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The qual- itative behavior of the trajectories is determined by the structure of the radial roots of the equation E2 −V 2(r) = 0,(68) which fixes the turning points

Critical trajectories whithE <1 Using the angular geodesic equation (25), the orbital motion can be expressed in integral form φ(r) =± Z r R0 L dr′ R(r′)2 p E2 −V 2(r′) ,(67) where

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Time Like Geodesics of Regular Black Holes with Scalar Hair

gr-qc · 2026-04-22 · unverdicted · novelty 3.0

Timelike geodesics around asymptotically flat regular black holes with phantom scalar hair show shifted circular orbits, ISCO locations, and perihelion precession corrections proportional to the scalar charge A that can be constrained by Solar System observations.

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  • Time Like Geodesics of Regular Black Holes with Scalar Hair gr-qc · 2026-04-22 · unverdicted · none · ref 10

    Timelike geodesics around asymptotically flat regular black holes with phantom scalar hair show shifted circular orbits, ISCO locations, and perihelion precession corrections proportional to the scalar charge A that can be constrained by Solar System observations.