Why Have the Observed High-frequency QPOs Not Been Produced by (MHD) Computer Simulations of Black Hole Accretion Disks?
Robert V. WagonerDept. of Physics and KIPAC, Stanford University, USA; [email protected]Celia R. TandonDept. of Physics and KIPAC, Stanford University, USA; [email protected]
2021en
ABI
Аннотация
Abstract We compare some predictions of Wagoner & Tandon (WT) with the results of the hydrodynamic and magnetohydrodynamic (MHD) simulations of Reynolds & Miller (RM). It appears that the MHD simulations were not run for long enough and the numerical damping was not small enough to produce the observed high-frequency QPOs (and the g-mode seen in the hydro simulations).
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