On phase transitions near black holes
arXiv:2211.04106 · doi:10.1134/S0021364022601907
Abstract
It has been shown that temperatures near the horizon of rotating black holes can be about the phase transition temperature in the Standard Model with the Higgs boson. The distance from the horizon and gravitational and electromagnetic radiation emitted in collisions between particles have been numerically estimated.
arXiv comment7 pages, accepted for publication in JETP Letters
References in corpus (9)
- Kerr Black Holes as Particle Accelerators to Arbitrarily High Energy
- On particle collisions in the gravitational field of the Kerr black hole
- On the collisions between particles in the vicinity of rotating black holes
- Collision of an object in the transition from adiabatic inspiral to plunge around a Kerr black hole
- Are SMBHs shrouded by "super-Oort" clouds of comets and asteroids?
- Schwarzschild black hole as accelerator of accelerated particles
- Black holes and particles with zero or negative energy
- Super-Penrose process for nonextremal black holes
- On the limiting energy of the collision of elementary particles close to horizon of the rotating black hole