The complete relativistic kinetic model of violation of symmetry in isotopic expanding plasma and production of baryons in hot Universe. II. Numerical model: X-boson distribution function

TL;DR

This paper develops a numerical relativistic kinetic model to calculate the distribution function of X-bosons, exploring baryon production in the early hot Universe with symmetry violations.

Contribution

It introduces a detailed numerical approach to model the distribution of X-bosons in a relativistic expanding universe, advancing understanding of baryogenesis mechanisms.

Findings

Calculated X-boson distribution functions in a relativistic cosmological setting

Provided insights into symmetry violation effects on baryon production

Enhanced modeling accuracy of early Universe particle dynamics

Abstract

In terms of proposed by authors general-relativistic kinetic model of baryon production in expanding primordially symmetrical hot Universe calculates distribution function of extra-massive bosons and concerned with it variables.