Derives causal second-order relativistic MHD equations from kinetic theory for non-resistive and resistive two-component plasmas, predicting cyclotron-related oscillations in Bjorken flow.
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Holographic calculation in a spinning Myers-Perry black brane shows that higher temperature or rotation parameter a shortens light-quark stopping distance and increases instantaneous energy loss, with stronger anisotropy for transverse motion.
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Relativistic magnetohydrodynamics from kinetic theory
Derives causal second-order relativistic MHD equations from kinetic theory for non-resistive and resistive two-component plasmas, predicting cyclotron-related oscillations in Bjorken flow.
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Holographic light-quark energy loss in a spinning plasma
Holographic calculation in a spinning Myers-Perry black brane shows that higher temperature or rotation parameter a shortens light-quark stopping distance and increases instantaneous energy loss, with stronger anisotropy for transverse motion.