Form of presentation | Articles in international journals and collections |
Year of publication | 2018 |
Язык | английский |
|
Agafonov Aleksandr Alekseevich, author
Ignatev Dmitriy Yurevich, author
Ignatev Yuriy Gennadievich, author
|
Bibliographic description in the original language |
Yu. G. Ignat'ev, A. A. Agathonov, and D. Yu. Ignatyev. Statistical Cosmological Fermion Systems with Phantom Scalar Interaction of Particles // Gravitation and Cosmology, 2018, Vol. 24, No. 1, pp. 1–12.
DOI: 10.1134/S0202289318010085
|
Annotation |
The article represents a research of the cosmological evolution of fermion statistical systems with phantom scalar interaction where the “kinetic” term's contribution to the total energy of a scalar field is negative. As a result of analytical and numerical simulation of such systems, we have revealed the existence of four possible scenarios depending on the system's parameters and the initial conditions. Among them
are scenarios with an early, intermediate and late nonrelativistic stages of the cosmological evolution, all of which also have a necessary inflationary stage. This paper contains only a small part of the research results. In a more complete form, they are presented in arXiv: 1608.05020 [1]. |
Keywords |
gravitation, cosmology,relativistic statistics, phantom scalar fields, numerical gravitation |
The name of the journal |
Gravitation and Cosmology
|
Please use this ID to quote from or refer to the card |
https://repository.kpfu.ru/eng/?p_id=173028&p_lang=2 |
Full metadata record |
Field DC |
Value |
Language |
dc.contributor.author |
Agafonov Aleksandr Alekseevich |
ru_RU |
dc.contributor.author |
Ignatev Dmitriy Yurevich |
ru_RU |
dc.contributor.author |
Ignatev Yuriy Gennadievich |
ru_RU |
dc.date.accessioned |
2018-01-01T00:00:00Z |
ru_RU |
dc.date.available |
2018-01-01T00:00:00Z |
ru_RU |
dc.date.issued |
2018 |
ru_RU |
dc.identifier.citation |
Yu. G. Ignat'ev, A. A. Agathonov, and D. Yu. Ignatyev. Statistical Cosmological Fermion Systems with Phantom Scalar Interaction of Particles // Gravitation and Cosmology, 2018, Vol. 24, No. 1, pp. 1–12.
DOI: 10.1134/S0202289318010085
|
ru_RU |
dc.identifier.uri |
https://repository.kpfu.ru/eng/?p_id=173028&p_lang=2 |
ru_RU |
dc.description.abstract |
Gravitation and Cosmology |
ru_RU |
dc.description.abstract |
The article represents a research of the cosmological evolution of fermion statistical systems with phantom scalar interaction where the “kinetic” term's contribution to the total energy of a scalar field is negative. As a result of analytical and numerical simulation of such systems, we have revealed the existence of four possible scenarios depending on the system's parameters and the initial conditions. Among them
are scenarios with an early, intermediate and late nonrelativistic stages of the cosmological evolution, all of which also have a necessary inflationary stage. This paper contains only a small part of the research results. In a more complete form, they are presented in arXiv: 1608.05020 [1]. |
ru_RU |
dc.language.iso |
ru |
ru_RU |
dc.subject |
gravitation |
ru_RU |
dc.subject |
cosmology |
ru_RU |
dc.subject |
relativistic statistics |
ru_RU |
dc.subject |
phantom scalar fields |
ru_RU |
dc.subject |
numerical gravitation |
ru_RU |
dc.title |
Yu. G. Ignat'ev, A. A. Agathonov, and D. Yu. Ignatyev. Statistical Cosmological Fermion Systems with Phantom Scalar Interaction of Particles // Gravitation and Cosmology, 2017, Vol. 24, No. 1, pp. 1–12.
DOI: 10.1134/S0202289318010085
|
ru_RU |
dc.type |
Articles in international journals and collections |
ru_RU |
|