Energetics of turbulence generated by chiral MHD dynamos

DOI10.1080/03091929.2018.1515313zbMath1499.86019arXiv1803.06350OpenAlexW3102497069WikidataQ114640086 ScholiaQ114640086MaRDI QIDQ5063545

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Publication date: 21 March 2022

Published in: Geophysical & Astrophysical Fluid Dynamics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1803.06350

zbMATH Keywords

turbulenceearly universechiral MHD dynamosrelativistic magnetohydrodynamics (MHD)

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Galactic and stellar dynamics (85A05) Geo-electricity and geomagnetism (86A25)

Related Items

Baryogenesis from axion inflation, Scale-invariant helical magnetic fields from inflation, Chiral gravitational waves produced in a helical magnetogenesis model

Cites Work

• Hydromagnetic turbulence in computer simulations
• Low-storage Runge-Kutta schemes
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