| Форма представления | Статьи в зарубежных журналах и сборниках |
| Год публикации | 2021 |
| Язык | русский |
|
Игнатьев Юрий Геннадиевич, автор
Самигуллина Алсу Ринатовна, автор
|
| Библиографическое описание на языке оригинала |
Yu. G. Ignat'ev, A. R. Samigullina. Complete cosmological evolution model of a classical scalar field with a higgs potential. II. Numerical simulation. // arXiv:2111.01133 [gr-qc]
|
| Аннотация |
A complete cosmological evolution model of the classical scalar field with a Higgs potential is studied and simulated on a computer without the assumption that the Hubble constant is nonnegative. It is shown that with most initial conditions, the cosmological model goes from the expansion stage to the compression stage. Thus, cosmological models based on the classical Higgs field are unstable to finite perturbations. |
| Ключевые слова |
cosmological models, Higgs fields, Einstein-Higgs hypersurface, global behavior. |
| Название журнала |
arXiv: General Relativity and Quantum Cosmology
|
| URL |
https://arxiv.org/abs/2111.01133 |
| Пожалуйста, используйте этот идентификатор, чтобы цитировать или ссылаться на эту карточку |
https://repository.kpfu.ru/?p_id=258702 |
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 |
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, A. R. Samigullina. Complete cosmological evolution model of a classical scalar field with a higgs potential. II. Numerical simulation. // arXiv:2111.01133 [gr-qc]
|
ru_RU |
| dc.identifier.uri |
https://repository.kpfu.ru/?p_id=258702 |
ru_RU |
| dc.description.abstract |
arXiv: General Relativity and Quantum Cosmology |
ru_RU |
| dc.description.abstract |
A complete cosmological evolution model of the classical scalar field with a Higgs potential is studied and simulated on a computer without the assumption that the Hubble constant is nonnegative. It is shown that with most initial conditions, the cosmological model goes from the expansion stage to the compression stage. Thus, cosmological models based on the classical Higgs field are unstable to finite perturbations. |
ru_RU |
| dc.language.iso |
ru |
ru_RU |
| dc.subject |
cosmological models |
ru_RU |
| dc.subject |
Higgs fields |
ru_RU |
| dc.subject |
Einstein-Higgs hypersurface |
ru_RU |
| dc.subject |
global behavior. |
ru_RU |
| dc.title |
Complete cosmological evolution model of a classical scalar field with a higgs potential. II. Numerical simulation. |
ru_RU |
| dc.type |
Статьи в зарубежных журналах и сборниках |
ru_RU |
|
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