Black hole horizon fluctuations

A. Casher; F. Englert; N. Itzhaki; S. Massar; R. Parentani

doi:10.1016/S0550-3213(96)00613-X

Black hole horizon fluctuations

A. Casher^*, F. Englert, N. Itzhaki, S. Massar, R. Parentani

^*Corresponding author for this work

School of Physics and Astronomy

Research output: Contribution to journal › Article › peer-review

Abstract

Some authors have suggested 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 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.

Original language	English
Pages (from-to)	419-434
Number of pages	16
Journal	Nuclear Physics B
Volume	484
Issue number	1-2
DOIs	https://doi.org/10.1016/S0550-3213(96)00613-X
State	Published - 20 Jan 1997

Keywords

Black hole
Hawking radiation

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10.1016/S0550-3213(96)00613-X

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AU - Casher, A.

AU - Englert, F.

AU - Itzhaki, N.

AU - Massar, S.

AU - Parentani, R.

PY - 1997/1/20

Y1 - 1997/1/20

N2 - Some authors have suggested 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 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.

AB - Some authors have suggested 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 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.

KW - Black hole

KW - Hawking radiation

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Black hole horizon fluctuations

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Keywords

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