Taking the temperature of a black hole
| Autor: | Larus Thorlacius, E. J. Brynjolfsson |
|---|---|
| Rok vydání: | 2008 |
| Předmět: |
High Energy Physics - Theory
Physics Nuclear and High Energy Physics Spacetime Event horizon Astrophysics::High Energy Astrophysical Phenomena FOS: Physical sciences General Relativity and Quantum Cosmology (gr-qc) General Relativity and Quantum Cosmology AdS black hole Black hole Theoretical physics Hawking High Energy Physics - Theory (hep-th) Thermal radiation Minkowski space Asymptotically flat spacetime |
| Zdroj: | Journal of High Energy Physics. 2008:066-066 |
| ISSN: | 1029-8479 |
| DOI: | 10.1088/1126-6708/2008/09/066 |
| Popis: | We use the global embedding of a black hole spacetime into a higher dimensional flat spacetime to define a local temperature for observers in free fall outside a static black hole. The local free-fall temperature remains finite at the event horizon and in asymptotically flat spacetime it approaches the Hawking temperature at spatial infinity. Freely falling observers outside an AdS black hole do not see any high-temperature thermal radiation even if the Hawking temperature of such black holes can be arbitrarily high. latex, 14 pages, 4 figures, v3: added references, matches published version |
| Databáze: | OpenAIRE |
| Externí odkaz: |
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