Form of presentation | Articles in international journals and collections |
Year of publication | 2018 |
Язык | английский |
|
Agafonov Aleksandr Alekseevich, author
Ignatev Yuriy Gennadievich, author
Kokh Irina Aleksandrovna, author
|
Bibliographic description in the original language |
Yurii Ignat'ev, Alexander Agathonov, Irina Kokh. The Peculiarities of the Cosmological Models Based on Nonlinear Classical and Phantom Fields with Minimal Interaction. II. The Cosmological Model Based on the Asymmetrical Scalar Doublet. // arXiv:1810.09873 [gr-qc]
|
Annotation |
A detailed comparative qualitative analysis and numerical simulation of evolution of the cosmological models based on the doublet of classical and phantom scalar fields with self-action. The 2-dimensional and 3-dimensional projections of the phase portraits of the corresponding dynamic system are built. Just as in the case of single scalar fields, the phase space of such systems, becomes multiply connected, the ranges of negative total effective energy unavailable for motion, getting appear here. The distinctive feature of the asymmetrical scalar doublet is the time dependency of the prohibited ranges' projections on the phase subspaces of each field as a result of which the existence of the limit cycles with null effective energy depends on the parameters of the field model and initial
conditions. The numerical models where the dynamic system has limit cycles on hypersurfaces of null energy, arebuilt. It is shown, that even quite weak phantom field in such model undertakes functions |
Keywords |
cosmological model, phantom and classical scalar fields, quality analysis, asymptotic behavior, numerical simulation |
The name of the journal |
arXiv: General Relativity and Quantum Cosmology
|
URL |
https://arxiv.org/pdf/1810.09873.pdf |
Please use this ID to quote from or refer to the card |
https://repository.kpfu.ru/eng/?p_id=187095&p_lang=2 |
Full metadata record |
Field DC |
Value |
Language |
dc.contributor.author |
Agafonov Aleksandr Alekseevich |
ru_RU |
dc.contributor.author |
Ignatev Yuriy Gennadievich |
ru_RU |
dc.contributor.author |
Kokh Irina Aleksandrovna |
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 |
Yurii Ignat'ev, Alexander Agathonov, Irina Kokh. The Peculiarities of the Cosmological Models Based on Nonlinear Classical and Phantom Fields with Minimal Interaction. II. The Cosmological Model Based on the Asymmetrical Scalar Doublet. // arXiv:1810.09873 [gr-qc]
|
ru_RU |
dc.identifier.uri |
https://repository.kpfu.ru/eng/?p_id=187095&p_lang=2 |
ru_RU |
dc.description.abstract |
arXiv: General Relativity and Quantum Cosmology |
ru_RU |
dc.description.abstract |
A detailed comparative qualitative analysis and numerical simulation of evolution of the cosmological models based on the doublet of classical and phantom scalar fields with self-action. The 2-dimensional and 3-dimensional projections of the phase portraits of the corresponding dynamic system are built. Just as in the case of single scalar fields, the phase space of such systems, becomes multiply connected, the ranges of negative total effective energy unavailable for motion, getting appear here. The distinctive feature of the asymmetrical scalar doublet is the time dependency of the prohibited ranges' projections on the phase subspaces of each field as a result of which the existence of the limit cycles with null effective energy depends on the parameters of the field model and initial
conditions. The numerical models where the dynamic system has limit cycles on hypersurfaces of null energy, arebuilt. It is shown, that even quite weak phantom field in such model undertakes functions |
ru_RU |
dc.language.iso |
ru |
ru_RU |
dc.subject |
cosmological model |
ru_RU |
dc.subject |
phantom and classical scalar fields |
ru_RU |
dc.subject |
quality analysis |
ru_RU |
dc.subject |
asymptotic behavior |
ru_RU |
dc.subject |
numerical simulation |
ru_RU |
dc.title |
Yurii Ignat'ev, Alexander Agathonov, Irina Kokh. The Peculiarities of the Cosmological Models Based on Nonlinear Classical and Phantom Fields with Minimal Interaction. II. The Cosmological Model Based on the Asymmetrical Scalar Doublet. // arXiv:1810.09873 [gr-qc] |
ru_RU |
dc.type |
Articles in international journals and collections |
ru_RU |
|