KFU. Card publication. A Complete Model of Cosmological Evolution of a Scalar Field with Higgs Potential and Euclidean Cycles

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A COMPLETE MODEL OF COSMOLOGICAL EVOLUTION OF A SCALAR FIELD WITH HIGGS POTENTIAL AND EUCLIDEAN CYCLES

Form of presentation

Articles in international journals and collections

Year of publication

2020

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Authors, employees of KFU

Ignatev Yuriy Gennadievich, author

Bibliographic description in the original language

Yu. G. Ignat'ev and D. Yu. Ignatyev. A Complete Model of Cosmological Evolution of a Scalar Field with Higgs Potential and Euclidean Cycles // Gravitation and Cosmology, 2020, Vol. 26, No. 1, pp. 29–37.

Annotation

A revision of the author's results concerning the possible existence of the so-called Euclidean cycles in cosmological evolution of a system of Higgs scalar fields is being performed. The assumption of a nonnegative velocity of the Universe expansion, which in certain cases contradicts the complete set of the Einstein equations, is removed. It is shown that in the cases where the effective energy of the system tends to zero, happens a smooth transition of the model to the range of negative values of the expansion rate, i.e., there is a transition to a collapsing stage rather than winding of the phase trajectories on the boundary of prohibited area. This process is studied with the help of numerical simulation methods for a model based on a classical scalar Higgs field.

Keywords

Higgs fields, cosmology, quality analysis, numerical modelling

The name of the journal

Gravitation and Cosmology

URL

https://link.springer.com/article/10.1134/S0202289320010065

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

https://repository.kpfu.ru/eng/?p_id=218916&p_lang=2

Full metadata record

Field DC	Value	Language
dc.contributor.author	Ignatev Yuriy Gennadievich	ru_RU
dc.date.accessioned	2020-01-01T00:00:00Z	ru_RU
dc.date.available	2020-01-01T00:00:00Z	ru_RU
dc.date.issued	2020	ru_RU
dc.identifier.citation	Yu. G. Ignat'ev and D. Yu. Ignatyev. A Complete Model of Cosmological Evolution of a Scalar Field with Higgs Potential and Euclidean Cycles // Gravitation and Cosmology, 2020, Vol. 26, No. 1, pp. 29–37.	ru_RU
dc.identifier.uri	https://repository.kpfu.ru/eng/?p_id=218916&p_lang=2	ru_RU
dc.description.abstract	Gravitation and Cosmology	ru_RU
dc.description.abstract	A revision of the author's results concerning the possible existence of the so-called Euclidean cycles in cosmological evolution of a system of Higgs scalar fields is being performed. The assumption of a nonnegative velocity of the Universe expansion, which in certain cases contradicts the complete set of the Einstein equations, is removed. It is shown that in the cases where the effective energy of the system tends to zero, happens a smooth transition of the model to the range of negative values of the expansion rate, i.e., there is a transition to a collapsing stage rather than winding of the phase trajectories on the boundary of prohibited area. This process is studied with the help of numerical simulation methods for a model based on a classical scalar Higgs field.	ru_RU
dc.language.iso	ru	ru_RU
dc.subject	Higgs fields	ru_RU
dc.subject	cosmology	ru_RU
dc.subject	quality analysis	ru_RU
dc.subject	numerical modelling	ru_RU
dc.title	A Complete Model of Cosmological Evolution of a Scalar Field with Higgs Potential and Euclidean Cycles	ru_RU
dc.type	Articles in international journals and collections	ru_RU