Nearby geodesics, spinning particles, magnetically charged particles and string probes all deviate from geodesic motion in a topological star, reducing to Schwarzschild plus small alpha-dependent corrections.
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Characterizing geodesic deviations in a Topological Star spacetime: massive, charged, spinning and stringy-like objects
Nearby geodesics, spinning particles, magnetically charged particles and string probes all deviate from geodesic motion in a topological star, reducing to Schwarzschild plus small alpha-dependent corrections.