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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Turbulent electron-ion coronae around accreting black holes self-regulate into a two-temperature state that generates nonthermal ions and X-ray spectra consistent with observations including an MeV tail.
Pair production via radiative magnetic reconnection near spinning black holes supplies non-uniform plasma to jets at levels sufficient to explain M87 radio emission.
A new observable signature from frame-dragging processes near spinning black holes enables testing Einstein gravity and spin measurement via X-ray polarimetry.
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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On The Nonthermal Power Laws In Magnetized Turbulent Plasmas
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.