KFU. Card publication. Complete cosmological evolution model of a classical scalar field with a higgs potential. II. Numerical simulation.

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FEDERAL UNIVERSITY

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COMPLETE COSMOLOGICAL EVOLUTION MODEL OF A CLASSICAL SCALAR FIELD WITH A HIGGS POTENTIAL. II. NUMERICAL SIMULATION.

Form of presentation

Articles in international journals and collections

Year of publication

2021

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Authors, employees of KFU

Ignatev Yuriy Gennadievich, author

Samigullina Alsu Rinatovna, author

Bibliographic description in the original language

Yu. G. Ignat'ev, A. R. Samigullina. Complete cosmological evolution model of a classical scalar field with a higgs potential. II. Numerical simulation. // arXiv:2111.01133 [gr-qc]

Annotation

A complete cosmological evolution model of the classical scalar field with a Higgs potential is studied and simulated on a computer without the assumption that the Hubble constant is nonnegative. It is shown that with most initial conditions, the cosmological model goes from the expansion stage to the compression stage. Thus, cosmological models based on the classical Higgs field are unstable to finite perturbations.

Keywords

cosmological models, Higgs fields, Einstein-Higgs hypersurface, global behavior.

The name of the journal

arXiv: General Relativity and Quantum Cosmology

URL

https://arxiv.org/abs/2111.01133

Please use this ID to quote from or refer to the card

https://repository.kpfu.ru/eng/?p_id=258702&p_lang=2

Full metadata record

Field DC	Value	Language
dc.contributor.author	Ignatev Yuriy Gennadievich	ru_RU
dc.contributor.author	Samigullina Alsu Rinatovna	ru_RU
dc.date.accessioned	2021-01-01T00:00:00Z	ru_RU
dc.date.available	2021-01-01T00:00:00Z	ru_RU
dc.date.issued	2021	ru_RU
dc.identifier.citation	Yu. G. Ignat'ev, A. R. Samigullina. Complete cosmological evolution model of a classical scalar field with a higgs potential. II. Numerical simulation. // arXiv:2111.01133 [gr-qc]	ru_RU
dc.identifier.uri	https://repository.kpfu.ru/eng/?p_id=258702&p_lang=2	ru_RU
dc.description.abstract	arXiv: General Relativity and Quantum Cosmology	ru_RU
dc.description.abstract	A complete cosmological evolution model of the classical scalar field with a Higgs potential is studied and simulated on a computer without the assumption that the Hubble constant is nonnegative. It is shown that with most initial conditions, the cosmological model goes from the expansion stage to the compression stage. Thus, cosmological models based on the classical Higgs field are unstable to finite perturbations.	ru_RU
dc.language.iso	ru	ru_RU
dc.subject	cosmological models	ru_RU
dc.subject	Higgs fields	ru_RU
dc.subject	Einstein-Higgs hypersurface	ru_RU
dc.subject	global behavior.	ru_RU
dc.title	Complete cosmological evolution model of a classical scalar field with a higgs potential. II. Numerical simulation.	ru_RU
dc.type	Articles in international journals and collections	ru_RU