Form of presentation | Articles in international journals and collections |
Year of publication | 2014 |
|
Agafonov Aleksandr Alekseevich, author
Ignatev Dmitriy Yurevich, author
Ignatev Yuriy Gennadievich, author
Mikhaylov Mikhail Leonidovich, author
|
Bibliographic description in the original language |
Yurii Ignat'ev, Alexander Agathonov, Mikhail Mikhailov, Dmitry Ignatyev. Cosmological Evolution of Statistical System of Scalar Charged Particles. arXiv:1411.6244v1 [gr-qc]; http://arxiv.org/abs/1411.6244
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Annotation |
arXiv[gr-qc] |
Keywords |
physics of the early universe, particle physics - cosmology connection, inflation, phantom scalar interaction |
The name of the journal |
arXiv[gr-qc]
|
URL |
http://arxiv.org/abs/1411.6244 |
Please use this ID to quote from or refer to the card |
https://repository.kpfu.ru/eng/?p_id=91866&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.contributor.author |
Mikhaylov Mikhail Leonidovich |
ru_RU |
dc.date.accessioned |
2014-01-01T00:00:00Z |
ru_RU |
dc.date.available |
2014-01-01T00:00:00Z |
ru_RU |
dc.date.issued |
2014 |
ru_RU |
dc.identifier.citation |
Yurii Ignat'ev, Alexander Agathonov, Mikhail Mikhailov, Dmitry Ignatyev. Cosmological Evolution of Statistical System of Scalar Charged Particles. arXiv:1411.6244v1 [gr-qc]; http://arxiv.org/abs/1411.6244
|
ru_RU |
dc.identifier.uri |
https://repository.kpfu.ru/eng/?p_id=91866&p_lang=2 |
ru_RU |
dc.description.abstract |
arXiv[gr-qc] |
ru_RU |
dc.description.abstract |
In the paper we consider the macroscopic model of plasma of scalar charged particles, obtained by means of the statistical averaging of the microscopic equations of particle dynamics in a scalar field. On the basis of kinetic equations, obtained from averaging, and their strict integral consequences, a self-consistent set of equations is formulated which describes the self-gravitating plasma of scalar charged particles. It was obtained the corresponding closed cosmological model which also was numerically simulated for the case of one-component degenerated Fermi gas and two-component Boltzmann system. It was shown that results depend weakly on the choice of a statistical model. Two specific features of cosmological evolution of a statistical system of scalar charged particles were obtained with respect to cosmological evolution of the minimal interaction models: appearance of giant bursts of invariant cosmological acceleration $\Omega$ at the time interval $8\cdot10^3\div2\cdot10^4. |
ru_RU |
dc.language.iso |
ru |
ru_RU |
dc.subject |
physics of the early universe |
ru_RU |
dc.subject |
particle physics - cosmology connection |
ru_RU |
dc.subject |
inflation |
ru_RU |
dc.subject |
phantom scalar interaction |
ru_RU |
dc.title |
Yurii Ignat'ev, Alexander Agathonov, Mikhail Mikhailov, Dmitry Ignatyev. Cosmological Evolution of Statistical System of Scalar Charged Particles. arXiv:1411.6244v1 [gr-qc]; http://arxiv.org/abs/1411.6244
|
ru_RU |
dc.type |
Articles in international journals and collections |
ru_RU |
|