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dc.contributor.author | Albert, A.![]() |
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dc.contributor.author | Alves, S![]() |
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dc.contributor.author | Andre, M.![]() |
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dc.contributor.author | Ardid, M.![]() |
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dc.contributor.author | Ardid, S.![]() |
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dc.contributor.author | Aubert, J.J.![]() |
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dc.contributor.author | Aublin, J.![]() |
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dc.contributor.author | Baret, B.![]() |
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dc.contributor.author | Basa, S.![]() |
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dc.contributor.author | Becherini, Y.![]() |
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dc.contributor.author | Belhorma, B.![]() |
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dc.contributor.author | Bendahman, M.![]() |
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dc.contributor.author | Benfenati, F.![]() |
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dc.contributor.author | Bertin, V.![]() |
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dc.contributor.author | Biagi, S.![]() |
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dc.contributor.author | García-Méndez, Juan![]() |
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dc.date.accessioned | 2024-06-03T18:17:53Z | |
dc.date.available | 2024-06-03T18:17:53Z | |
dc.date.issued | 2023-04 | es_ES |
dc.identifier.issn | 1475-7516 | es_ES |
dc.identifier.uri | http://hdl.handle.net/10251/204675 | |
dc.description.abstract | [EN] Since 2015 the LIGO and Virgo interferometers have detected gravitational waves from almost one hundred coalescences of compact objects (black holes and neutron stars). This article presents the results of a search performed with data from the ANTARES telescope to identify neutrino counterparts to the gravitational wave sources detected during the third LIGO/Virgo observing run and reported in the catalogues GWTC-2, GWTC-2.1, and GWTC-3. This search is sensitive to all-sky neutrinos of all flavours and of energies > 100 GeV, thanks to the inclusion of both track-like events (mainly induced by v mu charged -current interactions) and shower-like events (induced by other interaction types). Neutrinos are selected if they are detected within +/- 500 s from the GW merger and with a reconstructed direction compatible with its sky localisation. No significant excess is found for any of the 80 analysed GW events, and upper limits on the neutrino emission are derived. Using the information from the GW catalogues and assuming isotropic emission, upper limits on the total energy Etot,v emitted as neutrinos of all flavours and on the ratio fv = Etot,v/EGW between neutrino and GW emissions are also computed. Finally, a stacked analysis of all the 72 binary black hole mergers (respectively the 7 neutron star-black hole merger candidates) has been performed to constrain the typical neutrino emission within this population, leading to the limits: Etot,v < 4.0 x 1053 erg and fv < 0.15 (respectively, Etot,v < 3.2 x 1053 erg and fv < 0.88) for E-2 spectrum and isotropic emission. Other assumptions including softer spectra and non-isotropic scenarios have also been tested. | es_ES |
dc.description.sponsorship | The authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat a l'energie atomique et aux energies alternatives (CEA), Commission Europeenne (FEDER fund and Marie Curie Program), LabEx UnivEarthS (ANR-10-LABX-0023 and ANR-18-IDEX-0001), Region Alsace (contrat CPER), Region Provence-Alpes-Cpte d'Azur, Departement du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium fuer Bildung und Forschung (BMBF), Germany; Istituto Nazionale di Fisica Nucleare (INFN), the European Union's Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie grant agreement No 754496, Italy; Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands; Executive Unit for Financing Higher Education, Research, Development and Innovation (UEFISCDI), Romania; Grants PID2021-124591NB-C41,-C42,-C43 funded by MCIN/AEI/10.13039/501100011033 and, as appropriate, by "ERDF A way of making Europe", by the "European Union" or by the "European Union NextGenerationEU/PRTR", Programa de Planes Complementarios I+D+I (refs. ASFAE/2022/023, ASFAE/2022/014), Programa Prometeo (PROMETEO/2020/019) and GenT (refs. CIDEGENT/2018/034,/2019/043,/2020/049./2021/23) of the Generalitat<EM><STRONG> </STRONG></EM>Valenciana, Junta de Andalucia (ref. P18-FR-5057), EU: MSC program (ref. 101025085), Programa Maria Zambrano (Spanish Ministry of Universities, funded by the European Union, NextGenerationEU), Spain; Ministry of Higher Education, Scientific Research and Innovation, Morocco, and the Arab Fund for Economic and Social Development, Kuwait. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities. | es_ES |
