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dc.contributor.authorAiello, S.
dc.contributor.authorAnguita López, Mancia 
dc.contributor.authorDíaz García, Antonio Francisco 
dc.contributor.authorLópez Coto, Daniel 
dc.contributor.authorNavas Concha, Sergio 
dc.contributor.authorTenllado, Enrique
dc.contributor.authorKM3NeT Collaboration
dc.date.accessioned2021-09-03T11:44:16Z
dc.date.available2021-09-03T11:44:16Z
dc.date.issued2021-05-24
dc.identifier.citationAiello, S... [et al.]. The KM3NeT potential for the next core-collapse supernova observation with neutrinos. Eur. Phys. J. C 81, 445 (2021). [https://doi.org/10.1140/epjc/s10052-021-09187-5]es_ES
dc.identifier.urihttp://hdl.handle.net/10481/70095
dc.descriptionThe authors acknowledge the financial support of the funding agencies: Agence Nationale de la Recherche (contract ANR-15-CE31-0020), Centre National de la Recherche Scientifique (CNRS), Commission Europeenne (FEDER fund and Marie Curie Program), Institut Universitaire de France (IUF), LabEx UnivEarthS (ANR-10-LABX-0023 and ANR-18-IDEX-0001), Paris Ile-de-France Region, France; Shota Rustaveli National Science Foundation of Georgia (SRNSFG, FR-18-1268), Georgia; Deutsche Forschungsgemeinschaft (DFG), Germany; The General Secretariat of Research and Technology (GSRT), Greece; Istituto Nazionale di Fisica Nucleare (INFN), Ministero dell'Universita e della Ricerca (MIUR), PRIN 2017 program (Grant NAT-NET 2017W4HA7S) Italy; Ministry of Higher Education Scientific Research and Professional Training, ICTP through Grant AF-13, Morocco; Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands; The National Science Centre, Poland (2015/18/E/ST2/00758); National Authority for Scientific Research (ANCS), Romania; Ministerio de Ciencia, Innovacion, Investigacion y Universidades (MCIU): Programa Estatal de Generacion de Conocimiento (refs. PGC2018-096663-B-C41, -A-C42, -B-C43, -B-C44) (MCIU/FEDER), Severo Ochoa Centre of Excellence and MultiDark Consolider (MCIU), Junta de Andalucia (ref. SOMM17/6104/UGR), Generalitat Valenciana: Grisolia (ref. GRISO-LIA/2018/119) and GenT (ref. CIDEGENT/2018/034 and CIDE-GENT/2019/043) programs, La Caixa Foundation (ref. LCF/BQ/IN17/11620019), EU: MSC program (ref. 713673), Spain. This work has also received funding from the European Union'sHorizon 2020 research and innovation program under Grant agreement no 739560.es_ES
dc.description.abstractThe KM3NeT research infrastructure is under construction in the Mediterranean Sea. It consists of two water Cherenkov neutrino detectors, ARCA and ORCA, aimed at neutrino astrophysics and oscillation research, respectively. Instrumenting a large volume of sea water with similar to 6200 optical modules comprising a total of similar to 200,000 photomultiplier tubes, KM3NeT will achieve sensitivity to similar to 10 MeV neutrinos from Galactic and near-Galactic core-collapse supernovae through the observation of coincident hits in photomultipliers above the background. In this paper, the sensitivity of KM3NeT to a supernova explosion is estimated from detailed analyses of background data from the first KM3NeT detection units and simulations of the neutrino signal. The KM3NeT observational horizon (for a 5 sigma discovery) covers essentially the Milky-Way and for the most optimistic model, extends to the Small Magellanic Cloud (similar to 60 kpc). Detailed studies of the time profile of the neutrino signal allow assessment of the KM3NeT capability to determine the arrival time of the neutrino burst with a few milliseconds precision for sources up to 5-8 kpc away, and detecting the peculiar signature of the standing accretion shock instability if the core-collapse supernova explosion happens closer than 3-5 kpc, depending on the progenitor mass. KM3NeT's capability to measure the neutrino flux spectral parameters is also presented.es_ES
dc.description.sponsorshipFrench National Research Agency (ANR) ANR-15-CE31-0020es_ES
dc.description.sponsorshipCentre National de la Recherche Scientifique (CNRS)es_ES
dc.description.sponsorshipCommission Europeenne, Francees_ES
dc.description.sponsorshipInstitut Universitaire de France (IUF), Francees_ES
dc.description.sponsorshipLabEx UnivEarthS, France ANR-10-LABX-0023 ANR-18-IDEX-0001es_ES
dc.description.sponsorshipParis Ile-de-France Region, Francees_ES
dc.description.sponsorshipShota Rustaveli National Science Foundation of Georgia (SRNSFG), Georgia FR-18-1268es_ES
dc.description.sponsorshipGerman Research Foundation (DFG)es_ES
dc.description.sponsorshipGreek Ministry of Development-GSRTes_ES
dc.description.sponsorshipGreek Ministry of Development-GSRTes_ES
dc.description.sponsorshipIstituto Nazionale di Fisica Nucleare (INFN)es_ES
dc.description.sponsorshipMinistry of Education, Universities and Research (MIUR)es_ES
dc.description.sponsorshipPRIN 2017 program, Italy NAT-NET 2017W4HA7Ses_ES
dc.description.sponsorshipMinistry of Higher Education Scientific Research and Professional Training, ICTP, Morocco AF-13es_ES
dc.description.sponsorshipNetherlands Organization for Scientific Research (NWO)es_ES
dc.description.sponsorshipNetherlands Governmentes_ES
dc.description.sponsorshipNational Science Centre, Poland 2015/18/E/ST2/00758es_ES
dc.description.sponsorshipNational Authority for Scientific Research (ANCS), Romaniaes_ES
dc.description.sponsorshipMinisterio de Ciencia, Innovacion, Investigacion y Universidades (MCIU): Programa Estatal de Generacion de Conocimiento, Spain PGC2018-096663-B-C41 PGC2018-096663-A-C42 PGC2018-096663-B-C43 PGC2018-096663-B-C44es_ES
dc.description.sponsorshipSevero Ochoa Centre of Excellence and MultiDark Consolider (MCIU), Spaines_ES
dc.description.sponsorshipJunta de Andalucia European Commission SOMM17/6104/UGRes_ES
dc.description.sponsorshipGeneralitat Valenciana: Grisolia, Spain GRISO-LIA/2018/119 GenT program, Spain CIDEGENT/2018/034 CIDE-GENT/2019/043es_ES
dc.description.sponsorshipLa Caixa Foundation LCF/BQ/IN17/11620019 EU: MSC program, Spain 713673es_ES
dc.description.sponsorshipEuropean Commission 739560es_ES
dc.language.isoenges_ES
dc.publisherSpringeres_ES
dc.rightsAtribución 3.0 España*
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/es/*
dc.titleThe KM3NeT potential for the next core-collapse supernova observation with neutrinoses_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.relation.projectIDinfo:eu-repo/grantAgreement/EC/H2020/739560es_ES
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses_ES
dc.identifier.doi10.1140/epjc/s10052-021-09187-5
dc.type.hasVersioninfo:eu-repo/semantics/publishedVersiones_ES


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