Hawking radiation from AdS black holes
We investigate Hawking radiation from black holes in (d+1)-dimensional anti--de Sitter space. We focus on s waves, make use of the geometrical optics approximation, and follow three approaches to analyze the radiation. First, we compute a Bogoliubov transformation between Kruskal and asymptotic coordinates and compare the different vacua. Second, following a method due to Kraus, Parikh, and Wilczek, we view Hawking radiation as a tunneling process across the horizon and compute the tunneling probability. This approach uses an anti--de Sitter version of a metric originally introduced by Painleve for Schwarzschild black holes. From the tunneling probability one also finds a leading correction to the semiclassical emission rate arising from back reaction to the background geometry. Finally, we consider a spherically symmetric collapse geometry and the Bogoliubov transformation between the initial vacuum state and the vacuum of an asymptotic observer.
- Sponsoring Organization:
- (US)
- OSTI ID:
- 40230611
- Journal Information:
- Physical Review D, Vol. 64, Issue 4; Other Information: DOI: 10.1103/PhysRevD.64.044006; Othernumber: PRVDAQ000064000004044006000001; 072114PRD; PBD: 15 Aug 2001; ISSN 0556-2821
- Publisher:
- The American Physical Society
- Country of Publication:
- United States
- Language:
- English
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