Form of presentation | Articles in international journals and collections |
Year of publication | 2014 |
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Ignatev Yuriy Gennadievich, author
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Bibliographic description in the original language |
Yu. G. Ignatyev. Numerical Simulation of Thermodynamic Equilibrium Establishment in a Cosmological Model with Arbitrary Acceleration //Gravitation and Cosmology, 2014, Vol. 20, No. 1, pp. 99–105.
DOI: 10.1134/S0202289314020066 (Scopus, WoS)
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Annotation |
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.
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Keywords |
gravitational, cosmology, early Universary, nonequilibrium processes, cosmologigal acselaration |
The name of the journal |
Gravitation and Cosmology
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URL |
http://link.springer.com/article/10.1134/S0202289314020066 |
Please use this ID to quote from or refer to the card |
https://repository.kpfu.ru/eng/?p_id=80357&p_lang=2 |
Full metadata record |
Field DC |
Value |
Language |
dc.contributor.author |
Ignatev Yuriy Gennadievich |
ru_RU |
dc.date.accessioned |
2014-01-01T00:00:00Z |
ru_RU |
dc.date.available |
2014-01-01T00:00:00Z |
ru_RU |
dc.date.issued |
2014 |
ru_RU |
dc.identifier.citation |
Yu. G. Ignatyev. Numerical Simulation of Thermodynamic Equilibrium Establishment in a Cosmological Model with Arbitrary Acceleration //Gravitation and Cosmology, 2014, Vol. 20, No. 1, pp. 99–105.
DOI: 10.1134/S0202289314020066 (Scopus, WoS)
|
ru_RU |
dc.identifier.uri |
https://repository.kpfu.ru/eng/?p_id=80357&p_lang=2 |
ru_RU |
dc.description.abstract |
Gravitation and Cosmology |
ru_RU |
dc.description.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.
|
ru_RU |
dc.language.iso |
ru |
ru_RU |
dc.subject |
gravitational |
ru_RU |
dc.subject |
cosmology |
ru_RU |
dc.subject |
early Universary |
ru_RU |
dc.subject |
nonequilibrium processes |
ru_RU |
dc.subject |
cosmologigal acselaration |
ru_RU |
dc.title |
Yu. G. Ignatyev. Numerical Simulation of Thermodynamic Equilibrium Establishment in a Cosmological Model with Arbitrary Acceleration //Gravitation and Cosmology, 2014, Vol. 20, No. 1, pp. 99–105.
DOI: 10.1134/S0202289314020066
|
ru_RU |
dc.type |
Articles in international journals and collections |
ru_RU |
|