Evolution of a Large Scale Chern–Simons Magnetic Field in Expanding Space with a Negative Scalar Curvature Parameter

We study the problem of breaking non-Abelian gauge symmetry for solving the Yang–Mills equation in an expanding space with a parameter of negative scalar curvature, which becomes flat at large expansion times and which is called the geodesic flow space of the Lobachevsky plane. We use the following: the physical properties of the magnetic field are related to the Kolmogorov scale, which made it possible to estimate the α-effect of the space curvature parameter at each moment of time. On the other hand, in an expanding hyperbolic space, a change in the density of magnetic helicity is observed, unrelated to the α-effect. We compare the two indicated factors of change in magnetic helicity and conclude that, at a fairly stable stage of expansion, the α-effect caused by the influence of scalar curvature on the Kolmogorov MHD spectrum becomes small.

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Publication Details

Journal
Physics of Particles and Nuclei
Published
2025-04-01
DOI
https://doi.org/10.1134/s106377962470151x
Citations
2
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
3.74
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article

Evolution of a Large Scale Chern–Simons Magnetic Field in Expanding Space with a Negative Scalar Curvature Parameter

Maxim Dvornikov, Peter M. Akhmetiev
2 citations
Physics of Particles and Nuclei
Black Holes and Theoretical Physics
3.74
article

Evolution of a Large Scale Chern–Simons Magnetic Field in Expanding Space with a Negative Scalar Curvature Parameter

Maxim Dvornikov, Peter M. Akhmetiev
article en
2 citations

Abstract

We study the problem of breaking non-Abelian gauge symmetry for solving the Yang–Mills equation in an expanding space with a parameter of negative scalar curvature, which becomes flat at large expansion times and which is called the geodesic flow space of the Lobachevsky plane. We use the following: the physical properties of the magnetic field are related to the Kolmogorov scale, which made it possible to estimate the α-effect of the space curvature parameter at each moment of time. On the other hand, in an expanding hyperbolic space, a change in the density of magnetic helicity is observed, unrelated to the α-effect. We compare the two indicated factors of change in magnetic helicity and conclude that, at a fairly stable stage of expansion, the α-effect caused by the influence of scalar curvature on the Kolmogorov MHD spectrum becomes small.

Physics of Particles and NucleiVol. 56(2)
Joint Institute for Nuclear Research (RU), Institute of Terrestrial Magnetism Ionosphere and Radio Wave Propagation (RU)
Openalex Percentile: Top 8%
Black Holes and Theoretical Physics
3.74
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