On phase transitions near black holes

TL;DR

This paper investigates phase transitions near black holes, focusing on temperature conditions close to the horizon and their implications for particle collisions and radiation emissions.

Contribution

It provides numerical estimates of the distance from the horizon and radiation emitted during particle collisions near rotating black holes, linking black hole physics with Standard Model phase transitions.

Findings

Temperatures near black hole horizons can reach phase transition levels.

Numerical estimates of collision radiation near black holes.

Potential implications for Standard Model physics in strong gravity environments.

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.