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Generalized Newtonian description of particle motion in spherically symmetric spacetimes

We present a generalized Newtonian description of particle dynamics valid for any spherically symmetric, static black hole spacetime. This approach is derived from the geodesic motion of test particles in the low-energy limit. It reproduces exactly the location of the marginally stable, marginally bound, and photon circular orbits; the radial dependence of the energy and angular momentum of circular orbits; parabolic motion; pericentre shift; and the spatial projection of general trajectories. As explicit examples of the new prescription, we apply it to the Schwarzschild, Schwarzschild-de Sitter, Reissner-Nordström, Ayón Beato-García, and Kehagias-Sfetsos spacetimes. In all of these examples, the orbital and epicyclic frequencies are reproduced to better than 10%. The resulting equations of motion can be implemented easily and efficiently within existing Newtonian frameworks.