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      Black Holes Radiate Mainly on the Brane

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          Abstract

          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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          Author and article information

          Journal
          14 March 2000
          2000-06-06
          Article
          10.1103/PhysRevLett.85.499
          hep-th/0003118
          528e4f55-df09-4d3a-a4f6-5b2fbb5e9c03
          History
          Custom metadata
          Phys.Rev.Lett.85:499-502,2000
          11 pages
          hep-th gr-qc hep-ph

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