A Kinetics of non-equilibrium Universe. III. Stability of non-equilibrium scenario

TL;DR

This paper investigates how initial non-equilibrium conditions affect the process of reaching thermodynamic equilibrium in the early Universe, considering particle interactions at superhigh energies.

Contribution

It introduces a detailed analysis of the impact of initial distribution parameters on equilibrium recovery in a non-equilibrium cosmological scenario.

Findings

Initial distribution parameters significantly influence equilibrium recovery times

Scaling interactions at superhigh energies affect thermodynamical processes

The study provides a framework for understanding early Universe thermodynamics

Abstract

An influence of initial distribution nonequilibrium parameters on thermodynamical equilibrium recovery processes in early Universe under the assumption of elementary particles' scaling of interactions in range of superhigh energies is researched.