Macarena Lagos

The modeling of gravitational wave ringdown has traditionally relied on linear perturbation theory, which mainly describes the late-time behavior of a perturbed black hole after a binary merger. However, the need for more accurate ringdown models has motivated the understanding of nonlinear gravitational effects. In this paper, we summarize the main properties and latest developments of quadratic effects in ringdown models, which are expected to be detectable with next-generation gravitational wave detectors, and will allow for new consistency tests of general relativity.