  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.
