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.
arXiv comment4 pages, no figure, 3nd revsion with one reference added
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- A new metric for rotating black holes in Gauss-Bonnet gravity
- A new metric for rotating charged Gauss-Bonnet black holes in AdS spaces
- Black Hole Entropy: From Shannon to Bekenstein