Simulations show that the maximum radial epicyclic frequency acts as a proxy for observed QPO frequencies in supermassive black hole accretion, matching data when scaled by black hole mass.
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Radiation hydrodynamic simulations for the origin of quasi-periodic oscillations for accretion onto supermassive black holes
Simulations show that the maximum radial epicyclic frequency acts as a proxy for observed QPO frequencies in supermassive black hole accretion, matching data when scaled by black hole mass.