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Letter of intent for KM3NeT 2.0

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Letter of intent for KM3NeT 2.0

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dc.contributor.author Adrián Martínez, Silvia es_ES
dc.contributor.author Ardid Ramírez, Miguel es_ES
dc.contributor.author Llorens Alvarez, Carlos David es_ES
dc.contributor.author Martínez Mora, Juan Antonio es_ES
dc.contributor.author Saldaña-Coscollar, María es_ES
dc.contributor.author Ageron, M. es_ES
dc.contributor.author Aharonian, F. es_ES
dc.contributor.author Aiello, S. es_ES
dc.contributor.author Albert, A. es_ES
dc.contributor.author Ameli, F. es_ES
dc.contributor.author Anassontzis, E. es_ES
dc.contributor.author Andre, M. es_ES
dc.contributor.author Androulakis, G. es_ES
dc.contributor.author Anghinolfi, M. es_ES
dc.contributor.author Anton, G. es_ES
dc.date.accessioned 2017-07-17T16:13:42Z
dc.date.available 2017-07-17T16:13:42Z
dc.date.issued 2016-08
dc.identifier.issn 0954-3899
dc.identifier.uri http://hdl.handle.net/10251/85307
dc.description.abstract [EN] The 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 high-energy 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 three-dimensional 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.sponsorship The authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commission Europeenne (FEDER fund and Marie Curie Program), Institut Universitaire de France (IUF), IdEx program and UnivEarthS Labex program at Sorbonne Paris Cite (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'Universitae 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 Investigacion (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 Grisolia 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. en_EN
dc.language Inglés es_ES
dc.publisher IOP Publishing es_ES
dc.relation.ispartof Journal of Physics G: Nuclear and Particle Physics es_ES
dc.rights Reconocimiento (by) es_ES
dc.subject Neutrino astronomy es_ES
dc.subject Neutrino physics es_ES
dc.subject Deep sea neutrino telescope es_ES
dc.subject Neutrino mass hierarchy es_ES
dc.subject.classification FISICA APLICADA es_ES
dc.title Letter of intent for KM3NeT 2.0 es_ES
dc.type Artículo es_ES
dc.identifier.doi 10.1088/0954-3899/43/8/084001
dc.relation.projectID info:eu-repo/grantAgreement/EC/FP7/212525/EU/Preparatory Phase for a Deep Sea Facility in the Mediterranean for Neutrino Astronomy and Associated Sciences/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/EC/FP6/11937/EU/Design Study for a Deep Sea Facility in the Mediterranean for Neutrino Astronomy and Associated Sciences/KM3NET/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/ANR//ANR-10-LABX-0023/FR/Earth - Planets - Universe: observation, modeling, transfer/UnivEarthS/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/ANR//ANR-11-IDEX-0005/FR/Université Sorbonne Paris Cité/USPC/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/MINECO//FPA2015-65150-C3-1-P/ES/PARTICIPACION DEL IFIC EN ANTARES, KM3NET-ARCA%2FORCA Y PDG/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/MINECO//FPA2015-65150-C3-2-P/ES/PARTICIPACION DE LA UPV EN ANTARES Y KM3NET-ARCA%2FORCA/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/MINECO//FPA2015-65150-C3-3-P/ES/PARTICIPACION DE LA UGR EN ANTARES, KM3NET-ARCA%2FORCA Y PDG/ es_ES
dc.rights.accessRights Abierto es_ES
dc.contributor.affiliation Universitat Politècnica de València. Departamento de Física Aplicada - Departament de Física Aplicada 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 Politécnica Superior de Gandia - Escola Politècnica Superior de Gandia es_ES
dc.description.bibliographicCitation Adrián Martínez, S.; Ardid Ramírez, M.; Llorens Alvarez, CD.; Martínez Mora, JA.; Saldaña-Coscollar, M.; Ageron, M.; Aharonian, F.... (2016). Letter of intent for KM3NeT 2.0. Journal of Physics G: Nuclear and Particle Physics. 43(8):1-130. https://doi.org/10.1088/0954-3899/43/8/084001 es_ES
dc.description.accrualMethod S es_ES
dc.relation.publisherversion http://dx.doi.org/10.1088/0954-3899/43/8/084001 es_ES
dc.description.upvformatpinicio 1 es_ES
dc.description.upvformatpfin 130 es_ES
dc.type.version info:eu-repo/semantics/publishedVersion es_ES
dc.description.volume 43 es_ES
dc.description.issue 8 es_ES
dc.relation.senia 315613 es_ES
dc.identifier.eissn 1361-6471
dc.contributor.funder European Commission
dc.contributor.funder Centre National de la Recherche Scientifique, Francia
dc.contributor.funder Agence Nationale de la Recherche, Francia
dc.contributor.funder Ministero dell'Istruzione dell'Università e della Ricerca, Italia
dc.contributor.funder Ministerio de Educación y Ciencia


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