Approximate Metric for a Rotating Deformed Mass

@article{FrutosAlfaro2015ApproximateMF,
  title={Approximate Metric for a Rotating Deformed Mass},
  author={F. Frutos-Alfaro and Paulo Montero-Camacho and Miguel Araya-Arguedas and Javier Bonatti-Gonz'alez},
  journal={International Journal of Astronomy and Astrophysics},
  year={2015},
  volume={5},
  pages={1-10}
}
  • F. Frutos-Alfaro, Paulo Montero-Camacho, +1 author Javier Bonatti-Gonz'alez
  • Published 2015
  • Physics
  • International Journal of Astronomy and Astrophysics
  • A new Kerr-like metric with quadrupole moment is obtained by means of perturbing the Kerr spacetime. The form of this new metric is simple as the Kerr metric. By comparison with the exterior Hartle-Thorne metric, it is shown that it could be matched to an interior solution. This approximate metric may represent the spacetime of a real astrophysical object with any Kerr rotation parameter a and slightly deformed. 
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