| Форма представления | Статьи в зарубежных журналах и сборниках |
| Год публикации | 2018 |
| Язык | английский |
|
Агафонов Александр Алексеевич, автор
Игнатьев Дмитрий Юрьевич, автор
Игнатьев Юрий Геннадиевич, автор
|
| Библиографическое описание на языке оригинала |
Yu. G. Ignat'ev, A. A. Agathonov, and D. Yu. Ignatyev. Statistical Cosmological Fermion Systems with Phantom Scalar Interaction of Particles // Gravitation and Cosmology, 2018, Vol. 24, No. 1, pp. 1–12.
DOI: 10.1134/S0202289318010085
|
| Аннотация |
The article represents a research of the cosmological evolution of fermion statistical systems with phantom scalar interaction where the “kinetic” term's contribution to the total energy of a scalar field is negative. As a result of analytical and numerical simulation of such systems, we have revealed the existence of four possible scenarios depending on the system's parameters and the initial conditions. Among them
are scenarios with an early, intermediate and late nonrelativistic stages of the cosmological evolution, all of which also have a necessary inflationary stage. This paper contains only a small part of the research results. In a more complete form, they are presented in arXiv: 1608.05020 [1]. |
| Ключевые слова |
gravitation, cosmology,relativistic statistics, phantom scalar fields, numerical gravitation |
| Название журнала |
Gravitation and Cosmology
|
| Пожалуйста, используйте этот идентификатор, чтобы цитировать или ссылаться на эту карточку |
https://repository.kpfu.ru/?p_id=173028 |
Полная запись метаданных  |
| Поле DC |
Значение |
Язык |
| dc.contributor.author |
Агафонов Александр Алексеевич |
ru_RU |
| dc.contributor.author |
Игнатьев Дмитрий Юрьевич |
ru_RU |
| dc.contributor.author |
Игнатьев Юрий Геннадиевич |
ru_RU |
| dc.date.accessioned |
2018-01-01T00:00:00Z |
ru_RU |
| dc.date.available |
2018-01-01T00:00:00Z |
ru_RU |
| dc.date.issued |
2018 |
ru_RU |
| dc.identifier.citation |
Yu. G. Ignat'ev, A. A. Agathonov, and D. Yu. Ignatyev. Statistical Cosmological Fermion Systems with Phantom Scalar Interaction of Particles // Gravitation and Cosmology, 2018, Vol. 24, No. 1, pp. 1–12.
DOI: 10.1134/S0202289318010085
|
ru_RU |
| dc.identifier.uri |
https://repository.kpfu.ru/?p_id=173028 |
ru_RU |
| dc.description.abstract |
Gravitation and Cosmology |
ru_RU |
| dc.description.abstract |
The article represents a research of the cosmological evolution of fermion statistical systems with phantom scalar interaction where the “kinetic” term's contribution to the total energy of a scalar field is negative. As a result of analytical and numerical simulation of such systems, we have revealed the existence of four possible scenarios depending on the system's parameters and the initial conditions. Among them
are scenarios with an early, intermediate and late nonrelativistic stages of the cosmological evolution, all of which also have a necessary inflationary stage. This paper contains only a small part of the research results. In a more complete form, they are presented in arXiv: 1608.05020 [1]. |
ru_RU |
| dc.language.iso |
ru |
ru_RU |
| dc.subject |
gravitation |
ru_RU |
| dc.subject |
cosmology |
ru_RU |
| dc.subject |
relativistic statistics |
ru_RU |
| dc.subject |
phantom scalar fields |
ru_RU |
| dc.subject |
numerical gravitation |
ru_RU |
| dc.title |
Yu. G. Ignat'ev, A. A. Agathonov, and D. Yu. Ignatyev. Statistical Cosmological Fermion Systems with Phantom Scalar Interaction of Particles // Gravitation and Cosmology, 2017, Vol. 24, No. 1, pp. 1–12.
DOI: 10.1134/S0202289318010085
|
ru_RU |
| dc.type |
Статьи в зарубежных журналах и сборниках |
ru_RU |
|
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