Angular profile of emission of non-zero spin fields from a higher-dimensional black hole
arXiv:0907.1511 · doi:10.1016/j.physletb.2009.08.062
Abstract
Recent works have included the effect of rotation on simulations of black hole events at the LHC, showing that the angular momentum of the black hole cannot be ignored and it makes a non-trivial contribution for most of the lifetime of the black hole. A key consequence of the rotation of the black hole is that the Hawking radiation is no longer isotropic, making it more difficult to infer space-time parameters from measurements of the emitted particles. In this letter we study the angular distribution of the Hawking emission of non-zero spin particles with specific helicity on the brane. We argue that the shape of the distribution could be used as a measure of the angular momentum of the black hole.
11 pages, 3 figures, minor changes, matches published version
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Cited by in corpus (11)
- Greybody Factors for Scalar Fields emitted by a Higher-Dimensional Schwarzschild-de-Sitter Black-Hole
- Hawking emission from quantum gravity black holes
- Hawking Radiation Spectra for Scalar Fields by a Higher-Dimensional Schwarzschild-de-Sitter Black Hole
- Kermions: quantization of fermions on Kerr space-time
- Effective Temperatures and Radiation Spectra for a Higher-Dimensional Schwarzschild-de-Sitter Black-Hole
- Black holes and the LHC: A review
- Hawking Radiation from Higher-Dimensional Black Holes
- Emission of Massive Scalar Fields by a Higher-Dimensional Rotating Black-Hole
- Chiral anomalies in black hole spacetimes
- Angular correlations in TeV-gravity black hole events
- Angular profile of Particle Emission from a Higher-dimensional Black Hole: Analytic Results