Hawking radiation from the Schwarzschild black hole with a global monopole via gravitational anomaly
arXiv:0705.1225 · doi:10.1088/1674-1056/17/3/016
Abstract
Hawking flux from the Schwarzschild black hole with a global monopole is obtained by using Robinson and Wilczek's method. Adopting a dimension reduction technique, the effective quantum field in the (3+1)--dimensional global monopole background can be described by an infinite collection of the (1+1)--dimensional massless fields if neglecting the ingoing modes near the horizon, where the gravitational anomaly can be cancelled by the (1+1)--dimensional black body radiation at the Hawking temperature.
4 pages, no figure, 3nd revsion with one reference added
References in corpus (9)
- Anomalies, Hawking Radiations and Regularity in Rotating Black Holes
- Hawking Radiation from Charged Black Holes via Gauge and Gravitational Anomalies
- Hawking Radiation from Rotating Black Holes and Gravitational Anomalies
- Hawking radiation from rotating black holes in anti-de Sitter spaces via gauge and gravitational anomalies
- Hawking Radiation from General Kerr-(anti)de Sitter Black Holes
- Gauge and Gravitational Anomalies and Hawking Radiation of Rotating BTZ Black Holes
- Gravitational Anomalies, Hawking Radiation, and Spherically Symmetric Black Holes
- Hawking Radiation from Non-Extremal D1-D5 Black Hole via Anomalies
- Anomalies and Hawking radiation from the Reissner-Nordström black hole with a global monopole