Transplanckian bremsstrahlung and black hole production
arXiv:0908.0675 · doi:10.1016/j.physletb.2009.12.042
Abstract
Classical gravitational bremsstrahlung in particle collisions at transplanckian energies is studied in . The radiation efficiency is computed in terms of the Schwarzschild radius , the impact parameter and the Lorentz factor and found to be , larger than previous estimates by many powers of . The result is reliable for impact parameters in the overlap of , with marking (for ) the loss of the notion of classical trajectories and the Compton length of the scattered particles. The condition on and for extreme radiation damping and (presumably) no black hole production is also derived.
4 pages, revtex 4. The discussion section is changed to better clarify the region of validity of our calculation. The physical conclusions and the abstract are modified accordingly. A few more references added. We just added the preprint number CCTP-2010-18
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