(2015-12-16) Das, Saurya; Mukhopadhyay, Himan; Ramadevi, P.
The reduced phase space formalism for quantising black holes has recently been extended to
find the area and angular momentum spectra of four dimensional Kerr black holes. We extend
this further to rotating black holes in all spacetime dimensions and show that although as in four
dimensions the spectrum is discrete, it is not equispaced in general. As a result, Hawking radiation
spectra from these black holes are continuous, as opposed to the discrete spectrum predicted for
four dimensional black holes.