Форма представления | Статьи в зарубежных журналах и сборниках |
Год публикации | 2021 |
Язык | русский |
|
Игнатьев Юрий Геннадиевич, автор
Кох Ирина Александровна, автор
|
Библиографическое описание на языке оригинала |
Yu. G. Ignat'ev and I. A. Kokh. Phase Flows in the Complete Model of Cosmological Evolution of the Asymmetric Scalar Higgs Doublet // Gravitation and Cosmology, 2021, Vol. 27, No. 4, pp. 350–357.
|
Аннотация |
The flows of phase trajectories in cosmological models based on the asymmetric scalar Higgs doublet are investigated. It is shown that phase flows tend to split into several diverging flows. In this case,
initially close phase trajectories can diverge significantly over time, which indicates the instability of the model with respect to finite perturbations. |
Ключевые слова |
phase flows,cosmological evolution, asymmetric scalar Higgs doublet |
Название журнала |
Gravitation and Cosmology
|
URL |
https://link.springer.com/article/10.1134/S0202289321040071 |
Пожалуйста, используйте этот идентификатор, чтобы цитировать или ссылаться на эту карточку |
https://repository.kpfu.ru/?p_id=258701 |
Полная запись метаданных |
Поле DC |
Значение |
Язык |
dc.contributor.author |
Игнатьев Юрий Геннадиевич |
ru_RU |
dc.contributor.author |
Кох Ирина Александровна |
ru_RU |
dc.date.accessioned |
2021-01-01T00:00:00Z |
ru_RU |
dc.date.available |
2021-01-01T00:00:00Z |
ru_RU |
dc.date.issued |
2021 |
ru_RU |
dc.identifier.citation |
Yu. G. Ignat'ev and I. A. Kokh. Phase Flows in the Complete Model of Cosmological Evolution of the Asymmetric Scalar Higgs Doublet // Gravitation and Cosmology, 2021, Vol. 27, No. 4, pp. 350–357.
|
ru_RU |
dc.identifier.uri |
https://repository.kpfu.ru/?p_id=258701 |
ru_RU |
dc.description.abstract |
Gravitation and Cosmology |
ru_RU |
dc.description.abstract |
The flows of phase trajectories in cosmological models based on the asymmetric scalar Higgs doublet are investigated. It is shown that phase flows tend to split into several diverging flows. In this case,
initially close phase trajectories can diverge significantly over time, which indicates the instability of the model with respect to finite perturbations. |
ru_RU |
dc.language.iso |
ru |
ru_RU |
dc.subject |
phase flows |
ru_RU |
dc.subject |
cosmological evolution |
ru_RU |
dc.subject |
asymmetric scalar Higgs doublet |
ru_RU |
dc.title |
Phase Flows in the Complete Model of Cosmological Evolution of the Asymmetric Scalar Higgs Doublet |
ru_RU |
dc.type |
Статьи в зарубежных журналах и сборниках |
ru_RU |
|