Upper limits on ADD black hole mass MB at 14 TeV LHC range from 11.83 TeV (ζ=0, D=3, ΛD=1 TeV) down to 7.65 TeV (ζ=0.35), with similar shifts for D=7 and higher ΛD.
Black Holes Radiate Mainly on the Brane
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We examine the evaporation of a small black hole on a brane in a world with large extra dimensions. Since the masses of many Kaluza-Klein modes are much smaller than the Hawking temperature of the black hole, it has been claimed that most of the energy is radiated into these modes. We show that this is incorrect. Most of the energy goes into the modes on the brane. This raises the possibility of observing Hawking radiation in future high energy colliders if there are large extra dimensions.
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Constraining ADD black holes at the LHC with $\sqrt{s} = 14$ TeV
Upper limits on ADD black hole mass MB at 14 TeV LHC range from 11.83 TeV (ζ=0, D=3, ΛD=1 TeV) down to 7.65 TeV (ζ=0.35), with similar shifts for D=7 and higher ΛD.