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Hawking temperature from quasi-normal modes | | Claus Kiefer
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24 Jun 2004 | | Journal: | Class.Quant.Grav. 21 (2004) L123 | | Subject: | gr-qc | | Abstract: | 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. | | Source: | arXiv, gr-qc/0406097 | | Services: | Forum | Review | PDF | Favorites | |
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