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.
Perturbing the stable accretion disk in kerr and 4d einstein–gauss–bonnet gravities: Comprehensive analysis of instabilities and dynamics
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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.