On brane-world black holes and short scale physics
arXiv:hep-ph/0304099 · doi:10.1016/S0003-4916(03)00117-9
Abstract
There is evidence that trans-Planckian physics does not affect the Hawking radiation in four dimensions and, consequently, deviations from the linear dispersion relation (for massless particles) at very high energies cannot be revealed using four-dimensional black holes. We study this issue in the context of models with extra spatial dimensions and show that small black holes that could be produced in accelerators might also provide a chance of testing the high energy regime where non-linear dispersion relations are generally expected.
14 pages, 5 figures
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- Black Holes in Theories with Large Extra Dimensions: a Review
- Hawking Radiation from a (4+n)-dimensional Black Hole: Exact Results for the Schwarzschild Phase
- Quantum Gravity Effects in Black Holes at the LHC
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