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arXiv · hep-th/9606106

Black Hole Horizon Fluctuations

A. Casher·F. Englert·N. Itzhaki·S. Massar·R. Parentani
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Abstract

It is generally admitted that gravitational interactions become large at an invariant distance of order $1$ from the black hole horizon. We show that due to the ``atmosphere'' of high angular particles near the horizon strong gravitational interactions already occur at an invariant distance of the order of $\sqrt[3]{M}$. The implications of these results for the origin of black hole radiation, the meaning of black hole entropy and the information puzzle are discussed.

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A. Casher, F. Englert, N. Itzhaki, S. Massar, R. Parentani. 1996-07-20. Black Hole Horizon Fluctuations. https://doi.org/10.1016/s0550-3213(96)00613-x

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