Reflection from black holes and space-time topology
arXiv:gr-qc/0310134 · doi:10.1209/epl/i2003-10113-4
Abstract
The quantum corrections make the black hole capable of reflection: any particle that approaches the event horizon can bounce back in the outside world. The albedo of the black hole depends on its temperature. The reflection shares physical origins with the phenomenon of Hawking radiation; both effects are explained as consequences of the singular nature that the event horizon exhibits on the quantum level.
4 pages, revtex
References in corpus (7)
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Cited by in corpus (8)
- Scattering of scalar particles by a black hole
- Reflection, radiation and interference for black holes
- Dense spectrum of resonances and particle capture in a near-black-hole metric
- Reflection and Transmission at the Apparent Horizon during Gravitational Collapse
- Electromagnetic Albedo of Quantum Black Holes
- Particle absorption by black holes and the generalized second law of thermodynamics
- Krein's Formula And Heat-Kernel Expansion For Some Differential Operators With A Regular Singularity
- Absorption probabilities associated with spin-3/2 particles near -dimensional Schwarzschild black holes