Loading…

Fully relativistic three-dimensional Cauchy-characteristic matching for physical degrees of freedom

A fully relativistic three-dimensional Cauchy-characteristic matching (CCM) algorithm is implemented for physical degrees of freedom in a numerical relativity code SpECTRE. The method is free of approximations and can be applied to any physical system. We test the algorithm with various scenarios in...

Full description

Saved in:
Bibliographic Details
Published in:arXiv.org 2024-06
Main Authors: Ma, Sizheng, Moxon, Jordan, Scheel, Mark A, Nelli, Kyle C, Deppe, Nils, Bonilla, Marceline S, Kidder, Lawrence E, Kumar, Prayush, Lovelace, Geoffrey, Throwe, William, Vu, Nils L
Format: Article
Language:English
Subjects:
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by
cites
container_end_page
container_issue
container_start_page
container_title arXiv.org
container_volume
creator Ma, Sizheng
Moxon, Jordan
Scheel, Mark A
Nelli, Kyle C
Deppe, Nils
Bonilla, Marceline S
Kidder, Lawrence E
Kumar, Prayush
Lovelace, Geoffrey
Throwe, William
Vu, Nils L
description A fully relativistic three-dimensional Cauchy-characteristic matching (CCM) algorithm is implemented for physical degrees of freedom in a numerical relativity code SpECTRE. The method is free of approximations and can be applied to any physical system. We test the algorithm with various scenarios involving smooth data, including the propagation of Teukolsky waves within a flat background, the perturbation of a Kerr black hole with a Teukolsky wave, and the injection of a gravitational-wave pulse from the characteristic grid. Our investigations reveal no numerical instabilities in the simulations. In addition, the tests indicate that the CCM algorithm effectively directs characteristic information into the inner Cauchy system, yielding higher precision in waveforms and smaller violations of Bondi-gauge constraints, especially when the outer boundary of the Cauchy evolution is at a smaller radius.
doi_str_mv 10.48550/arxiv.2308.10361
format article
fullrecord <record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_journals_2854680176</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2854680176</sourcerecordid><originalsourceid>FETCH-LOGICAL-a526-dc0a60e742ae116102bc3da660e62edc5691305d6cab6adf47b242cad380eab33</originalsourceid><addsrcrecordid>eNotjsFqwzAQREWh0JDmA3oT9Ox0tbJk91hM0xYCveQe1pIcK9hWKtmh_vsa0tMMw5thGHsSsM1LpeCF4q-_blFCuRUgtbhjK5RSZGWO-MA2KZ0BAHWBSskVM7up62YeXUejv_o0esPHNjqXWd-7IfkwUMcrmkw7Z6alSGZ08cb1NJrWDyfehMgv7Zy8WVjrTks98dDwZjE29I_svqEuuc2_rtlh936oPrP998dX9bbPSKHOrAHS4IocyQmhBWBtpCW9ZBqdNUq_CgnKakO1JtvkRY05GrKyBEe1lGv2fJu9xPAzuTQez2GKy_10xFLlugRRaPkHTT1ZOg</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2854680176</pqid></control><display><type>article</type><title>Fully relativistic three-dimensional Cauchy-characteristic matching for physical degrees of freedom</title><source>Publicly Available Content Database</source><creator>Ma, Sizheng ; Moxon, Jordan ; Scheel, Mark A ; Nelli, Kyle C ; Deppe, Nils ; Bonilla, Marceline S ; Kidder, Lawrence E ; Kumar, Prayush ; Lovelace, Geoffrey ; Throwe, William ; Vu, Nils L</creator><creatorcontrib>Ma, Sizheng ; Moxon, Jordan ; Scheel, Mark A ; Nelli, Kyle C ; Deppe, Nils ; Bonilla, Marceline S ; Kidder, Lawrence E ; Kumar, Prayush ; Lovelace, Geoffrey ; Throwe, William ; Vu, Nils L</creatorcontrib><description>A fully relativistic three-dimensional Cauchy-characteristic matching (CCM) algorithm is implemented for physical degrees of freedom in a numerical relativity code SpECTRE. The method is free of approximations and can be applied to any physical system. We test the algorithm with various scenarios involving smooth data, including the propagation of Teukolsky waves within a flat background, the perturbation of a Kerr black hole with a Teukolsky wave, and the injection of a gravitational-wave pulse from the characteristic grid. Our investigations reveal no numerical instabilities in the simulations. In addition, the tests indicate that the CCM algorithm effectively directs characteristic information into the inner Cauchy system, yielding higher precision in waveforms and smaller violations of Bondi-gauge constraints, especially when the outer boundary of the Cauchy evolution is at a smaller radius.