A Kinetics Of The Non-Equilibrium Universe. II. A Kinetics Of The Local Thermodynamical Equilibrium's Recovery

TL;DR

This paper investigates the process and conditions under which local thermodynamical equilibrium is restored in the early Universe, considering weak initial violations and their cosmological implications.

Contribution

It introduces a kinetic model for the recovery of thermal equilibrium in the early Universe with superhigh energy interactions, focusing on weak initial violations.

Findings

Thermal equilibrium can be restored under certain conditions.

Weak initial violations have significant cosmological consequences.

The model predicts specific timescales for equilibrium recovery.

Abstract

It has been researched the kinetics of the thermal equilibrium's establishment in an early Universe under the assumption of the recovery of interaction scaling of elementary particles in range of superhigh energies. The case of the thermal equilibrium's weak initial violation and basic cosmological consequences of the thermal equilibrium's violation have been researched.