Hawking radiation from rotating brane black holes
arXiv:0708.2656
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