Oscillating standing shocks in low-angular-momentum relativistic accretion flows produce 0.1-10 Hz luminosity oscillations for stellar-mass black holes and 10^-6 to 10^-5 Hz oscillations for Sgr A*, matching observed X-ray variability.
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Relativistic Low Angular Momentum Advective Flows onto Black Hole and associated observational signatures
Oscillating standing shocks in low-angular-momentum relativistic accretion flows produce 0.1-10 Hz luminosity oscillations for stellar-mass black holes and 10^-6 to 10^-5 Hz oscillations for Sgr A*, matching observed X-ray variability.