http://arxiv.org/abs/2112.01415
We compare some predictions of Wagoner & Tandon (2021) with the results of the hydrodynamic and magnetohydrodynamic (MHD) simulations of Reynolds & Miller (2009). 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).
R. Wagoner and C. Tandon
Fri, 3 Dec 21
8/81
Comments: 2 pages
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