Turbulence-mediated reconnection dominates over plasmoid-mediated reconnection in AGN accretion flows, driving faster reconnection and flares at rates ~0.1 V_A.
E., et al.Particle acceleration by relativistic magnetic reconnection driven by kink instability turbulence in Poyntingflux–dominated jets
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Is plasmoid-mediated reconnection really important in accretion flows to drive flares in AGNs?
Turbulence-mediated reconnection dominates over plasmoid-mediated reconnection in AGN accretion flows, driving faster reconnection and flares at rates ~0.1 V_A.