Turbulence-mediated reconnection dominates over plasmoid-mediated reconnection in AGN accretion flows, driving faster reconnection and flares at rates ~0.1 V_A.
N.Characterizing Power Spectra of Density Fluctuations in GRMHD Simulations of Black Hole Accretion Using Taylor’s Frozen- in Hypothesis(2025) arXiv:2510.09746 [astro-ph.HE]
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.HE 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
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.