Gravitational Anomaly and Hawking Radiation of Brane World Black Holes
arXiv:0710.4766 · doi:10.1142/S0217732308026364
Abstract
We apply Wilczek and his collaborators' anomaly cancellation approach to the 3-dimensional Schwarzschild- and BTZ-like brane world black holes induced by the generalized C metrics in the Randall-Sundrum scenario. Based on the fact that the horizon of brane world black hole will extend into the bulk spacetime, we do the calculation from the bulk generalized C metrics side and show that this approach also reproduces the correct Hawking radiation for these brane world black holes. Besides, since this approach does not involve the dynamical equation, it also shows that the Hawking radiation is only a kinematic effect.
11 pages. v2: minor changes and references added
References in corpus (5)
- Hawking radiation from rotating black holes in anti-de Sitter spaces via gauge and gravitational anomalies
- Hawking Radiation and Covariant Anomalies
- Hawking Radiation from General Kerr-(anti)de Sitter Black Holes
- Gravitational anomalies: a recipe for Hawking radiation
- Hawking radiation of a vector field and gravitational anomalies
Cited by in corpus (8)
- Covariant anomalies and Hawking radiation from charged rotating black strings in anti-de Sitter spacetimes
- Hawking radiation, W-infinity algebra and trace anomalies
- Anomalies, effective action and Hawking temperatures of a Schwarzschild black hole in the isotropic coordinates
- Hawking radiation from covariant anomalies in 2+1 dimensional black holes
- Hawking radiation via anomaly cancelation for the black holes of five-dimensional minimal gauged supergravity
- On Gravitational anomaly and Hawking radiation near weakly isolated horizon
- Hawking Radiation, Gravitational Anomaly and Conformal Symmetry - the Origin of Universality -
- Higher Derivative Correction to the Hawking Flux via Trace Anomaly