In adiabatically stratified cluster gas the MTI saturates via large plumes destroyed by shear, producing turbulent kinetic energy that scales as χ ω_T.
and Scepi, Nicolas and Dexter, Jason , year =
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Pairing square-root-area-weighted vacuum perturbations with full-area-weighted resonant fields produces a coupling matrix whose singular values and reconstructed real-space patterns are invariant to coordinate choice.
Simulations of accreting black holes in standard and complex spacetimes indicate that magnetic geometry, quantum corrections, and binary dynamics influence flares, precession, photon rings, and multi-wavelength variability, with potential EHT constraints.
Radio precedes X-ray Compton luminosity by ~3 days in the rising hard state but lags by ~8 days in the decaying hard state of GX 339-4, with inner magnetic field strength estimated from accretion rate and truncation radius accounting for both.
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Coordinate-invariant flux-surface Fourier analysis in tokamaks
Pairing square-root-area-weighted vacuum perturbations with full-area-weighted resonant fields produces a coupling matrix whose singular values and reconstructed real-space patterns are invariant to coordinate choice.