Exact Hawking Radiation of Scalars, Fermions, and Bosons Using the Tunneling Method Without Back-Reaction
arXiv:1012.3165 · doi:10.1016/j.physletb.2011.02.023
Abstract
Hawking radiation is studied for arbitrary scalars, fermions, and spin-1 bosons, using a tunneling approach, to every order in but ignoring back-reaction effects. It is shown that the additional quantum terms yield no new contribution to the Hawking temperature. Indeed, it is found that the limit of small in the standard quantum WKB approximation is replaced by the near-horizon limit in the gravitational WKB approach.
8 pages, no figures. v3: Introduction updated. Version to appear in PLB
References in corpus (21)
- Fermions Tunnelling from Black Holes
- Tunnelling, Temperature and Taub-NUT Black Holes
- Charged Fermions Tunnelling from Kerr-Newman Black Holes
- Temporal contribution to gravitational WKB-like calculations
- Dirac particles tunneling from BTZ black hole
- Subtleties in the quasi-classical calculation of Hawking radiation
- Fermion Tunneling Beyond Semiclassical Approximation
- Thermal radiation of various gravitational backgrounds
- Corrected entropy of BTZ black hole in tunneling approach
- Hawking radiation of Dirac particles via tunneling from Kerr black hole
- On the Hawking radiation as tunneling for a class of dynamical black holes
- Tunnelling From Gödel Black Holes
- Remarks on Hawking radiation as tunneling from the BTZ black holes
- Problems with Tunneling of Thin Shells from Black Holes
- Black Hole Thermodynamics and the Factor of 2 Problem
- Tunnelling Effect and Hawking Radiation from a Vaidya Black Hole
- Tunnelling through black rings
- Insights and possible resolution to the information loss paradox via the tunneling picture
- Tunneling Effect Near Weakly Isolated Horizon
- Band-aid for information loss from black holes
- Observer Dependent Horizon Temperatures: a Coordinate-Free Formulation of Hawking Radiation as Tunneling