Form of presentation | Articles in international journals and collections |
Year of publication | 2022 |
Язык | английский |
|
Ignatev Yuriy Gennadievich, author
|
Bibliographic description in the original language |
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.
|
Annotation |
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. |
Keywords |
black hoyles, formation, higgs field, degenerative fermions, cjsmology, unstability |
The name of the journal |
GRAVITATION & COSMOLOGY
|
URL |
https://link.springer.com/article/10.1134/S0202289322040107 |
Please use this ID to quote from or refer to the card |
https://repository.kpfu.ru/eng/?p_id=271074&p_lang=2 |
Full metadata record |
Field DC |
Value |
Language |
dc.contributor.author |
Ignatev Yuriy Gennadievich |
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/eng/?p_id=271074&p_lang=2 |
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 |
Articles in international journals and collections |
ru_RU |
|