Gravitational waves in the circular restricted three body problem

The prospect of unprecedented high-quality data of gravitational waves in the upcoming decades demands a theoretical effort to optimally study and analyze the signals that next generation detectors will provide. Here we study the gravitational wave emission and related dynamics during the inspiralli...

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Detalles Bibliográficos
Autores: Martin Barandiaran, Mikel, Kuroyanagi, Sachiko, Nesseris, Savvas
Tipo de recurso: artículo
Fecha de publicación:2024
País:España
Institución:Universidad Autónoma de Madrid
Repositorio:Biblos-e Archivo. Repositorio Institucional de la UAM
Idioma:inglés
OAI Identifier:oai:repositorio.uam.es:10486/720074
Acceso en línea:http://hdl.handle.net/10486/720074
https://dx.doi.org/10.1088/1361-6382/ad36a7
Access Level:acceso abierto
Palabra clave:black holes
circular restricted three body problem
general relativity
gravitational waves
Física
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spelling Gravitational waves in the circular restricted three body problemMartin Barandiaran, MikelKuroyanagi, SachikoNesseris, Savvasblack holescircular restricted three body problemgeneral relativitygravitational wavesFísicaThe prospect of unprecedented high-quality data of gravitational waves in the upcoming decades demands a theoretical effort to optimally study and analyze the signals that next generation detectors will provide. Here we study the gravitational wave emission and related dynamics during the inspiralling phase of the Circular Restricted Three Body Problem, a modification of the conventional binary scenario in which a small third object co-rotates with the parent binary system. Specifically, we obtain analytic expressions for the emitted power, frequency variation and other dynamical variables that describe the evolution of the system. As a key highlight, we find that the presence of the third body actually slows down the coalescence of the binary, which can be partially interpreted as an effective rescaling of the binary’s chirp-mass. Our analysis assumes semi-Keplerian orbits for the particles and a highly mass asymmetric parent binary needed for the stability of orbitsThe authors acknowledge support from the research Project PID2021-123012NB-C43 and the Spanish Research Agency (Agencia Estatal de Investigaci\u00F3n) through the Grant IFT Centro de Excelencia Severo Ochoa No. CEX2020-001007-S, funded by MCIN/AEI/10.13039/501100011033. S K is supported by the Spanish Atracci\u00F3n de Talento Contract No. 2019-T1/TIC-13177 granted by Comunidad de Madrid, the I+D Grant PID2020-118159GA-C42 funded by MCIN/AEI/10.13039/501100011033, the i-LINK 2021 Grant LINKA20416 of CSIC, and Japan Society for the Promotion of Science (JSPS) KAKENHI Grant Nos. 20H01899, 20H05853, and 23H00110. M M acknowledges support from the JAE Intro ICU Grant No. JAEIntroICU-2022-IFT-14.IOP PublishingFacultad de Ciencias20242024-05-02research articlehttp://purl.org/coar/resource_type/c_2df8fbb1AMhttp://purl.org/coar/version/c_ab4af688f83e57aainfo:eu-repo/semantics/articleapplication/pdfhttp://hdl.handle.net/10486/720074https://dx.doi.org/10.1088/1361-6382/ad36a7reponame:Biblos-e Archivo. Repositorio Institucional de la UAMinstname:Universidad Autónoma de MadridInglésengopen accesshttp://purl.org/coar/access_right/c_abf2Attribution 4.0 Internationalhttp://creativecommons.org/licenses/by/4.0/info:eu-repo/semantics/openAccessoai:repositorio.uam.es:10486/7200742026-06-23T12:46:27Z
dc.title.none.fl_str_mv Gravitational waves in the circular restricted three body problem
title Gravitational waves in the circular restricted three body problem
spellingShingle Gravitational waves in the circular restricted three body problem
Martin Barandiaran, Mikel
black holes
circular restricted three body problem
general relativity
gravitational waves
Física
title_short Gravitational waves in the circular restricted three body problem
title_full Gravitational waves in the circular restricted three body problem
title_fullStr Gravitational waves in the circular restricted three body problem
title_full_unstemmed Gravitational waves in the circular restricted three body problem
title_sort Gravitational waves in the circular restricted three body problem
dc.creator.none.fl_str_mv Martin Barandiaran, Mikel
Kuroyanagi, Sachiko
Nesseris, Savvas
author Martin Barandiaran, Mikel
author_facet Martin Barandiaran, Mikel
Kuroyanagi, Sachiko
Nesseris, Savvas
author_role author
author2 Kuroyanagi, Sachiko
Nesseris, Savvas
author2_role author
author
dc.contributor.none.fl_str_mv Facultad de Ciencias
dc.subject.none.fl_str_mv black holes
circular restricted three body problem
general relativity
gravitational waves
Física
topic black holes
circular restricted three body problem
general relativity
gravitational waves
Física
description The prospect of unprecedented high-quality data of gravitational waves in the upcoming decades demands a theoretical effort to optimally study and analyze the signals that next generation detectors will provide. Here we study the gravitational wave emission and related dynamics during the inspiralling phase of the Circular Restricted Three Body Problem, a modification of the conventional binary scenario in which a small third object co-rotates with the parent binary system. Specifically, we obtain analytic expressions for the emitted power, frequency variation and other dynamical variables that describe the evolution of the system. As a key highlight, we find that the presence of the third body actually slows down the coalescence of the binary, which can be partially interpreted as an effective rescaling of the binary’s chirp-mass. Our analysis assumes semi-Keplerian orbits for the particles and a highly mass asymmetric parent binary needed for the stability of orbits
publishDate 2024
dc.date.none.fl_str_mv 2024
2024-05-02
dc.type.none.fl_str_mv research article
http://purl.org/coar/resource_type/c_2df8fbb1
AM
http://purl.org/coar/version/c_ab4af688f83e57aa
dc.type.openaire.fl_str_mv info:eu-repo/semantics/article
format article
dc.identifier.none.fl_str_mv http://hdl.handle.net/10486/720074
https://dx.doi.org/10.1088/1361-6382/ad36a7
url http://hdl.handle.net/10486/720074
https://dx.doi.org/10.1088/1361-6382/ad36a7
dc.language.none.fl_str_mv Inglés
eng
language_invalid_str_mv Inglés
language eng
dc.rights.none.fl_str_mv open access
http://purl.org/coar/access_right/c_abf2
Attribution 4.0 International
http://creativecommons.org/licenses/by/4.0/
dc.rights.openaire.fl_str_mv info:eu-repo/semantics/openAccess
rights_invalid_str_mv open access
http://purl.org/coar/access_right/c_abf2
Attribution 4.0 International
http://creativecommons.org/licenses/by/4.0/
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv IOP Publishing
publisher.none.fl_str_mv IOP Publishing
dc.source.none.fl_str_mv reponame:Biblos-e Archivo. Repositorio Institucional de la UAM
instname:Universidad Autónoma de Madrid
instname_str Universidad Autónoma de Madrid
reponame_str Biblos-e Archivo. Repositorio Institucional de la UAM
collection Biblos-e Archivo. Repositorio Institucional de la UAM
repository.name.fl_str_mv
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