Letter of intent for KM3NeT 2.0
Metadatos
Mostrar el registro completo del ítemEditorial
IOP Publishing Ltd
Materia
Neutrino astronomy Neutrino Physics Deep sea neutrino telescope, Neutrino mass hierarchy
Fecha
2016Referencia bibliográfica
Adrian-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]
Patrocinador
The 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.Resumen
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 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.