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.
Caprioli \ and\ author A
4 Pith papers cite this work. Polarity classification is still indexing.
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2026 4verdicts
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A one-zone model fitted to radio observations of WR 102's bubble predicts that protons accelerated at the wind shock dominate high-energy emission but produce an undetectable gamma-ray flux.
Hybrid simulations of the ion Weibel instability require a minimum grid resolution that scales with Alfvénic Mach number to correctly reproduce magnetic-field growth and saturation without introducing unphysical whistler modes.
This review summarizes the basic principles of electron transport in inhomogeneous and tangled magnetic fields through gyro-centre trajectories, kinetic instabilities, trapping, and diffusion processes.
citing papers explorer
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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.
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High-energy Processes in the Bubbles of Wolf-Rayet Stars: The case of WR 102
A one-zone model fitted to radio observations of WR 102's bubble predicts that protons accelerated at the wind shock dominate high-energy emission but produce an undetectable gamma-ray flux.
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Ion Weibel Instability in the hybrid framework: the optimal resolution
Hybrid simulations of the ion Weibel instability require a minimum grid resolution that scales with Alfvénic Mach number to correctly reproduce magnetic-field growth and saturation without introducing unphysical whistler modes.
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Transport of electrons in tangled magnetic fields
This review summarizes the basic principles of electron transport in inhomogeneous and tangled magnetic fields through gyro-centre trajectories, kinetic instabilities, trapping, and diffusion processes.