Hawking Radiation from a Vaidya Black Hole: A Semi-Classical Approach and Beyond
arXiv:0811.1132
Abstract
We derive the Hawking radiation for Vaidya black hole in the tunneling picture from the corresponding single particle action by the use of the radial null geodesic and the Hamilton-Jacobi method (beyond semi-classical approximation). Both results are then analyzed and compared.
arXiv commentCorrected version of presented talk at 2nd ICMNS (October 28, 2008), Bandung, Indonesia. 13 pages, jhep style, v4: some minor corrections, references added
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- Hawking Radiation due to Photon and Gravitino Tunneling
- Hawking Radiation from Kerr-Newman Black Hole and Tunneling Mechanism
- Corrected Entropy of Friedmann-Robertson-Walker Universe in Tunneling Method
- Corrections to Unruh effect in tunneling formalism and mapping with Hawking effect
- Thermodynamics of Black Holes: Semi-Classical Approaches and Beyond