PIC simulations of oblique shocks in turbulent plasma show that pre-existing 15% compressive turbulence produces a shorter hotter foreshock and more numerous higher-energy non-thermal electrons.
Monthly Notices of the Royal Astronomical Society , volume =
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Jet and wind feedback from AGN couple nonlinearly through Kelvin-Helmholtz instability, raising energy dissipation efficiency to 0.64 and dropping star formation rate to 10^{-3} solar masses per year.
citing papers explorer
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PIC simulations of nonrelativistic high-Mach-number oblique shocks propagating in a turbulent medium
PIC simulations of oblique shocks in turbulent plasma show that pre-existing 15% compressive turbulence produces a shorter hotter foreshock and more numerous higher-energy non-thermal electrons.
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The MeerKAT Massive Distant Clusters Survey: a search for diffuse radio emission in 30 massive SZ-selected clusters at $z > 1$
MeerKAT observations detect radio halos in 27% of 30 massive clusters at z>1, a rate lower than at intermediate redshifts but above model predictions, with power-mass scaling similar to lower-z samples.
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Active Galactic Nucleus Feedback in an Elliptical Galaxy. IV. The Importance of the Jet Wind Coupling
Jet and wind feedback from AGN couple nonlinearly through Kelvin-Helmholtz instability, raising energy dissipation efficiency to 0.64 and dropping star formation rate to 10^{-3} solar masses per year.