New comprehensive description of the scaling evolution of the cosmological magneto-hydrodynamic system
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| Main Authors: | , , , |
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| Format: | Preprint |
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2024
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| _version_ | 1866912521733013504 |
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| author | Uchida, Fumio Fujiwara, Motoko Kamada, Kohei Yokoyama, Jun'ichi |
| author_facet | Uchida, Fumio Fujiwara, Motoko Kamada, Kohei Yokoyama, Jun'ichi |
| contents | We study the evolution of primordial magnetic fields until the recombination epoch, which is constrained by the conservation of magnetic helicity density if they are maximally helical and by the Hosking integral if they are non-helical. We combine these constraints with conditions obtained by estimating time scales of energy dissipation processes to describe the evolution of magnetic field strength and magnetic coherence length analytically. The dissipation processes depend on whether magnetic or kinetic energy is dominant, whether the decay dynamics is linear or not, and whether the dominant dissipation term is shear viscosity or drag force. We apply the description to compare constraints on primordial magnetic fields at different epochs in the early universe and argue that magnetogenesis before the electroweak symmetry breaking is not feasible. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2405_06194 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | New comprehensive description of the scaling evolution of the cosmological magneto-hydrodynamic system Uchida, Fumio Fujiwara, Motoko Kamada, Kohei Yokoyama, Jun'ichi Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology Fluid Dynamics We study the evolution of primordial magnetic fields until the recombination epoch, which is constrained by the conservation of magnetic helicity density if they are maximally helical and by the Hosking integral if they are non-helical. We combine these constraints with conditions obtained by estimating time scales of energy dissipation processes to describe the evolution of magnetic field strength and magnetic coherence length analytically. The dissipation processes depend on whether magnetic or kinetic energy is dominant, whether the decay dynamics is linear or not, and whether the dominant dissipation term is shear viscosity or drag force. We apply the description to compare constraints on primordial magnetic fields at different epochs in the early universe and argue that magnetogenesis before the electroweak symmetry breaking is not feasible. |
| title | New comprehensive description of the scaling evolution of the cosmological magneto-hydrodynamic system |
| topic | Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology Fluid Dynamics |
| url | https://arxiv.org/abs/2405.06194 |