| Форма представления | Статьи в зарубежных журналах и сборниках |
| Год публикации | 2023 |
| Язык | английский |
|
Игнатьев Юрий Геннадиевич, автор
|
| Библиографическое описание на языке оригинала |
Yu. G. Ignat'ev. Two-Field Model of Gravitational-Scalar Instability and Formation
of Supermassive Black Holes in the Early Universe // arXiv:2305.15456[physics.gen-ph]
|
| Аннотация |
Based on the previously formulated mathematical model of a statistical system with scalar interaction of fermions and the theory of gravitational-scalar instability of a cosmological model based on a two-component statistical system of scalarly charged degenerate fermions, a numerical model of the cosmological evolution of gravitational-scalar perturbations in the presence of classical and phantom scalar fields is constructed and studied. The gravitational-scalar instability in the early stages of expansion in the model under study arises at sufficiently large scalar charges, and the instability develops near the unstable points of the vacuum doublet. Shortwave perturbations of the free phantom field turn out to be stable at stable singular points of the vacuum doublet. It is shown that for sufficiently large scalar charges, mass perturbations can grow to the values of masses Black Hole Seeds (BHS). |
| Ключевые слова |
gravitation,cosmology,scalar charge,fermions,Higgs fields,asymmetric scalar doublet,scalar black holes,creation |
| Название журнала |
arXiv: General Relativity and Quantum Cosmology
|
| URL |
https://arxiv.org/abs/2305.15456 |
| Пожалуйста, используйте этот идентификатор, чтобы цитировать или ссылаться на эту карточку |
https://repository.kpfu.ru/?p_id=280806 |
Полная запись метаданных  |
| Поле DC |
Значение |
Язык |
| dc.contributor.author |
Игнатьев Юрий Геннадиевич |
ru_RU |
| dc.date.accessioned |
2023-01-01T00:00:00Z |
ru_RU |
| dc.date.available |
2023-01-01T00:00:00Z |
ru_RU |
| dc.date.issued |
2023 |
ru_RU |
| dc.identifier.citation |
Yu. G. Ignat'ev. Two-Field Model of Gravitational-Scalar Instability and Formation
of Supermassive Black Holes in the Early Universe // arXiv:2305.15456[physics.gen-ph]
|
ru_RU |
| dc.identifier.uri |
https://repository.kpfu.ru/?p_id=280806 |
ru_RU |
| dc.description.abstract |
arXiv: General Relativity and Quantum Cosmology |
ru_RU |
| dc.description.abstract |
Based on the previously formulated mathematical model of a statistical system with scalar interaction of fermions and the theory of gravitational-scalar instability of a cosmological model based on a two-component statistical system of scalarly charged degenerate fermions, a numerical model of the cosmological evolution of gravitational-scalar perturbations in the presence of classical and phantom scalar fields is constructed and studied. The gravitational-scalar instability in the early stages of expansion in the model under study arises at sufficiently large scalar charges, and the instability develops near the unstable points of the vacuum doublet. Shortwave perturbations of the free phantom field turn out to be stable at stable singular points of the vacuum doublet. It is shown that for sufficiently large scalar charges, mass perturbations can grow to the values of masses Black Hole Seeds (BHS). |
ru_RU |
| dc.language.iso |
ru |
ru_RU |
| dc.subject |
gravitation |
ru_RU |
| dc.subject |
cosmology |
ru_RU |
| dc.subject |
scalar charge |
ru_RU |
| dc.subject |
fermions |
ru_RU |
| dc.subject |
Higgs fields |
ru_RU |
| dc.subject |
asymmetric scalar doublet |
ru_RU |
| dc.subject |
scalar black holes |
ru_RU |
| dc.subject |
creation |
ru_RU |
| dc.title |
Two-Field Model of Gravitational-Scalar Instability and Formation
of Supermassive Black Holes in the Early Universe |
ru_RU |
| dc.type |
Статьи в зарубежных журналах и сборниках |
ru_RU |
|
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