| Форма представления | Статьи в зарубежных журналах и сборниках |
| Год публикации | 2022 |
| Язык | английский |
|
Игнатьев Юрий Геннадиевич, автор
|
| Библиографическое описание на языке оригинала |
Yu. G. Ignat'ev, Single-Field Model of Gravitational-Scalar Instability.
II. Black Hole Formation // Gravitation and Cosmology, 2022, Vol. 28, No. 4, pp. 375–381.
|
| Аннотация |
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 onecomponent statistical system of scalarly charged degenerate fermions (Mc 1 models), has led to the possibility
of black hole formation in the earlyUniverse using the mechanism of gravitational-scalar instability, which ensures the exponential growth of perturbations. The evolution of sphericalmasses in theMc 1 model,
as well as the evolution of black holes with allowance for their evaporation, is studied. Arguments in favor of the possibility of black hole formation in the early Universe with the help of the proposed mechanism
is given, and a numerical model is constructed that confirms this reasoning. The range of parameters of theMc 1 model, which ensures the growth of black hole masses in the early Universe up to 104−106M
, is identified. |
| Ключевые слова |
black hoyles, formation, higgs field, degenerative fermions, cjsmology, unstability |
| Название журнала |
GRAVITATION & COSMOLOGY
|
| URL |
https://link.springer.com/article/10.1134/S0202289322040107 |
| Пожалуйста, используйте этот идентификатор, чтобы цитировать или ссылаться на эту карточку |
https://repository.kpfu.ru/?p_id=271074 |
Полная запись метаданных  |
| Поле DC |
Значение |
Язык |
| dc.contributor.author |
Игнатьев Юрий Геннадиевич |
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, Single-Field Model of Gravitational-Scalar Instability.
II. Black Hole Formation // Gravitation and Cosmology, 2022, Vol. 28, No. 4, pp. 375–381.
|
ru_RU |
| dc.identifier.uri |
https://repository.kpfu.ru/?p_id=271074 |
ru_RU |
| dc.description.abstract |
GRAVITATION & COSMOLOGY |
ru_RU |
| dc.description.abstract |
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 onecomponent statistical system of scalarly charged degenerate fermions (Mc 1 models), has led to the possibility
of black hole formation in the earlyUniverse using the mechanism of gravitational-scalar instability, which ensures the exponential growth of perturbations. The evolution of sphericalmasses in theMc 1 model,
as well as the evolution of black holes with allowance for their evaporation, is studied. Arguments in favor of the possibility of black hole formation in the early Universe with the help of the proposed mechanism
is given, and a numerical model is constructed that confirms this reasoning. The range of parameters of theMc 1 model, which ensures the growth of black hole masses in the early Universe up to 104−106M
, is identified. |
ru_RU |
| dc.language.iso |
ru |
ru_RU |
| dc.subject |
black hoyles |
ru_RU |
| dc.subject |
formation |
ru_RU |
| dc.subject |
higgs field |
ru_RU |
| dc.subject |
degenerative fermions |
ru_RU |
| dc.subject |
cjsmology |
ru_RU |
| dc.subject |
unstability |
ru_RU |
| dc.title |
Single-Field Model of Gravitational-Scalar Instability.
II. Black Hole Formation |
ru_RU |
| dc.type |
Статьи в зарубежных журналах и сборниках |
ru_RU |
|
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