The neutrino plays a key role at the frontier of particle physics and astrophysics. Its mass has strong implications in particle physics, for it opens a door to theories of great unification beyond the standard model, and in cosmology, in connection with dark matter. Its very nature is not established: is it a particle of Majorana or of Dirac, that is to say, is it or not its own antiparticle? In addition, the neutrino is an incomparable messenger: its low probability of interaction allows it to be easily extracted from the densest emissive media (Sun, deep layers of supernovas, active nuclei of galaxies) and to probe the universe over distances cosmological.

The neutrino exists in three flavors (ne, nm, nt). One of the most important results of recent years in particle physics is the discovery of the phenomenon of oscillation of neutrinos, that is, their transformation from one flavor to another during their propagation, which implies that The neutrinos have a non-zero mass (which was not originally foreseen by the standard model of particle physics). The oscillations were discovered with the experiments of solar neutrinos (as Borexino) and atmospheric neutrinos and then confirmed by experiments with reactors and on beams, which allowed an accurate measurement of the mixing parameters. The latest is the mixing angle q13, measured, among other things, by the Double Chooz experiment (image) in which the laboratory took a leading part. The non-zero value of this parameter now opens the way to the precise study of the nm-to-ne transition with atmospheric neutrinos (KM3NeT / ORCA project) and beam neutrinos (DUNE project and associated R & D WA105 at CERN). This should make it possible to know the ordering of the masses of the neutrinos and the measurement of the phase CP, fundamental parameter related to the asymmetry matter-antimatter in the universe.

It is in this context that the "neutrinos" group of the APC laboratory contributes to the main axes of neutrino physics through the projects already mentioned and participation in the future generation experiment with JUNO reactors. The group is also involved in the SOX experiment that studies short-range oscillations to explore the possible existence of a fourth family of neutrinos, known as sterile, in the sense that it does not interact with matter.

The APC Neutrinos Group is also a member of the DarkSide collaboration, which develops a new TPC technology for liquid and gaseous Argon for direct dark matter research.

In the field of neutrino astronomy, participation in the exploitation of the submarine telescope ANTARES and its successor KM3NeT / ARCA is discussed in the section on high energy astrophysics.

Contact for the CNRS 01/02 opening « Neutrino Physics at Accelerators »: (subject: Concours%20CNRS) (Thomas Patzak)

Group Leader: Davide Franco

Deputy Head: Antoine Kouchner

The Neutrinos Team

    AGNES Paolo
    AVGITAS Theodore
    BOURRET Simon
    CABRERA Anatael
    CRIBIER Michel
    DE KERRET Hervé
    FRANCO Davide
    GALATA Salvatore
    GOMEZ Hector
    HOUDY Thibaut
    HOUQUE Dawson Jaime
    HOURLIER Adrien
    KATSANEVAS Stavros
    KOUCHNER Antoine
    KRYN Didier
    LASSERRE Thierry
    OBOLENSKY Michel
    PATZAK Thomas
    RONCIN Romain
    TONAZZO Alessandra
    VAN ELEWYCK Veronique
    VANNUCCI François
    VIGNAUD Daniel


    The history of neutrinos
    The Neutrino Oscillation Industry