On the limiting energy of the collision of elementary particles close to horizon of the rotating black hole
arXiv:1911.03392 · doi:10.1142/S0217732320502624
Abstract
Arguments are given for the conclusion that the energy of collision of two ultrarelativistic elementary particles due to gravitational radiation cannot exceed the Planck value. Comparison of the gravitational and electromagnetic radiation for charged particles close to the horizon of Kerr black hole is made. If for trans-Planckian energy the black hole can arise it is shown that the energy growth used in scattering for interaction of particles is still limited.
9 pages, no figures, published version
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