On the limiting energy of the collision of elementary particles close to horizon of the rotating black hole

Author:

Grib A. A.12,Pavlov Yu. V.34

Affiliation:

1. A. Friedmann Laboratory for Theoretical Physics, Saint Petersburg, Russia

2. Theoretical Physics and Astronomy Department of the Herzen University, Moika 48, Saint Petersburg 191186, Russia

3. Institute of Problems in Mechanical Engineering of Russian Academy of Sciences, Bol’shoy pr. 61, St. Petersburg 199178, Russia

4. N.I. Lobachevsky Institute of Mathematics and Mechanics, Kazan Federal University, 18 Kremlyovskaya St., Kazan 420008, Russia

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.

Funder

Russian Foundation for Basic Research

Publisher

World Scientific Pub Co Pte Lt

Subject

General Physics and Astronomy,Astronomy and Astrophysics,Nuclear and High Energy Physics

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