Simulations with mass ratio 100 show Weibel instability generating magnetic seeds that undergo dynamo amplification, with the electron heat-flux closure controlling the shift between kinetic and fluid-like regimes.
& Kamionkowski, Marc2006 Cluster magnetic fields from large-scale structure and galaxy cluster shocks.The Astrophysical Journal 642(1), L1
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From Weibel seeds to collisionless dynamos beyond pair-plasmas
Simulations with mass ratio 100 show Weibel instability generating magnetic seeds that undergo dynamo amplification, with the electron heat-flux closure controlling the shift between kinetic and fluid-like regimes.