Observation of Gravitational Waves from the Coalescence of a 2.5–4.5 M⊙ Compact Object and a Neutron Star

The LIGO Scientific Collaboration, the Virgo Collaboration, and the KAGRA Collaboration: A. G. Abac et al.

Detalles Bibliográficos
Autores: Abac, A. G., Bera, S., Colleoni, Marta, Cremonese, P., Braglia, M., García-Bellido, Juan, Jaraba, Santiago, Kuroyanagi, Sachiko, Morrás, Gonzalo, Nuño Siles, J.F., Ruiz Morales, E., Marín Pina, Daniel, LIGO Scientific Collaboration, Virgo Collaboration, KAGRA Collaboration
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2024
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/382352
Acceso en línea:http://hdl.handle.net/10261/382352
Access Level:acceso abierto
Palabra clave:Gravitational wave astronomy
Gravitational wave detectors
Gravitational wave sources
Stellar mass black holes
Neutron stars
http://astrothesaurus.org/uat/675
http://astrothesaurus.org/uat/676
http://astrothesaurus.org/uat/677
http://astrothesaurus.org/uat/1611
http://astrothesaurus.org/uat/1108
id ES_f49b890b9bbfd6038c32b52cc5ea5f39
oai_identifier_str oai:digital.csic.es:10261/382352
network_acronym_str ES
network_name_str España
repository_id_str
dc.title.none.fl_str_mv Observation of Gravitational Waves from the Coalescence of a 2.5–4.5 M⊙ Compact Object and a Neutron Star
title Observation of Gravitational Waves from the Coalescence of a 2.5–4.5 M⊙ Compact Object and a Neutron Star
spellingShingle Observation of Gravitational Waves from the Coalescence of a 2.5–4.5 M⊙ Compact Object and a Neutron Star
Abac, A. G.
Gravitational wave astronomy
Gravitational wave detectors
Gravitational wave sources
Stellar mass black holes
Neutron stars
http://astrothesaurus.org/uat/675
http://astrothesaurus.org/uat/676
http://astrothesaurus.org/uat/677
http://astrothesaurus.org/uat/1611
http://astrothesaurus.org/uat/1108
title_short Observation of Gravitational Waves from the Coalescence of a 2.5–4.5 M⊙ Compact Object and a Neutron Star
title_full Observation of Gravitational Waves from the Coalescence of a 2.5–4.5 M⊙ Compact Object and a Neutron Star
title_fullStr Observation of Gravitational Waves from the Coalescence of a 2.5–4.5 M⊙ Compact Object and a Neutron Star
title_full_unstemmed Observation of Gravitational Waves from the Coalescence of a 2.5–4.5 M⊙ Compact Object and a Neutron Star
title_sort Observation of Gravitational Waves from the Coalescence of a 2.5–4.5 M⊙ Compact Object and a Neutron Star
dc.creator.none.fl_str_mv Abac, A. G.
Bera, S.
Colleoni, Marta
Cremonese, P.
Braglia, M.
García-Bellido, Juan
Jaraba, Santiago
Kuroyanagi, Sachiko
Morrás, Gonzalo
Nuño Siles, J.F.
Ruiz Morales, E.
Marín Pina, Daniel
LIGO Scientific Collaboration
Virgo Collaboration
KAGRA Collaboration
author Abac, A. G.
author_facet Abac, A. G.
Bera, S.
Colleoni, Marta
Cremonese, P.
Braglia, M.
García-Bellido, Juan
Jaraba, Santiago
Kuroyanagi, Sachiko
Morrás, Gonzalo
Nuño Siles, J.F.
Ruiz Morales, E.
Marín Pina, Daniel
LIGO Scientific Collaboration
Virgo Collaboration
KAGRA Collaboration
author_role author
author2 Bera, S.
Colleoni, Marta
Cremonese, P.
Braglia, M.
García-Bellido, Juan
Jaraba, Santiago
Kuroyanagi, Sachiko
Morrás, Gonzalo
Nuño Siles, J.F.
Ruiz Morales, E.
