics - Theory

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http://salesiana.dossiersoluciones.com/handle/123456789/95315

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/gr-qc/0509038
 http://arxiv.org/abs/gr-qc/0509038

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arXiv