First relativistic MHD turbulence simulations with self-consistent synchrotron cooling find a cooling-driven two-phase plasma and frequency-dependent polarization and Faraday-rotation variability resembling high-energy source observations.
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Synchrotron-Regulated Relativistic Magnetohydrodynamic Turbulence: Emission, Polarization, and Faraday Rotation
First relativistic MHD turbulence simulations with self-consistent synchrotron cooling find a cooling-driven two-phase plasma and frequency-dependent polarization and Faraday-rotation variability resembling high-energy source observations.