Magnetized Kerr spacetime admits a critical magnetic field beyond which no circular timelike or null geodesics exist, and subcritical fields induce periastron precession reversal within a finite radial range.
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Orbital dynamics and precession in magnetized Kerr spacetime
Magnetized Kerr spacetime admits a critical magnetic field beyond which no circular timelike or null geodesics exist, and subcritical fields induce periastron precession reversal within a finite radial range.