Perturbed stellar motions around the rotating black hole in Sgr A * for a generic orientation of its spin axis

@article{Iorio2011PerturbedSM,
  title={Perturbed stellar motions around the rotating black hole in Sgr A * for a generic orientation of its spin axis},
  author={Lorenzo Iorio},
  journal={Physical Review D},
  year={2011},
  volume={84},
  pages={124001}
}
  • L. Iorio
  • Published 14 July 2011
  • Physics
  • Physical Review D
Empirically determining the averaged variations of the orbital parameters of the stars orbiting the Supermassive Black Hole (SBH) hosted by the Galactic center (GC) in Sgr ${\mathrm{A}}^{*}$ is, in principle, a valuable tool to test the General Theory of Relativity (GTR), in regimes far stronger than those tested so far, and certain key predictions of it like the ``no-hair'' theorems. We analytically work out the long-term variations of all the six osculating Keplerian orbital elements of a… 

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