Marín Pina, Daniel
LIGO Scientific Collaboration
Virgo Collaboration
KAGRA Collaboration
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.contributor.none.fl_str_mv Agencia Estatal de Investigación (España)
Ministerio de Ciencia, Innovación y Universidades (España)
European Commission
Govern de les Illes Balears
Generalitat Valenciana
Generalitat de Catalunya
National Science Foundation (US)
Abac, A. G. [0000-0003-4786-2698]
Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
dc.subject.none.fl_str_mv Gravitational wave astronomy
Gravitational wave detectors
Gravitational wave sources
Stellar mass black holes
Neutron stars
http://astrothesaurus.org/uat/675
http://astrothesaurus.org/uat/676
http://astrothesaurus.org/uat/677
http://astrothesaurus.org/uat/1611
http://astrothesaurus.org/uat/1108
topic Gravitational wave astronomy
Gravitational wave detectors
Gravitational wave sources
Stellar mass black holes
Neutron stars
http://astrothesaurus.org/uat/675
http://astrothesaurus.org/uat/676
http://astrothesaurus.org/uat/677
http://astrothesaurus.org/uat/1611
http://astrothesaurus.org/uat/1108
description The LIGO Scientific Collaboration, the Virgo Collaboration, and the KAGRA Collaboration: A. G. Abac et al.
publishDate 2024
dc.date.none.fl_str_mv 2024
2025
2025
dc.type.none.fl_str_mv info:eu-repo/semantics/article
http://purl.org/coar/resource_type/c_6501
Publisher's version
info:eu-repo/semantics/publishedVersion
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/10261/382352
url http://hdl.handle.net/10261/382352
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.relation.none.fl_str_mv The underlying dataset has been published as supplementary material of the article in the publisher platform at DOI 10.3847/2041-8213/ad5beb
https://doi.org/10.3847/2041-8213/ad5beb
Sí
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
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:DIGITAL.CSIC. Repositorio Institucional del CSIC
instname:Consejo Superior de Investigaciones Científicas (CSIC)
instname_str Consejo Superior de Investigaciones Científicas (CSIC)
reponame_str DIGITAL.CSIC. Repositorio Institucional del CSIC
collection DIGITAL.CSIC. Repositorio Institucional del CSIC
repository.name.fl_str_mv
repository.mail.fl_str_mv
_version_ 1869424487504543744
spelling Observation of Gravitational Waves from the Coalescence of a 2.5–4.5 M⊙ Compact Object and a Neutron StarAbac, A. G.Bera, S.Colleoni, MartaCremonese, P.Braglia, M.García-Bellido, JuanJaraba, SantiagoKuroyanagi, SachikoMorrás, GonzaloNuño Siles, J.F.Ruiz Morales, E.Marín Pina, DanielLIGO Scientific CollaborationVirgo CollaborationKAGRA CollaborationGravitational wave astronomyGravitational wave detectorsGravitational wave sourcesStellar mass black holesNeutron starshttp://astrothesaurus.org/uat/675http://astrothesaurus.org/uat/676http://astrothesaurus.org/uat/677http://astrothesaurus.org/uat/1611http://astrothesaurus.org/uat/1108The LIGO Scientific Collaboration, the Virgo Collaboration, and the KAGRA Collaboration: A. G. Abac et al.We report the observation of a coalescing compact binary with component masses 2.5–4.5 M⊙ and 1.2–2.0 M⊙ (all measurements quoted at the 90% credible level). The gravitational-wave signal GW230529_181500 was observed during the fourth observing run of the LIGO–Virgo–KAGRA detector network on 2023 May 29 by the LIGO Livingston observatory. The primary component of the source has a mass less than 5 M⊙ at 99% credibility. We cannot definitively determine from gravitational-wave data alone whether either component of the source is a neutron star or a black hole. However, given existing estimates of the maximum neutron star mass, we find the most probable interpretation of the source to be the coalescence of a neutron star with a black hole that has a mass between the most massive neutron stars and the least massive black holes observed in the Galaxy. We provisionally estimate a merger rate density of for compact binary coalescences with properties similar to the source of GW230529_181500; assuming that the source is a neutron star–black hole merger, GW230529_181500-like sources may make up the majority of neutron star–black hole coalescences. The discovery of this system implies an increase in the expected rate of neutron star–black hole mergers with electromagnetic counterparts and provides further evidence for compact objects existing within the purported lower mass gap.This material is based on work supported by NSF's LIGO Laboratory, which is a major facility fully funded by the National Science Foundation. The authors also gratefully acknowledge the support of the Science and Technology Facilities Council (STFC) of the United Kingdom, the Max-Planck-Society (MPS), and the State of Niedersachsen/Germany for support of the construction of Advanced LIGO and construction and operation of the GEO 