Monte Carlo radiation transport through a chain of trans-relativistic plasmoids reproduces the 100 keV cutoff and predicts strong perpendicular polarization above 1 keV due to planar confinement of plasmoid motion.
harvard.edu/abs/1978MNRAS.182..147B/abstract Beloborodov, A
6 Pith papers cite this work. Polarity classification is still indexing.
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A population of AGN coronae with magnetization parameters spanning up to σ ~ 10 can reproduce the entire observed diffuse neutrino flux from TeV to PeV energies.
Derives and validates via PIC simulations a scaling law for nonthermal spectral tails in mildly to strongly magnetized turbulent plasmas, with application to black-hole coronae.
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