Turbulent Dynamo as Spontaneous Symmetry Breaking: α-Effect
This paper focuses on advancements in understanding the processes of magnetic field transport in the regime of fully developed stationary magnetohydrodynamic (MHD) chiral turbulence, utilizing the methods of statistical field theory. Within the framework of a model describing homogeneous and isotropic turbulence in the inertial range, an estimation of the transport coefficient α (the so-called α-effect) is provided.
Authors
- T. Lučivjanský (ORCID: https://orcid.org/0000-0001-8529-4893)
- Yu. G. Molotkov
- Michal Hnatič (ORCID: https://orcid.org/0000-0003-0051-3036)
- L. Mižišin (ORCID: https://orcid.org/0000-0002-3758-5837)
- A. Ovsiannikov
Institutions
- University of Pavol Jozef Šafárik (SK)
- Slovak Academy of Sciences (SK)
- Joint Institute for Nuclear Research (RU)
- Institute of Experimental Physics of the Slovak Academy of Sciences (SK)
- Institute of Physics of the Slovak Academy of Sciences (SK)
Publication Details
- Journal
- Physics of Particles and Nuclei
- Published
- 2025-10-25
- DOI
- https://doi.org/10.1134/s1063779625700698
- Primary Topic
- Geomagnetism and Paleomagnetism Studies
- Type
- article
- Field-Weighted Citation Impact
- 0.00