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• W4220786075 abstract "Magnetic energy around astrophysical compact objects can strongly dominate over plasma rest mass. Emission observed from these systems may be fed by dissipation of Alfvén wave turbulence, which cascades to small damping scales, energizing the plasma. We use 3D kinetic simulations to investigate this process. When the cascade is excited naturally, by colliding large-scale Alfvén waves, we observe quasithermal heating with no nonthermal particle acceleration. We also find that the particles are energized along the magnetic field lines and so are poor producers of synchrotron radiation. At low plasma densities, our simulations show the transition to charge-starved cascades, with a distinct damping mechanism." @default.
• W4220786075 created "2022-04-03" @default.
• W4220786075 creator A5002440723 @default.
• W4220786075 creator A5062917864 @default.
• W4220786075 date "2022-02-14" @default.
• W4220786075 modified "2023-10-14" @default.
• W4220786075 title "Heating of Magnetically Dominated Plasma by Alfvén-Wave Turbulence" @default.
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• W4220786075 doi "https://doi.org/10.1103/physrevlett.128.075101" @default.
• W4220786075 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/35244444" @default.
• W4220786075 hasPublicationYear "2022" @default.
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