Hawking radiation from rotating brane black holes

Abstract

We review recent work on the Hawking radiation of rotating brane black holes, as may be produced at the LHC. We outline the methodology for calculating the fluxes of particles, energy and angular momentum by spin-0, spin-1/2 and spin-1 quantum fields on the brane. We briefly review some of the key features of the emission, in particular the changes in the spectra as the number of extra dimensions or the angular velocity of the black hole increases. These quantities will be useful for accurate simulations of black hole events at the LHC.

19 pages, 13 figures, talk given at the ``Workshop on Dynamics and Thermodynamics of Black Holes and Naked Singularities II'', Milan, 10-12 May 2007

References in corpus (1)

• Greybody factors in a rotating black-hole background-II : fermions and gauge bosons

Cited by in corpus (14)

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• Hawking Radiation Spectra for Scalar Fields by a Higher-Dimensional Schwarzschild-de-Sitter Black Hole
• Scalar Emission in the Bulk in a Rotating Black Hole Background
• Bulk emission of scalars by a rotating black hole
• Effective Temperatures and Radiation Spectra for a Higher-Dimensional Schwarzschild-de-Sitter Black-Hole
• Graviton Emission in the Bulk by a Simply Rotating Black Hole
• Geometric model of black hole quantum $N$-portrait, extradimensions and thermodynamics
• Angular profile of emission of non-zero spin fields from a higher-dimensional black hole
• Hawking evaporation of cosmogenic black holes in TeV-gravity models
• Radiation Spectra and Effective Temperatures in Higher-Dimensional Charged-de Sitter Black Holes
• Planck scale black holes - Theory vs. observations
• Black holes, TeV-scale gravity and the LHC
• Signatures of TeV gravity from the evaporation of cosmogenic black holes