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dc.contributor.authorDíaz García, Antonio Francisco 
dc.contributor.authorNavas Concha, Sergio 
dc.date.accessioned2020-06-19T11:52:22Z
dc.date.available2020-06-19T11:52:22Z
dc.date.issued2016
dc.identifier.citationAdrian-Martinez, S., Ageron, M., Aharonian, F., Aiello, S., Albert, A., Ameli, F., ... & Anton, G. (2016). Letter of intent for KM3NeT 2.0. Journal of Physics G: Nuclear and Particle Physics, 43(8). [doi:10.1088/0954-3899/43/8/084001]es_ES
dc.identifier.urihttp://hdl.handle.net/10481/62568
dc.descriptionThe authors would like to thank D Allard, A Esmaili, G Fogli, O Mena, K Murase, S Palomares Ruiz, E Parizot, S T Petcov, S Razzaque, D Semikoz, A Yu Smirnov, F L Villante, F Vissani and R Zukanovich Funchal for their support and valuable discussions and suggestions in preparing this Letter of Intent.es_ES
dc.description.abstractThe main objectives of the KM3NeT Collaboration are (i) the discovery and subsequent observation of high-energy neutrino sources in the Universe and (ii) the determination of the mass hierarchy of neutrinos. These objectives are strongly motivated by two recent important discoveries, namely: (1) the highenergy astrophysical neutrino signal reported by IceCube and (2) the sizable contribution of electron neutrinos to the third neutrino mass eigenstate as reported by Daya Bay, Reno and others. To meet these objectives, the KM3NeT Collaboration plans to build a new Research Infrastructure consisting of a network of deep-sea neutrino telescopes in the Mediterranean Sea. A phased and distributed implementation is pursued which maximises the access to regional funds, the availability of human resources and the synergistic opportunities for the Earth and sea sciences community. Three suitable deep-sea sites are selected, namely off-shore Toulon (France), Capo Passero (Sicily, Italy) and Pylos (Peloponnese, Greece). The infrastructure will consist of three so-called building blocks. A building block comprises 115 strings, each string comprises 18 optical modules and each optical module comprises 31 photo-multiplier tubes. Each building block thus constitutes a threedimensional array of photo sensors that can be used to detect the Cherenkov light produced by relativistic particles emerging from neutrino interactions. Two building blocks will be sparsely configured to fully explore the IceCube signal with similar instrumented volume, different methodology, improved resolution and complementary field of view, including the galactic plane. One building block will be densely configured to precisely measure atmospheric neutrino oscillations.es_ES
dc.description.sponsorshipThe authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commission Européenne (FEDER fund and Marie Curie Program), Institut Universitaire de France (IUF), IdEx program and UnivEarthS Labex program at Sorbonne Paris Cité (ANR-10-LABX-0023 and ANR-11-IDEX-0005-02), France; The General Secretariat of Research and Technology (GSRT), Greece; Istituto Nazionale di Fisica Nucleare (INFN), Ministero dell'Istruzione, dell’Universitàe della Ricerca (MIUR), Italy; Agence de l’Oriental and CNRST, Morocco; Stichting voor Fundamenteel Onderzoek der Materie (FOM), Nederlandseorganisatie voor Wetenschappelijk Onderzoek (NWO), The Netherlands; National Authority for Scientific Research (ANCS), Romania; Plan Estatal de Investigación (refs. FPA2015-65150-C3-1-P, -2-P and -3-P, (MINECO/FEDER)), Severo Ochoa Centre of Excellence and MultiDark Consolider (MINECO), and Prometeo and Grisolía programs (Generalitat Valenciana), Spain. The KM3NeT collaboration has received funding from the European Community Sixth Framework Programme under Contract 011937 and the Seventh Framework Programme under Grant Agreement 212525.es_ES
dc.language.isoenges_ES
dc.publisherIOP Publishing Ltdes_ES
dc.rightsAtribución 3.0 España*
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/es/*
dc.subjectNeutrino astronomyes_ES
dc.subjectNeutrino Physicses_ES
dc.subjectDeep sea neutrino telescope,es_ES
dc.subjectNeutrino mass hierarchyes_ES
dc.titleLetter of intent for KM3NeT 2.0es_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.relation.projectIDeu-repo/grantAgreement/EC/FP7/212525es_ES
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses_ES
dc.identifier.doi10.1088/0954-3899/43/8/084001


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