On Reflectivity of Quantum Black Hole Horizons - INSPIRE

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On Reflectivity of Quantum Black Hole Horizons

Naritaka Oshita
(
- Perimeter Inst. Theor. Phys. and
- Tokyo U., RESCEU and
- Tokyo U.
)
,
Qingwen Wang
(
- Perimeter Inst. Theor. Phys. and
- Waterloo U.
)
,
Niayesh Afshordi
(
- Perimeter Inst. Theor. Phys. and
- Waterloo U.
)

May 1, 2019

15 pages

Published in:

JCAP 04 (2020) 016

Published: Apr 14, 2020

e-Print:

1905.00464 [hep-th]

DOI:

10.1088/1475-7516/2020/04/016 (publication)

View in:

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Abstract: (IOP)

We study the reflectivity of quantum black hole (BH) horizons using detailed balance and fluctuation-dissipation theorem, finding a universal flux reflectivity given by the Boltzmann factor &calR; = &exp;(−(ℏ |&tildeomega;|)/(k TH)), where ˜ω is frequency in the horizon frame and TH is the Hawking temperature. This implies CP-symmetry (or &BbbR;&BbbP;3 topology) of the extended BH spacetime. We then briefly discuss related physical implications: we predict echoes in the ringdown of Kerr BHs, but they do not exhibit ergoregion instability. The viscosity in the membrane paradigm is modified to η = (c3)/(16πG) tanh((ℏ |&tildeomega;| )/(4 k TH)), only approaching General Relativistic value at high frequencies.

Note:

15 pages, 5 figures, appendixes added

black hole: quantum
black hole: horizon
temperature: Hawking
frequency: high
space-time
viscosity
stability
membrane
topology
Kerr

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