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.2308.10361</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Algorithms ; Gravitational waves ; Matching ; Numerical relativity ; Perturbation ; Relativistic effects ; Relativity ; Wave propagation ; Waveforms</subject><ispartof>arXiv.org, 2024-06</ispartof><rights>2024. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.proquest.com/docview/2854680176?pq-origsite=primo$$EHTML$$P50$$Gproquest$$Hfree_for_read</linktohtml><link.rule.ids>780,784,25751,27923,37010,44588</link.rule.ids></links><search><creatorcontrib>Ma, Sizheng</creatorcontrib><creatorcontrib>Moxon, Jordan</creatorcontrib><creatorcontrib>Scheel, Mark A</creatorcontrib><creatorcontrib>Nelli, Kyle C</creatorcontrib><creatorcontrib>Deppe, Nils</creatorcontrib><creatorcontrib>Bonilla, Marceline S</creatorcontrib><creatorcontrib>Kidder, Lawrence E</creatorcontrib><creatorcontrib>Kumar, Prayush</creatorcontrib><creatorcontrib>Lovelace, Geoffrey</creatorcontrib><creatorcontrib>Throwe, William</creatorcontrib><creatorcontrib>Vu, Nils L</creatorcontrib><title>Fully relativistic three-dimensional Cauchy-characteristic matching for physical degrees of freedom</title><title>arXiv.org</title><description>A fully relativistic three-dimensional Cauchy-characteristic matching (CCM) algorithm is implemented for physical degrees of freedom in a numerical relativity code SpECTRE. The method is free of approximations and can be applied to any physical system. We test the algorithm with various scenarios involving smooth data, including the propagation of Teukolsky waves within a flat background, the perturbation of a Kerr black hole with a Teukolsky wave, and the injection of a gravitational-wave pulse from the characteristic grid. Our investigations reveal no numerical instabilities in the simulations. In addition, the tests indicate that the CCM algorithm effectively directs characteristic information into the inner Cauchy system, yielding higher precision in waveforms and smaller violations of Bondi-gauge constraints, especially when the outer boundary of the Cauchy evolution is at a smaller radius.</description><subject>Algorithms</subject><subject>Gravitational waves</subject><subject>Matching</subject><subject>Numerical relativity</subject><subject>Perturbation</subject><subject>Relativistic effects</subject><subject>Relativity</subject><subject>Wave propagation</subject><subject>Waveforms</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2024</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><recordid>eNotjsFqwzAQREWh0JDmA3oT9Ox0tbJk91hM0xYCveQe1pIcK9hWKtmh_vsa0tMMw5thGHsSsM1LpeCF4q-_blFCuRUgtbhjK5RSZGWO-MA2KZ0BAHWBSskVM7up62YeXUejv_o0esPHNjqXWd-7IfkwUMcrmkw7Z6alSGZ08cb1NJrWDyfehMgv7Zy8WVjrTks98dDwZjE29I_svqEuuc2_rtlh936oPrP998dX9bbPSKHOrAHS4IocyQmhBWBtpCW9ZBqdNUq_CgnKakO1JtvkRY05GrKyBEe1lGv2fJu9xPAzuTQez2GKy_10xFLlugRRaPkHTT1ZOg</recordid><startdate>20240611</startdate><enddate>20240611</enddate><creator>Ma, Sizheng</creator><creator>Moxon, Jordan</creator><creator>Scheel, Mark A</creator><creator>Nelli, Kyle C</creator><creator>Deppe, Nils</creator><creator>Bonilla, Marceline S</creator><creator>Kidder, Lawrence E</creator><creator>Kumar, Prayush</creator><creator>Lovelace, Geoffrey</creator><creator>Throwe, William</creator><creator>Vu, Nils L</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20240611</creationdate><title>Fully relativistic three-dimensional Cauchy-characteristic matching for physical degrees of freedom</title><author>Ma, Sizheng ; Moxon, Jordan ; Scheel, Mark A ; Nelli, Kyle C ; Deppe, Nils ; Bonilla, Marceline S ; Kidder, Lawrence E ; Kumar, Prayush ; Lovelace, Geoffrey ; Throwe, William ; Vu, Nils L</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a526-dc0a60e742ae116102bc3da660e62edc5691305d6cab6adf47b242cad380eab33</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2024</creationdate><topic>Algorithms</topic><topic>Gravitational waves</topic><topic>Matching</topic><topic>Numerical relativity</topic><topic>Perturbation</topic><topic>Relativistic effects</topic><topic>Relativity</topic><topic>Wave propagation</topic><topic>Waveforms</topic><toplevel>online_resources</toplevel><creatorcontrib>Ma, Sizheng</creatorcontrib><creatorcontrib>Moxon, Jordan</creatorcontrib><creatorcontrib>Scheel, Mark A</creatorcontrib><creatorcontrib>Nelli, Kyle C</creatorcontrib><creatorcontrib>Deppe, Nils</creatorcontrib><creatorcontrib>Bonilla, Marceline S</creatorcontrib><creatorcontrib>Kidder, Lawrence E</creatorcontrib><creatorcontrib>Kumar, Prayush</creatorcontrib><creatorcontrib>Lovelace, Geoffrey</creatorcontrib><creatorcontrib>Throwe, William</creatorcontrib><creatorcontrib>Vu, Nils L</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science &amp; Engineering Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>ProQuest Central Essentials</collection><collection>AUTh Library subscriptions: ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central</collection><collection>SciTech Premium Collection (Proquest) (PQ_SDU_P3)</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Ma, Sizheng</au><au>Moxon, Jordan</au><au>Scheel, Mark A</au><au>Nelli, Kyle C</au><au>Deppe, Nils</au><au>Bonilla, Marceline S</au><au>Kidder, Lawrence E</au><au>Kumar, Prayush</au><au>Lovelace, Geoffrey</au><au>Throwe, William</au><au>Vu, Nils L</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Fully relativistic three-dimensional Cauchy-characteristic matching for physical degrees of freedom</atitle><jtitle>arXiv.org</jtitle><date>2024-06-11</date><risdate>2024</risdate><eissn>2331-8422</eissn><abstract>A fully relativistic three-dimensional Cauchy-characteristic matching (CCM) algorithm is implemented for physical degrees of freedom in a numerical relativity code SpECTRE. The method is free of approximations and can be applied to any physical system. We test the algorithm with various scenarios involving smooth data, including the propagation of Teukolsky waves within a flat background, the perturbation of a Kerr black hole with a Teukolsky wave, and the injection of a gravitational-wave pulse from the characteristic grid. Our investigations reveal no numerical instabilities in the simulations. In addition, the tests indicate that the CCM algorithm effectively directs characteristic information into the inner Cauchy system, yielding higher precision in waveforms and smaller violations of Bondi-gauge constraints, especially when the outer boundary of the Cauchy evolution is at a smaller radius.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.2308.10361</doi><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier EISSN: 2331-8422
ispartof arXiv.org, 2024-06
issn 2331-8422
language eng
recordid cdi_proquest_journals_2854680176
source Publicly Available Content Database
subjects Algorithms
Gravitational waves
Matching
Numerical relativity
Perturbation
Relativistic effects
Relativity
Wave propagation
Waveforms
title Fully relativistic three-dimensional Cauchy-characteristic matching for physical degrees of freedom
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-09T11%3A48%3A30IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Fully%20relativistic%20three-dimensional%20Cauchy-characteristic%20matching%20for%20physical%20degrees%20of%20freedom&rft.jtitle=arXiv.org&rft.au=Ma,%20Sizheng&rft.date=2024-06-11&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.2308.10361&rft_dat=%3Cproquest%3E2854680176%3C/proquest%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-a526-dc0a60e742ae116102bc3da660e62edc5691305d6cab6adf47b242cad380eab33%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=2854680176&rft_id=info:pmid/&rfr_iscdi=true