Collaborative Research: Multidimensional Kinetic Simulations of Particle Acceleration in Astrophysical Collisionless Shocks
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Collisionless shocks are ubiquitous in space and astrophysical plasmas: they dissipate kinetic energy into heat, produce energetic particles, and generate magnetic turbulence. Shock-accelerated particles are key for the non-thermal emission (from radio to gamma-ray bands to high-energy neutrinos) observed in many astrophysical objects and events,…
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