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.
In this limit, the magnetization functions reduce to unity, Λ e = Λ0 = 1, andA e = (r2 +a 2)2 −a 2∆
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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.