Eur. Phys. J. C (2015) 75: 233
https://doi.org/10.1140/epjc/s10052-015-3465-y

Letter

Quantum-gravity fluctuations and the black-hole temperature

¹ The Ruppin Academic Center, 40250, Emeq Hefer, Israel
² The Hadassah Institute, 91010, Jerusalem, Israel

^* e-mail: shaharhod@gmail.com

Received: 3 January 2015
Accepted: 18 May 2015
Published online: 29 May 2015

Abstract

Bekenstein has put forward the idea that, in a quantum theory of gravity, a black hole should have a discrete energy spectrum with concomitant discrete line emission. The quantized black-hole radiation spectrum is expected to be very different from Hawking’s semi-classical prediction of a thermal black-hole radiation spectrum. One naturally wonders: Is it possible to reconcile the discrete quantum spectrum suggested by Bekenstein with the continuous semi-classical spectrum suggested by Hawking? In order to address this fundamental question, in this essay we shall consider the zero-point quantum-gravity fluctuations of the black-hole spacetime. In a quantum theory of gravity, these spacetime fluctuations are closely related to the characteristic gravitational resonances of the corresponding black-hole spacetime. Assuming that the energy of the black-hole radiation stems from these zero-point quantum-gravity fluctuations of the black-hole spacetime, we derive the effective temperature of the quantized black-hole radiation spectrum. Remarkably, it is shown that this characteristic temperature of the discrete (quantized) black-hole radiation agrees with the well-known Hawking temperature of the continuous (semi-classical) black-hole spectrum.