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.
Curled orbit and epicyclic oscillation of charged particles around the weakly magnetized black hole in the presence of lorentz violation
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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.