In the context of the scenario with Large Extra Dimensions, we investigate the emission spectra for Hawking radiation on the brane from a variety of higher‐dimensional black holes: Schwarzschild, Kerr and Schwarzschild ‐ de Sitter. The energy emission spectra in each case are presented, and their dependence on the spin of the emitted particle, dimension of spacetime, angular momentum of the black hole and cosmological constant of spacetime is discussed.

Topics
General relativity, Hawking radiation, Cosmological constant, Black holes, Emission spectroscopy, Kerr effects
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© 2007 American Institute of Physics.
2007
American Institute of Physics
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