Thermal Equations of the Radiation Dominated Universe Evolution
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.
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| Veröffentlicht in: | Vestnik Samarskogo gosudarstvennogo tehničeskogo universiteta. Seriâ Fiziko-matematičeskie nauki 2011-03, Vol.1(22), p.297-304 |
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| Hauptverfasser: | , |
| Format: | Artikel |
| Sprache: | eng ; rus |
| Online-Zugang: | Volltext |
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| Zusammenfassung: | 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. |
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| ISSN: | 1991-8615 2310-7081 |
| DOI: | 10.14498/vsgtu896 |