Published October 4, 2023
| Version v1
Dataset
Open
Example calculation of E1[h1] contribution to the source for second-order metric perturbations of a Schwarzschild black hole
Authors/Creators
- 1. Center for Gravitational Physics, University of Texas at Austin, Austin, TX 78712, USA.
- 2. School of Mathematics and Statistics, University College Dublin, Belfield, Dublin 4, Ireland
Description
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
Files
SecondOrderE1h1.zip
Files
(40.9 MB)
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Additional details
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