КФУ. Карточка публикации. Complete cosmological evolution model of a classical scalar field with a Higgs potential.III. Features of phase trajectory flows.

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COMPLETE COSMOLOGICAL EVOLUTION MODEL OF A CLASSICAL SCALAR FIELD WITH A HIGGS POTENTIAL.III. FEATURES OF PHASE TRAJECTORY FLOWS.

Форма представления

Статьи в зарубежных журналах и сборниках

Год публикации

2022

Язык

английский

Авторы, сотрудники КФУ

Игнатьев Юрий Геннадиевич, автор

Самигуллина Алсу Ринатовна, автор

Библиографическое описание на языке оригинала

Yu. G. Ignat'ev and A. R. Samigullina. Complete cosmological evolution model of a classical scalar field with a Higgs potential.III. Features of phase trajectory flows. // Russ. Phys. J., Vol. 64, No. 10, 1808-1814

Аннотация

The flows of phase trajectories of cosmological models based on the vacuum classical Higgs field and their behavior on the Einstein–Higgs surface near singular points of a dynamical system are investigated by numerical simulation. The influence of the singular points on the process of phase flow splitting is shown and the efficiency of the Einstein–Higgs hypersurface application is demonstrated.

Ключевые слова

cosmology,scalar field,phase fluids, mathematic modelling,,dynamic systems

Название журнала

Russian Physics Journal

URL

https://link.springer.com/article/10.1007/s11182-022-02529-0

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https://repository.kpfu.ru/?p_id=264101

Полная запись метаданных

Поле DC	Значение	Язык
dc.contributor.author	Игнатьев Юрий Геннадиевич	ru_RU
dc.contributor.author	Самигуллина Алсу Ринатовна	ru_RU
dc.date.accessioned	2022-01-01T00:00:00Z	ru_RU
dc.date.available	2022-01-01T00:00:00Z	ru_RU
dc.date.issued	2022	ru_RU
dc.identifier.citation	Yu. G. Ignat'ev and A. R. Samigullina. Complete cosmological evolution model of a classical scalar field with a Higgs potential.III. Features of phase trajectory flows. // Russ. Phys. J., Vol. 64, No. 10, 1808-1814	ru_RU
dc.identifier.uri	https://repository.kpfu.ru/?p_id=264101	ru_RU
dc.description.abstract	Russian Physics Journal	ru_RU
dc.description.abstract	The flows of phase trajectories of cosmological models based on the vacuum classical Higgs field and their behavior on the Einstein–Higgs surface near singular points of a dynamical system are investigated by numerical simulation. The influence of the singular points on the process of phase flow splitting is shown and the efficiency of the Einstein–Higgs hypersurface application is demonstrated.	ru_RU
dc.language.iso	ru	ru_RU
dc.subject	cosmology	ru_RU
dc.subject	scalar field	ru_RU
dc.subject	phase fluids	ru_RU
dc.subject	mathematic modelling	ru_RU
dc.subject		ru_RU
dc.subject	dynamic systems	ru_RU
dc.title	Complete cosmological evolution model of a classical scalar field with a Higgs potential.III. Features of phase trajectory flows.	ru_RU
dc.type	Статьи в зарубежных журналах и сборниках	ru_RU