Black hole perturbation theory and gravitational self-force

@inproceedings{Pound2021BlackHP,
  title={Black hole perturbation theory and gravitational self-force},
  author={Adam Pound and Barry Wardell},
  year={2021}
}
Much of the success of gravitational-wave astronomy rests on perturbation theory. Historically, perturbative analysis of gravitational-wave sources has largely focused on post-Newtonian theory. However, strong-field perturbation theory is essential in many cases such as the quasinormal ringdown following the merger of a binary system, tidally perturbed compact objects, and extreme-mass-ratio inspirals. In this review, motivated primarily by small-mass-ratio binaries but not limited to them, we… 

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