The paper derives Bayesian constraints on magnetic field strength and dipole coupling in magnetized Schwarzschild black holes by fitting QPO frequencies from stellar-mass to supermassive systems within the relativistic precession model.
Mass of intermediate black hole in the source m82 x-1 restricted by models of twin high-frequency quasi-periodic oscillations
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QPO-Based Bayesian Constraints on Charged Particle Dynamics Around Magnetized Schwarzschild Black Holes
The paper derives Bayesian constraints on magnetic field strength and dipole coupling in magnetized Schwarzschild black holes by fitting QPO frequencies from stellar-mass to supermassive systems within the relativistic precession model.