Based on the strict mathematical model of restoration of thermodynamic equilibrium in an originally nonequilibrium Universe suggested by the author under assumption of restoration of interaction scaling in the region of energies above a unitary limit and on the exact solution of the Einstein equations, numerical models of this process in an accelerated Universe are constructed. © 2014 Springer Science+Business Media New York
The matter creation model of Prigogine–Géhéniau–Gunzig–Nardone is revisited in terms of a redefined ...
A self-consistent set of equations describing the evolution of linear spherically symmetrical pertur...
In this (second) part of the work we present the results of numerical and qualitative analysis, base...
Based on the strict mathematical model of restoration of thermodynamic equilibrium in an originally ...
An exact mathematical model of restoration of thermodynamic equilibrium in an initially nonequilibri...
We build a strict mathematical model of thermodynamic equilibrium establishment in an originally non...
Abstract. In this article there are considered non-equilibrium cosmological scenarios with the assum...
The pivotal point of the paper is to discuss the behavior of temperature, pressure, energy density a...
International audienceWe consider a flat Universe filled with a vacuum energy coupled to matter and ...
In a recent article, it has been shown that the system of relativistic thermodynamics previously dev...
If the cosmological term in the equations of relativistic mechanics is set equal to zero, it has bee...
The structure of the equation of state $\omega$ could be very complicate in nature while a few linea...
The evolution of a superthermal relict plasma component is studied using a nonequilibrium model of t...
ABSTRACT We present a thermodynamic approach in modeling the evolution of the universe ba...
A model for the Universe is proposed where it is considered as a mixture of scalar and matter fields...
The matter creation model of Prigogine–Géhéniau–Gunzig–Nardone is revisited in terms of a redefined ...
A self-consistent set of equations describing the evolution of linear spherically symmetrical pertur...
In this (second) part of the work we present the results of numerical and qualitative analysis, base...
Based on the strict mathematical model of restoration of thermodynamic equilibrium in an originally ...
An exact mathematical model of restoration of thermodynamic equilibrium in an initially nonequilibri...
We build a strict mathematical model of thermodynamic equilibrium establishment in an originally non...
Abstract. In this article there are considered non-equilibrium cosmological scenarios with the assum...
The pivotal point of the paper is to discuss the behavior of temperature, pressure, energy density a...
International audienceWe consider a flat Universe filled with a vacuum energy coupled to matter and ...
In a recent article, it has been shown that the system of relativistic thermodynamics previously dev...
If the cosmological term in the equations of relativistic mechanics is set equal to zero, it has bee...
The structure of the equation of state $\omega$ could be very complicate in nature while a few linea...
The evolution of a superthermal relict plasma component is studied using a nonequilibrium model of t...
ABSTRACT We present a thermodynamic approach in modeling the evolution of the universe ba...
A model for the Universe is proposed where it is considered as a mixture of scalar and matter fields...
The matter creation model of Prigogine–Géhéniau–Gunzig–Nardone is revisited in terms of a redefined ...
A self-consistent set of equations describing the evolution of linear spherically symmetrical pertur...
In this (second) part of the work we present the results of numerical and qualitative analysis, base...