Reflection, radiation and interference for black holes
arXiv:gr-qc/0310051 · doi:10.1103/PhysRevD.69.124031
Abstract
Black holes are capable of reflection: there is a finite probability for any particle that approaches the event horizon to bounce back. The albedo of the black hole depends on its temperature and the energy of the incoming particle. The reflection shares its physical origins with the Hawking process of radiation, both of them arise as consequences of the mixing of the incoming and outgoing waves that takes place on the event horizon.
10 pages, 1 figure, Revtex
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- Particle absorption by black holes and the generalized second law of thermodynamics
- Scattering of Scalar Field by an Extended Black Hole in F(R) gravity
- Spectral Functions of Singular Operators
- Krein's Formula And Heat-Kernel Expansion For Some Differential Operators With A Regular Singularity
- Absorption cross section of RN and SdS extremal black hole