Effective Viscosity in the Intracluster Medium During Magnetic Field Amplification via Turbulent Dynamo

Galaxy clusters, the largest gravitationally bound structures, host a hot, diffuse plasma with poorly understood viscosity and magnetic field amplification. Astrophysical plasmas are often modeled with magnetohydrodynamics (MHD), but low collision rates in environments such as the intracluster mediu...

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Detalhes bibliográficos

Principais autores:	S. Adduci Faria, R. Santos-Lima, E. M. de Gouveia Dal Pino
Formato:	Artigo
Idioma:	Inglês
Publicado em:	IOP Publishing 2025-01-01
Colecção:	The Astrophysical Journal
Assuntos:	Magnetic fields Intracluster medium Plasma astrophysics Magnetohydrodynamical simulations Galaxy clusters
Acesso em linha:	https://doi.org/10.3847/1538-4357/addc5f
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