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, A. R. Samigullina. Complete cosmological evolution model of a classical scalar field with a Higgs potential. III. Features of phase trajectory flows // arXiv:2203.13667 [gr-qc]
|
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 |
gravitation, cosmology, scalar field, cosmological model, phase trajectories, numeric modeling |
The name of the journal |
arXiv: General Relativity and Quantum Cosmology
|
URL |
https://arxiv.org/abs/2203.13667 |
Please use this ID to quote from or refer to the card |
https://repository.kpfu.ru/eng/?p_id=264307&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, A. R. Samigullina. Complete cosmological evolution model of a classical scalar field with a Higgs potential. III. Features of phase trajectory flows // arXiv:2203.13667 [gr-qc]
|
ru_RU |
dc.identifier.uri |
https://repository.kpfu.ru/eng/?p_id=264307&p_lang=2 |
ru_RU |
dc.description.abstract |
arXiv: General Relativity and Quantum Cosmology |
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 |
gravitation |
ru_RU |
dc.subject |
cosmology |
ru_RU |
dc.subject |
scalar field |
ru_RU |
dc.subject |
cosmological model |
ru_RU |
dc.subject |
phase trajectories |
ru_RU |
dc.subject |
numeric modeling |
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 |
|