• Corpus ID: 119205805

Generalized Newtonian description of particle motion in spherically symmetric spacetimes

@article{Tejeda2014GeneralizedND,
  title={Generalized Newtonian description of particle motion in spherically symmetric spacetimes},
  author={Emilio Tejeda and Stephan Rosswog},
  journal={arXiv: General Relativity and Quantum Cosmology},
  year={2014}
}

• E. Tejeda, S. Rosswog
• Published 5 February 2014
• Physics
• arXiv: General Relativity and Quantum Cosmology

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-Nordstr\"om, Ay\'on Beato-Garc\'ia, 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.