# The Kinetics Of Nonequilibrium Universe. I. The Condition Of Local Thermodynamical Equilibrium

Source: [The Kinetics Of Nonequilibrium Universe. I. The Condition Of Local Thermodynamical Equilibrium](<https://www.sota2.com/research/paper/68fa2a691e209131ce83d217>)

Collection index: [llms.txt](<https://www.sota2.com/research/llms.txt>)

Data updated: 2025-10-27T03:15:19.018Z

Authors: Yurii G. Ignatyev

Published: 2011-01-01T19:30:14.000Z

## Abstract

In terms of fundamental principles of quantum theory of interacting particles and relativistic kinetic theory there was carried out an analysis of the main principle of standard cosmological scenario - the initial existence of local thermodynamical equilibrium. It has been shown, that condition of the existence of local thermodynamical equilibrium in Universe is determined essentially by means of function of total cross-section of particles' interaction from the kinematic invariant and in case of scaling's recovery in range of superhigh energies it is initially broken.

## Recorded benchmark results

A research result applies to its stated dataset, split, metric and evaluation configuration. Compare like-for-like settings, preserve the metric's unit and direction, and distinguish paper-reported results from independent reproduction. The best result recorded here is not a claim of exhaustive, current global coverage.

## Original sources and implementation

[Original paper](<https://arxiv.org/abs/1101.0364>)

[PDF](<https://arxiv.org/pdf/1101.0364.pdf>)
