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.
Corrected version of presented talk at 2nd ICMNS (October 28, 2008), Bandung, Indonesia. 13 pages, jhep style, v4: some minor corrections, references added
References in corpus (10)
- Tunnelling, Temperature and Taub-NUT Black Holes
- Quantum Tunneling and Back Reaction
- Noncommutative Black Hole Thermodynamics
- Subtleties in the quasi-classical calculation of Hawking radiation
- Fermion Tunneling Beyond Semiclassical Approximation
- Quantum Tunneling and Trace Anomaly
- Thermal radiation of various gravitational backgrounds
- Corrected entropy of BTZ black hole in tunneling approach
- Black Hole Thermodynamics and the Factor of 2 Problem
- Local Hawking temperature for dynamical black holes
Cited by in corpus (4)
- Exact Differential and Corrected Area Law for Stationary Black Holes in Tunneling Method
- 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