Форма представления | Статьи в зарубежных журналах и сборниках |
Год публикации | 2017 |
Язык | русский |
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Агафонов Александр Алексеевич, автор
Игнатьев Юрий Геннадиевич, автор
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Библиографическое описание на языке оригинала |
Yu. G. Ignat'ev and A. A. Agathonov. Qualitative and Numerical Analysis of a Cosmological Model Based on a Phantom Scalar Field with Self-Interaction // Gravitation and Cosmology, 2017, Vol. 23, No. 3, pp. 230–235.
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Аннотация |
We investigate the asymptotic behavior of a cosmological model based on a phantom scalar field by qualitative analysis of the set of differential equations. We show that, as opposed to models with a classical scalar field, such models have stable asymptotic solutions with a constant value of the potential both in the infinite past and the infinite future. We also develop numerical models of the cosmological evolution with a phantom scalar field. |
Ключевые слова |
relativistic gravitation, cosmology, phantom field, quality theory, dynamic systems, numeric modeling |
Название журнала |
Gravitation and Cosmology
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Пожалуйста, используйте этот идентификатор, чтобы цитировать или ссылаться на эту карточку |
https://repository.kpfu.ru/?p_id=161092 |
Полная запись метаданных |
Поле DC |
Значение |
Язык |
dc.contributor.author |
Агафонов Александр Алексеевич |
ru_RU |
dc.contributor.author |
Игнатьев Юрий Геннадиевич |
ru_RU |
dc.date.accessioned |
2017-01-01T00:00:00Z |
ru_RU |
dc.date.available |
2017-01-01T00:00:00Z |
ru_RU |
dc.date.issued |
2017 |
ru_RU |
dc.identifier.citation |
Yu. G. Ignat'ev and A. A. Agathonov. Qualitative and Numerical Analysis of a Cosmological Model Based on a Phantom Scalar Field with Self-Interaction // Gravitation and Cosmology, 2017, Vol. 23, No. 3, pp. 230–235.
|
ru_RU |
dc.identifier.uri |
https://repository.kpfu.ru/?p_id=161092 |
ru_RU |
dc.description.abstract |
Gravitation and Cosmology |
ru_RU |
dc.description.abstract |
We investigate the asymptotic behavior of a cosmological model based on a phantom scalar field by qualitative analysis of the set of differential equations. We show that, as opposed to models with a classical scalar field, such models have stable asymptotic solutions with a constant value of the potential both in the infinite past and the infinite future. We also develop numerical models of the cosmological evolution with a phantom scalar field. |
ru_RU |
dc.language.iso |
ru |
ru_RU |
dc.subject |
relativistic gravitation |
ru_RU |
dc.subject |
cosmology |
ru_RU |
dc.subject |
phantom field |
ru_RU |
dc.subject |
quality theory |
ru_RU |
dc.subject |
dynamic systems |
ru_RU |
dc.subject |
numeric modeling |
ru_RU |
dc.title |
Yu. G. Ignat'ev and A. A. Agathonov. Qualitative and Numerical Analysis of a Cosmological Model Based on a Phantom Scalar Field with Self-Interaction // Gravitation and Cosmology, 2017, Vol. 23, No. 3, pp. 230–235. |
ru_RU |
dc.type |
Статьи в зарубежных журналах и сборниках |
ru_RU |
|