Dynamo Effect and Turbulence in Hydrodynamic Weyl Metals
Victor Galitski, Mehdi Kargarian, Sergey Syzranov

TL;DR
This paper explores the potential for observing the dynamo effect in hydrodynamic Weyl semimetals, deriving relevant equations, estimating key parameters, and showing how the chiral anomaly influences dynamo thresholds.
Contribution
It introduces a theoretical framework for realizing the dynamo effect in solid-state Weyl semimetals, expanding experimental possibilities beyond traditional fluids.
Findings
Hydrodynamic Weyl semimetals can achieve large magnetic Reynolds numbers.
The chiral anomaly reduces the threshold for dynamo instability.
Derived magneto-hydrodynamic equations for Weyl electron-hole plasma.
Abstract
The dynamo effect is a class of macroscopic phenomena responsible for generation and maintaining magnetic fields in astrophysical bodies. It hinges on hydrodynamic three-dimensional motion of conducting gases and plasmas that achieve high hydrodynamic and/or magnetic Reynolds numbers due to large length scales involved. The existing laboratory experiments modeling dynamos are challenging and involve large apparatuses containing conducting fluids subject to fast helical flows. Here we propose that electronic solid-state materials -- in particular, hydrodynamic metals -- may serve as an alternative platform to observe some aspects of the dynamo effect. Motivated by recent experimental developments, this paper focuses on hydrodynamic Weyl semimetals, where the dominant scattering mechanism is due to interactions. We derive Navier-Stokes equations along with equations of…
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