Anomaly Analysis of Hawking Radiation from Acoustic Black Hole
arXiv:0706.3563 · doi:10.1088/1126-6708/2007/07/070
Abstract
The Hawking radiation from the three dimensional rotating acoustic black hole is considered from the viewpoint of anomaly cancellation method initiated by Robinson and Wilczek. Quantum field near the horizon is effectively described by two dimensional charged field with a charge identified as the angular momentum m. The fluxes of charge and energy are obtained from the anomaly cancellation condition and regularity at the horizon, and are shown to match with those of the two dimensional black body radiation at the Hawking temperature.
arXiv comment11 pages; added reference, version to appear in JHEP
References in corpus (22)
- Acoustic black holes: horizons, ergospheres, and Hawking radiation
- Relationship between Hawking Radiation and Gravitational Anomalies
- Nonextremal Black Hole Microstates and U-duality
- Anomalies, Hawking Radiations and Regularity in Rotating Black Holes
- Hawking Radiation from Charged Black Holes via Gauge and Gravitational Anomalies
- Quasinormal modes and classical wave propagation in analogue black holes
- Hawking Radiation from Rotating Black Holes and Gravitational Anomalies
- Hawking radiation from dilatonic black holes via anomalies
- Hawking radiation from rotating black holes in anti-de Sitter spaces via gauge and gravitational anomalies
- `Superresonance' from a rotating acoustic black hole
- Hawking Radiation from General Kerr-(anti)de Sitter Black Holes
- Gauge and Gravitational Anomalies and Hawking Radiation of Rotating BTZ Black Holes
- Two-dimensional gravitational anomalies, Schwinger terms and dispersion relations
- Quantum Anomalies at Horizon and Hawking Radiations in Myers-Perry Black Holes
- Hawking radiation from (2+1)-dimensional BTZ black holes
- Gravitational Anomalies, Hawking Radiation, and Spherically Symmetric Black Holes
- Quasinormal modes, Superradiance and Area Spectrum for 2+1 Acoustic Black Holes
- Anomalies of the Achucarro-Ortiz black hole
- Anomalies and de Sitter radiation from the generic black holes in de Sitter spaces
- Higher-spin Currents and Thermal Flux from Hawking Radiation
- Hawking Radiation from Non-Extremal D1-D5 Black Hole via Anomalies
- Decay Rate and Low-Energy Near-Horizon Dynamics of Acoustic Black Holes
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