Quantized black holes, correspondence principle, and holographic bound

I. B. Khriplovich

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arXiv · gr-qc/0409031

Quantized black holes, correspondence principle, and holographic bound

I. B. Khriplovich

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Abstract

An equidistant spectrum of the horizon area of a quantized black hole does not follow from the correspondence principle or from general statistical arguments. Such a spectrum obtained earlier in loop quantum gravity (LQG) does not comply with the holographic bound. This bound fixes the Barbero-Immirzi parameter of LQG, and thus leads to the unique result for the spectrum of horizon area.

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I. B. Khriplovich. 2004-10-03. Quantized black holes, correspondence principle, and holographic bound. https://arxiv.org/abs/gr-qc/0409031

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