Spinning charged test particles around a Schwarzschild black hole in a uniform magnetic field have integrable equatorial motion with explicit frequencies but exhibit chaotic non-integrable dynamics off the equatorial plane.
Therein, we expect a regular trajectory to display a closed curve with epicyclic oscillations superposed due to the coupling between the radial and spin DoF
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Spinning charged test particle dynamics around a Schwarzschild black hole embedded in a homogeneous magnetic field
Spinning charged test particles around a Schwarzschild black hole in a uniform magnetic field have integrable equatorial motion with explicit frequencies but exhibit chaotic non-integrable dynamics off the equatorial plane.