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.
Modeling hf-qpos in microquasars and agns: charged particles around black holes with cdm halos
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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.