Center of Mass Energy of Three General Geodesic Colliding Particles Around a Kerr-MOG Black Hole

TL;DR

This paper investigates the center of mass energy resulting from the collision of three particles near a Kerr-MOG black hole, revealing conditions under which extremely high energies can be achieved close to the horizon.

Contribution

It provides a detailed analysis of three-particle collisions in Kerr-MOG black holes and identifies scenarios for ultra-high energy collisions near the horizons.

Findings

High center of mass energy is achievable near the horizons.

Extremal and non-extremal Kerr-MOG black holes both permit large collision energies.

Constraints limit but do not prevent ultra-high energy collisions.

Abstract

In this research paper, we scrutinize the center of mass energy of the collision for three neutral particles with different rest masses falling freely from rest at infinity in the vicinity of a Kerr-Modified-Gravity black hole. In addition, we deliberate the center of mass energy adjacent to the horizon(s) of an extremal and non-extremal Kerr-Modified-Gravity black hole and demonstrate that a swiftly huge center of mass energy is attainable concealed by few constraints.