Hawking temperature from quasi-normal modes

Details Hawking temperature from quasi-normal modes Hawking temperature from quasi-normal modes

2004-06-24

arxiv.org/abs/gr-qc/0406097v1

Class.Quant.Grav. 21 (2004) L123

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

7 pages

Scientific paper

10.1088/0264-9381/21/17/L02

A perturbed black hole has characteristic frequencies (quasi-normal modes). Here I apply a quantum measurement analysis of the quasi-normal mode frequency in the limit of high damping. It turns out that a measurement of this mode necessarily adds noise to it. For a Schwarzschild black hole, this corresponds exactly to the Hawking temperature. The situation for other black holes is briefly discussed.

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