Numerical simulation of thermodynamic equilibrium establishment in a cosmological model with arbitrary acceleration

Yu.G. Ignatyev1

Abstract

We present the results of a numerical simulation of the previously constructed strict mathematical model of thermodynamic equilibrium establishment in an originally nonequilibrium cosmological ultrarelativistic plasma in a universe with any acceleration, under the assumption of scaling restoration for elementary particle interactions at energies above a unitary limit. The limiting parametres are found for a residual nonequilibrium distribution of nonequilibrium relic ultra-high energy particles.

References

  1. Yu. G. IgnatÁ??ev, Russ. Phys. J. 56(6), 745 (2013).
  2. Yu. G. Ignatyev, arXiv: 1306.3633; Grav. Cosmol. 19(4), 232 (2013).
  3. Yu. G. IgnatÁ??ev, Sov. Phys. J. (Izv. Vuzov) 29(2), 19 (1986).
  4. Yu. G. Ignatyev and D. Yu. Ignatyev, Grav. Cosmol. 13 101 (2007).
  5. Yu. G. IgnatÁ??ev, Russ. Phys. J. 57(1), 15 (2014).
For more information about this paper please visit Springer's Home Page of this paper.



Back to The Contents Page