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Numerical Simulation of Establishment of thermodynamic equilibrium in cosmological model with an arbitrary acceleration

2013/10/08 by Yu. G. Ignatyev, Ignatyev, Yu. G.
Physics and Astronomy · #FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc) #gr-qc

paper · pdf · doi:10.48550/arxiv.1310.2183

16 pages, 15 figures, 5 references

arxiv created 2013/10/08 · arxiv updated 2013/10/09

Abstract

Results of numerical simulation constructed before strict mathematical model of an establishment of thermodynamic equilibrium in originally nonequilibrium cosmological ultrarelativistic plasma for the Universe with any acceleration in the assumption of restoration of a scalling of interactions of elementary particles are presented at energies above a unitary limit. Limiting parametres of residual nonequilibrium distribution of nonequilibrium relic particles of ultrahigh energies are found.

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