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This repository contains data for the h1 an dr0/h1 perturbations that can be used to compute a piece of the source for the second-order metric perturbation. The Mathematica notebook 'SecondOrderE1h1.nb' shows how to combine the data to compute E1[h1]. The h1 data was computed using the h1Lorenz code that is available in the Black Hole Perturbation Toolkit (https://github.com/BlackHolePerturbationToolkit/h1Lorenz). The dr0/dh1 data was computed by Leanne Durkan following the method detailed in "Slow evolution of the metric perturbation due to a quasicircular inspiral into a Schwarzschild black hole" by Leanne Durkan and Niels Warburton, arXiv:2206.08179 Authors: Leanne Durkan, Niels Warburton
{"references": ["Slow evolution of the metric perturbation due to a quasicircular inspiral into a Schwarzschild black hole, Leanne Durkan and Niels Warburton,Phys. Rev. D 106, 084023 (2022), arXiv:2206.08179"]}
gravitational waves, metric perturbations, second-order in the mass ratio, extreme and intermediate mass ratio inspirals
gravitational waves, metric perturbations, second-order in the mass ratio, extreme and intermediate mass ratio inspirals
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