  Black holes are predicted to be copiously produced at the CERN Large Hadron
Collider in the scenarios of TeV scale gravity. We report recent progress in
studying decay of such a higher dimensional black hole in D=4+n dimensions
through the Hawking radiation into brane localized fields taking into account
its angular momentum which is indispensable for realistic simulations.
Presented is the greybody factors for a scalar field emission, which confirms
our previous results in low energy approximation: (i) the existence of
super-radiance modes and (ii) the non-trivial angular distribution of radiated
scalar field. Phenomenological implications and future plans are discussed.

High Energy Physics - Phenomenology