Форма представления | Статьи в зарубежных журналах и сборниках |
Год публикации | 2014 |
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Игнатьев Юрий Геннадиевич, автор
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Библиографическое описание на языке оригинала |
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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Аннотация |
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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Ключевые слова |
gravitational, cosmology, early Universary, nonequilibrium processes, cosmologigal acselaration |
Название журнала |
Gravitation and Cosmology
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URL |
http://link.springer.com/article/10.1134/S0202289314020066 |
Пожалуйста, используйте этот идентификатор, чтобы цитировать или ссылаться на эту карточку |
https://repository.kpfu.ru/?p_id=80357 |
Полная запись метаданных |
Поле DC |
Значение |
Язык |
dc.contributor.author |
Игнатьев Юрий Геннадиевич |
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/?p_id=80357 |
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.
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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 |
Статьи в зарубежных журналах и сборниках |
ru_RU |
|