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dc.contributor.authorAlbert, Arthur
dc.contributor.authorAlves Garre, Sergio
dc.contributor.authorAndré, Michel
dc.contributor.authorArdid Ramírez, Miguel
dc.contributor.authorArdid Ramírez, Joan Salvador
dc.contributor.authorAubert, J.-J.
dc.contributor.authorAublin, J.
dc.contributor.authorBaret, Bruny
dc.contributor.authorBasa, S.
dc.contributor.authorBecherini, Y.
dc.contributor.authorBelhorma, Bouchra
dc.contributor.authorBendahman, Meriem
dc.contributor.authorBenfenati, Fabio
dc.contributor.authorBertin, Vincent
dc.contributor.authorBiagi, S.
dc.contributor.otherCentre Tecnològic de Vilanova i la Geltrú
dc.date.accessioned2023-05-08T10:10:40Z
dc.date.available2023-05-08T10:10:40Z
dc.date.issued2023-04-01
dc.identifier.citationAlbert, A. [et al.]. Search for neutrino counterparts to the gravitational wave sources from LIGO/Virgo O3 run with the ANTARES detector. "Journal of cosmology and astroparticle physics", 1 Abril 2023, vol. 2023, núm. 4.
dc.identifier.issn1475-7516
dc.identifier.otherhttps://arxiv.org/abs/2302.07723
dc.identifier.urihttp://hdl.handle.net/2117/387159
dc.description.abstractSince 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 ¿µ chargedcurrent 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,¿ emitted as neutrinos of all flavours and on the ratio f¿ = Etot,¿/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,¿ < 4.0 × 1053 erg and f¿ < 0.15 (respectively, Etot,¿ < 3.2 × 1053 erg and f¿ < 0.88) for E-2 spectrum and isotropic emission. Other assumptions including softer spectra and non-isotropic scenarios have also been tested
dc.language.isoeng
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 International
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/
dc.subjectÀrees temàtiques de la UPC::Física::Astronomia i astrofísica
dc.subject.lcshNeutrinos
dc.subject.lcshAstrophysics
dc.subject.lcshTelescopes
dc.subject.lcshGravitational waves
dc.subject.otherGravitational waves
dc.subject.otherSources
dc.subject.otherNeutrino astronomy
dc.subject.otherNeutron stars
dc.titleSearch for neutrino counterparts to the gravitational wave sources from LIGO/Virgo O3 run with the ANTARES detector
dc.typeArticle
dc.subject.lemacNeutrins
dc.subject.lemacAstrofísica
dc.subject.lemacTelescopis
dc.subject.lemacOnes gravitacionals
dc.contributor.groupUniversitat Politècnica de Catalunya. LAB - Laboratori d'Aplicacions Bioacústiques
dc.identifier.doi10.1088/1475-7516/2023/04/004
dc.description.peerreviewedPeer Reviewed
dc.relation.publisherversionhttps://iopscience.iop.org/article/10.1088/1475-7516/2023/04/004
dc.rights.accessOpen Access
local.identifier.drac35752507
dc.description.versionPostprint (published version)
local.citation.authorAlbert, A.; Alves, S.; Andre, M.; Ardid, M.; Ardid, J.; Aubert, J.; Aublin, J.; Baret, B.; Basa, S.; Becherini, Y.; Belhorma, B.; Bendahman, M.; Benfenati, F.; Bertin, V.; Biagi, S.
local.citation.publicationNameJournal of cosmology and astroparticle physics
local.citation.volume2023
local.citation.number004
dc.description.authorshipA. Albert, S. Alves, M. André, M. Ardid, S. Ardid, J.-J. Aubert, J. Aublin, B. Baret, S. Basa, Y. Becherini, B. Belhorma, M. Bendahman, F. Benfenati, V. Bertin, S. Biagi, M. Bissinger, J. Boumaaza, M. Bouta, M.C. Bouwhuis, H. Brânzaş, R. Bruijn, J. Brunner, J. Busto, B. Caiffi, D. Calvo, S. Campion, A. Capone, L. Caramete, F. Carenini, J. Carr, V. Carretero, S. Celli, L. Cerisy, M. Chabab, T.N. Chau, R. Cherkaoui El Moursli, T. Chiarusi, M. Circella, J.A.B. Coelho, A. Coleiro, R. Coniglione, P. Coyle, A. Creusot, A.S.M. Cruz, A.F. Díaz, B. De Martino, C. Distefano, I. Di Palma, A. Domi, C. Donzaud, D. Dornic, D. Drouhin, T. Eberl, T. van Eeden, D. van Eijk, S. El Hedri, N. El Khayati, A. Enzenhöfer, P. Fermani, G. Ferrara, F. Filippini, L. Fusco, S. Gagliardini, J. García, C. Gatius Oliver, P. Gay, N. Geißelbrecht, H. Glotin, R. Gozzini, R. Gracia Ruiz, K. Graf, C. Guidi, L. Haegel, S. Hallmann, H. van Haren, A.J. Heijboer, Y. Hello, J.J. Hernández-Rey, J. Hößl, J. Hofestädt, F. Huang, G. Illuminati, C.W. James, B. Jisse-Jung, M. de Jong, P. de Jong, M. Kadler, O. Kalekin, U. Katz, A. Kouchner, I. Kreykenbohm, V. Kulikovskiy, R. Lahmann, M. Lamoureux, A. Lazo, D. Lefèvre, E. Leonora, G. Levi, S. Le Stum, D. Lopez-Coto, S. Loucatos, L. Maderer, J. Manczak, M. Marcelin, A. Margiotta, A. Marinelli, J.A. Martínez-Mora, P. Migliozzi, A. Moussa, R. Muller, L. Nauta, S. Navas, E. Nezri, B. Ó Fearraigh, A. Păun, G.E. Păvălaş, M. Perrin-Terrin, V. Pestel, P. Piattelli, C. Poirè, V. Popa, T. Pradier, N. Randazzo, D. Real, S. Reck, G. Riccobene, A. Romanov, A. Sánchez-Losa, A. Saina, F. Salesa Greus, D.F.E. Samtleben, M. Sanguineti, P. Sapienza, J. Schnabel, J. Schumann, F. Schüssler, J. Seneca, M. Spurio, Th. Stolarczyk, M. Taiuti, Y. Tayalati, S.J. Tingay, B. Vallage, G. Vannoye, V. Van Elewyck, S. Viola, D. Vivolo, J. Wilms, S. Zavatarelli, A. Zegarelli, J.D. Zornoza, J. Zúñiga


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