dc.language | Inglés | es_ES |
dc.publisher | IOP Publishing | es_ES |
dc.relation.ispartof | Journal of Cosmology and Astroparticle Physics | es_ES |
dc.rights | Reconocimiento (by) | es_ES |
dc.subject | Gravitational waves | es_ES |
dc.subject | Sources | es_ES |
dc.subject | Neutrino astronomy | es_ES |
dc.subject | Neutron stars | es_ES |
dc.subject.classification | FISICA APLICADA | es_ES |
dc.title | Search for neutrino counterparts to the gravitational wave sources from LIGO/Virgo O3 run with the ANTARES detector | es_ES |
dc.type | Artículo | es_ES |
dc.identifier.doi | 10.1088/1475-7516/2023/04/004 | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/PID2021-124591NB-C41/ES/ELESCOPIOS DE NEUTRINOS PARA FISICA FUNDAMENTAL Y ASTRONOMIA MULTIMENSAJERO EN EL IFIC/ | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/PID2021-124591NB-C42/ES/TELESCOPIOS DE NEUTRINOS PARA FISICA FUNDAMENTAL Y ASTRONOMIA MULTI-MENSAJERO EN LA UPV/ | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/PID2021-124591NB-C43/ES/TELESCOPIOS DE NEUTRINOS PARA FISICA FUNDAMENTAL Y ASTRONOMIA MULTI-MENSAJERO EN LA UGR/ | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/ANR//ANR-10-LABX-0023/FR/Universe: observation, modeling, transfer/ | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/ANR//ANR-18-IDEX-0001/FR/Université de Paris/ | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/EC/H2020/101025085/EU/Unifying Neutrino Observatories Searches/ | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/EC/H2020/754496/EU/FELLowship for Innovation at INFN/ | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/GV INNOV.UNI.CIENCIA//ASFAE%2F2022%2F014//Telescopios submarinos de neutrinos: nuevas perspectivas / | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/GENERALITAT VALENCIANA//CIDEGENT%2F2019%2F043//ARTIFICIAL GENERAL INTELLIGENCE:BEYOND DEEP LEARNING/ | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/Junta de Andalucía//P18-FR-5057/ | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/GVA//CIDEGENT%2F2018%2F034 / | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/GVA//CIDEGENT%2F2019%2F043/ | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/GVA//CIDEGENT%2F2020%2F049 / | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/GVA//CIDEGENT%2F2021%2F23/ | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/GVA//PROMETEO%2F2020%2F019/ | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/MICINN//ASFAE%2F2022%2F014/ | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/MICINN//ASFAE%2F2022%2F023/ | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/Conseil Régional d'Alsace//CPER/ | es_ES |
dc.rights.accessRights | Abierto | es_ES |
dc.contributor.affiliation | Universitat Politècnica de València. Instituto de Investigación para la Gestión Integral de Zonas Costeras - Institut d'Investigació per a la Gestió Integral de Zones Costaneres | es_ES |
dc.contributor.affiliation | Universitat Politècnica de València. Escuela Técnica Superior de Ingeniería del Diseño - Escola Tècnica Superior d'Enginyeria del Disseny | es_ES |
dc.description.bibliographicCitation | Albert, A.; Alves, S.; Andre, M.; Ardid, M.; Ardid, S.; Aubert, J.; Aublin, J.... (2023). Search for neutrino counterparts to the gravitational wave sources from LIGO/Virgo O3 run with the ANTARES detector. Journal of Cosmology and Astroparticle Physics. (4). https://doi.org/10.1088/1475-7516/2023/04/004 | es_ES |
dc.description.accrualMethod | S | es_ES |
dc.relation.publisherversion | https://doi.org/10.1088/1475-7516/2023/04/004 | es_ES |
dc.type.version | info:eu-repo/semantics/publishedVersion | es_ES |
dc.description.issue | 4 | es_ES |
dc.relation.pasarela | S\513174 | es_ES |
dc.contributor.funder | European Commission | es_ES |
dc.contributor.funder | Junta de Andalucía | es_ES |
dc.contributor.funder | GENERALITAT VALENCIANA | es_ES |
dc.contributor.funder | Conseil Régional d'Alsace | es_ES |
dc.contributor.funder | AGENCIA ESTATAL DE INVESTIGACION | es_ES |
dc.contributor.funder | Agencia Estatal de Investigación | es_ES |
dc.contributor.funder | European Regional Development Fund | es_ES |
dc.contributor.funder | Ministerio de Ciencia e Innovación | es_ES |
dc.contributor.funder | Instituto Nazionale di Fisica Nucleare | es_ES |
dc.contributor.funder | Arab Fund for Economic and Social Development | es_ES |
dc.contributor.funder | Netherlands Organization for Scientific Research | es_ES |
dc.contributor.funder | Centre National de la Recherche Scientifique, Francia | es_ES |
dc.contributor.funder | Bundesministerium für Bildung und Forschung, Alemania | es_ES |
dc.contributor.funder | Executive Agency for Higher Education, Scientific Research, Development and Innovation Funding, Rumanía | es_ES |
dc.contributor.funder | Ministère de l'Education Nationale, de la Formation professionnelle, de l'Enseignement Supérieur et de la Recherche Scientifique, Marruecos | es_ES |