Form of presentation | Articles in international journals and collections |
Year of publication | 2023 |
Язык | английский |
|
Ignatev Yuriy Gennadievich, author
|
Bibliographic description in the original language |
Yu. G. Ignat'ev, Two-Field Model of Gravitational-Scalar Instability and Formation
of Supermassive Black Holes in the Early Universe // Gravitation and Cosmology, 2023, Vol. 29, No. 2, pp. 163–176.
|
Annotation |
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 at early stages of expansion arises
in the model under study at sufficiently large scalar charges, and the instability develops near unstable points of the vacuum doublet. Short-wave 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). |
Keywords |
gravitation, cosmology, black holes, scalar-gravitation unstability, Higgs scalar fields, two-fields model, scalar charged fermions |
The name of the journal |
Gravitation and Cosmology
|
URL |
https://link.springer.com/article/10.1134/S0202289323020056 |
Please use this ID to quote from or refer to the card |
https://repository.kpfu.ru/eng/?p_id=279183&p_lang=2 |
Full metadata record |
Field DC |
Value |
Language |
dc.contributor.author |
Ignatev Yuriy Gennadievich |
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 // Gravitation and Cosmology, 2023, Vol. 29, No. 2, pp. 163–176.
|
ru_RU |
dc.identifier.uri |
https://repository.kpfu.ru/eng/?p_id=279183&p_lang=2 |
ru_RU |
dc.description.abstract |
Gravitation and 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 at early stages of expansion arises
in the model under study at sufficiently large scalar charges, and the instability develops near unstable points of the vacuum doublet. Short-wave 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 |
black holes |
ru_RU |
dc.subject |
scalar-gravitation unstability |
ru_RU |
dc.subject |
Higgs scalar fields |
ru_RU |
dc.subject |
two-fields model |
ru_RU |
dc.subject |
scalar charged fermions |
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 |
Articles in international journals and collections |
ru_RU |
|