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Main Authors: Buchman, Luisa T., Duez, Matthew D., Morales, Marlo, Scheel, Mark A., Kostersitz, Tim M., Evans, Andrew M., Mitman, Keefe
Format: Preprint
Published: 2024
Subjects:
Online Access:https://arxiv.org/abs/2402.12544
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author Buchman, Luisa T.
Duez, Matthew D.
Morales, Marlo
Scheel, Mark A.
Kostersitz, Tim M.
Evans, Andrew M.
Mitman, Keefe
author_facet Buchman, Luisa T.
Duez, Matthew D.
Morales, Marlo
Scheel, Mark A.
Kostersitz, Tim M.
Evans, Andrew M.
Mitman, Keefe
contents Errors due to imperfect boundary conditions in numerical relativity simulations of binary black holes can produce unphysical reflections of gravitational waves which compromise the accuracy of waveform predictions, especially for subdominant modes. A system of higher order absorbing boundary conditions which greatly reduces this problem was introduced in earlier work [arXiv:gr-qc/0608051]. In this paper, we devise two new implementations of this boundary condition system in the Spectral Einstein Code (SpEC), and test them in both linear multipolar gravitational wave and inspiralling mass ratio 7:1 binary black hole simulations. One of our implementations in particular is shown to be extremely robust and to produce accuracy superior to the standard freezing-Psi_0 boundary condition usually used by SpEC.
format Preprint
id arxiv_https___arxiv_org_abs_2402_12544
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Numerical Relativity Multimodal Waveforms using Absorbing Boundary Conditions
Buchman, Luisa T.
Duez, Matthew D.
Morales, Marlo
Scheel, Mark A.
Kostersitz, Tim M.
Evans, Andrew M.
Mitman, Keefe
General Relativity and Quantum Cosmology
Errors due to imperfect boundary conditions in numerical relativity simulations of binary black holes can produce unphysical reflections of gravitational waves which compromise the accuracy of waveform predictions, especially for subdominant modes. A system of higher order absorbing boundary conditions which greatly reduces this problem was introduced in earlier work [arXiv:gr-qc/0608051]. In this paper, we devise two new implementations of this boundary condition system in the Spectral Einstein Code (SpEC), and test them in both linear multipolar gravitational wave and inspiralling mass ratio 7:1 binary black hole simulations. One of our implementations in particular is shown to be extremely robust and to produce accuracy superior to the standard freezing-Psi_0 boundary condition usually used by SpEC.
title Numerical Relativity Multimodal Waveforms using Absorbing Boundary Conditions
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2402.12544