Rotating black holes at future colliders. III. Determination of black hole evolution
Abstract
TeV scale gravity scenario predicts that the black hole production dominates over all other interactions above the scale and that the Large Hadron Collider will be a black hole factory. Such higherdimensional black holes mainly decay into the standard model fields via the Hawking radiation whose spectrum can be computed from the greybody factor. Here we complete the series of our work by showing the greybody factors and the resultant spectra for the branelocalized spinor and vector field emissions for arbitrary frequencies. Combining these results with the previous works, we determine the complete radiation spectra and the subsequent time evolution of the black hole. We find that, for a typical event, well more than half a black hole mass is emitted when the hole is still highly rotating, confirming our previous claim that it is important to take into account the angular momentum of black holes.
 Publication:

Physical Review D
 Pub Date:
 June 2006
 DOI:
 10.1103/PhysRevD.73.124022
 arXiv:
 arXiv:hepth/0602188
 Bibcode:
 2006PhRvD..73l4022I
 Keywords:

 04.70.Dy;
 04.50.+h;
 11.25.Mj;
 11.25.Wx;
 Quantum aspects of black holes evaporation thermodynamics;
 Gravity in more than four dimensions KaluzaKlein theory unified field theories;
 alternative theories of gravity;
 Compactification and fourdimensional models;
 String and brane phenomenology;
 High Energy Physics  Theory;
 General Relativity and Quantum Cosmology;
 High Energy Physics  Phenomenology
 EPrint:
 typoes in eqs(82)(84) corrected