Resonance Broadening and Heating of Charged Particles in Magnetohydrodynamic Turbulence

The heating, acceleration, and pitch-angle scattering of charged particles by MHD turbulence are important in a wide range of astrophysical environments, including the solar wind, accreting black holes, and galaxy clusters. We simulate the interaction of high-gyrofrequency test particles with fully...

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Veröffentlicht in:	arXiv.org 2012-09
Hauptverfasser:	Lynn, Jacob W, Parrish, Ian J, Quataert, Eliot, Chandran, Benjamin D G
Format:	Artikel
Sprache:	eng
Schlagworte:	Acceleration Beads Black holes Charged particles Damping Deposition Diffusion rate Distribution functions Fluid dynamics Fluid flow Galactic clusters Galaxies Gyrofrequency Heating Magnetohydrodynamic turbulence Mathematical analysis Particle physics Physics - Solar and Stellar Astrophysics Simulation Solar wind Velocity
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