600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council. The authors gratefully acknowledge the Italian Istituto Nazionale di Fisica Nucleare (INFN), the French Centre National de la Recherche Scientifique (CNRS), and the Netherlands Organization for Scientific Research (NWO) for the construction and operation of the Virgo detector and the creation and support of the EGO consortium. The authors also gratefully acknowledge research support from these agencies, as well as by the Council of Scientific and Industrial Research of India, the Department of Science and Technology, India, the Science & Engineering Research Board (SERB), India, the Ministry of Human Resource Development, India, the Spanish Agencia Estatal de Investigación (AEI), the Spanish Ministerio de Ciencia, Innovación y Universidades, the European Union NextGenerationEU/PRTR (PRTR-C17.I1), the ICSC - CentroNazionale di Ricerca in High Performance Computing, Big Dataand Quantum Computing, funded by the European Union NextGenerationEU​​​​, the Comunitat Autonòma de les Illes Balears through the Direcció General de Recerca, Innovació i Transformació Digital with funds from the Tourist Stay Tax Law ITS 2017-006, the Conselleria d'Economia, Hisenda i Innovació the FEDER Operational Program 2021–2027 of the Balearic Islands, the Conselleria d'Innovació Universitats, Ciència i Societat Digital de la Generalitat Valenciana and the CERCA Programme Generalitat de Catalunya, Spain, the National Science Centre of Poland and the European Union—European Regional Development Fund; Foundation for Polish Science (FNP), the Polish Ministry of Science and Higher Education, the Swiss National Science Foundation (SNSF), the Russian Science Foundation, the European Commission, the European Social Funds (ESF), the European Regional Development Funds (ERDF), the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, the Hungarian Scientific Research Fund (OTKA), the French Lyon Institute of Origins (LIO), the Belgian Fonds de la Recherche Scientifique (FRS-FNRS), Actions de Recherche Concertées (ARC) and Fonds Wetenschappelijk Onderzoek—Vlaanderen (FWO), Belgium, the Paris Île-de-France Region, the National Research, Development and Innovation Office Hungary (NKFIH), the National Research Foundation of Korea, the Natural Science and Engineering Research Council Canada, Canadian Foundation for Innovation (CFI), the Brazilian Ministry of Science, Technology, and Innovations, the International Center for Theoretical Physics South American Institute for Fundamental Research (ICTP-SAIFR), the Research Grants Council of Hong Kong, the National Natural Science Foundation of China (NSFC), the Leverhulme Trust, the Research Corporation, the National Science and Technology Council (NSTC), Taiwan, the United States Department of Energy, and the Kavli Foundation. The authors gratefully acknowledge the support of the NSF, STFC, INFN, and CNRS for provision of computational resources. This work was supported by MEXT, JSPS Leading-edge Research Infrastructure Program, JSPS Grant-in-Aid for Specially Promoted Research 26000005, JSPS Grant-in-Aid for Scientific Research on Innovative Areas 2905: JP17H06358, JP17H06361 and JP17H06364, JSPS Core-to-Core Program A. Advanced Research Networks, JSPS Grant-in-Aid for Scientific Research (S) 17H06133 and 20H05639, JSPS Grant-in-Aid for Transformative Research Areas (A) 20A203: JP20H05854, the joint research program of the Institute for Cosmic Ray Research, University of Tokyo, National Research Foundation (NRF), Computing Infrastructure Project of Global Science experimental Data hub Center (GSDC) at KISTI, Korea Astronomy and Space Science Institute (KASI), and Ministry of Science and ICT (MSIT) in Korea, Academia Sinica (AS), AS Grid Center (ASGC) and the National Science and Technology Council (NSTC) in Taiwan under grants including the Rising Star Program and Science Vanguard Research Program, Advanced Technology Center (ATC) of NAOJ, and Mechanical Engineering Center of KEK. We thank the anonymous journal referee for helpful comments.Peer reviewedIOP PublishingAgencia Estatal de Investigación (España)Ministerio de Ciencia, Innovación y Universidades (España)European CommissionGovern de les Illes BalearsGeneralitat ValencianaGeneralitat de CatalunyaNational Science Foundation (US)Abac, A. G. [0000-0003-4786-2698]Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]202520252024info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionapplication/pdfhttp://hdl.handle.net/10261/382352reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)InglésThe underlying dataset has been published as supplementary material of the article in the publisher platform at DOI 10.3847/2041-8213/ad5bebhttps://doi.org/10.3847/2041-8213/ad5bebSíinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/3823522026-05-22T06:33:51Z
score 15.811543

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