Thermal Equations of the Radiation Dominated Universe Evolution
Journal of Samara State Technical University, Ser. Physical and Mathematical Sciences, no. 1 (2011), pp. 297-304

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The equations of the evolution of the Universe in Friedmann model are considered using thermodynamic functions and temperature as function of time. The exit for frameworks of the standard model is carried out, the influence of dark energy is considered.
Mots-clés : radiation dominance, Universe evolution, thermal equations.
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M. V. Dolgopolov; E. Yu. Petrova. Thermal Equations of the Radiation Dominated Universe Evolution. Journal of Samara State Technical University, Ser. Physical and Mathematical Sciences, no. 1 (2011), pp. 297-304. http://geodesic.mathdoc.fr/item/VSGTU_2011_1_a37/