  We discuss the thermodynamics of the noncommutative inspired Kerr black hole
by means of a reformulated Hamilton-Jacobi method and a dimensional reduction
technique. In order to investigate the effect of the angular momentum of the
tunneling particle, we calculate the wave function to the first order of the
WKB ansatz. Then, using a density matrix technique we derive the radiation
spectrum from which the radiation temperature can be read out. Our results show
that the radiation of this noncommutative inspired black hole corresponds to a
modified temperature which involves the effect of noncommutativity. However,
the angular momentum of the tunneling particle has no influence on the
radiation temperature. Moreover, we analyze the entropy spectrum and verify
that its quantization is modified neither by the noncommutativity of spacetime
nor by the quantum correction of wave functions.

High Energy Physics - Theory;General Relativity and Quantum Cosmology