Form of presentation | Articles in international journals and collections |
Year of publication | 2022 |
Язык | английский |
|
Ignatev Yuriy Gennadievich, author
Samigullina Alsu Rinatovna, author
|
Bibliographic description in the original language |
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
|
Annotation |
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. |
Keywords |
cosmology,scalar field,phase fluids, mathematic modelling,,dynamic systems |
The name of the journal |
Russian Physics Journal
|
URL |
https://link.springer.com/article/10.1007/s11182-022-02529-0 |
Please use this ID to quote from or refer to the card |
https://repository.kpfu.ru/eng/?p_id=264101&p_lang=2 |
Full metadata record |
Field DC |
Value |
Language |
dc.contributor.author |
Ignatev Yuriy Gennadievich |
ru_RU |
dc.contributor.author |
Samigullina Alsu Rinatovna |
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/eng/?p_id=264101&p_lang=2 |
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 |
Articles in international journals and collections |
ru_RU |
|