Particle emission from a black hole on a tense codimension-2 brane
arXiv:0902.2194 · doi:10.1103/PhysRevD.79.084041
Abstract
We calculate analytically grey-body factors of Schwarzschild black-holes localized on a 3-brane of finite tension and codimension 2. We obtain explicit expressions for various types of particles emitted in the bulk as well as on the brane in both the low and high frequency regimes. In the latter case, we obtain expressions which are valid for arbitrary number of extra dimensions if the brane tension vanishes.
35 pages incl. 13 figures, added/corrected references
References in corpus (13)
- BlackMax: A black-hole event generator with rotation, recoil, split branes and brane tension
- Catfish: A Monte Carlo simulator for black holes at the LHC
- WKB analysis of the Regge-Wheeler equation down in the frequency plane
- Split fermion quasi-normal modes
- Evaporation of a black hole off of a tense brane
- Wave dynamics of a six-dimensional black hole localized on a tensional three-brane
- Greybody Factors for Rotating Black Holes on Codimension-2 Branes
- Bulk dominated fermion emission on a Schwarzschild background
- Bulk scalar emission from a rotating black hole pierced by a tense brane
- Fermion excitations of a tense brane black hole
- Rotating Black Holes on Codimension-2 Branes
- Quasi-normal modes of a black hole localized on a codimension-two brane of finite tension
- Bulk versus Brane Emissivities of Photon Fields: For the case of Higher-Dimensional Schwarzschild Phase