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Published byStanley Cannon Modified over 8 years ago
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Michel Gonin – Ecole Polytechnique – France
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1987 : SUPER NOVA SN1987A Super-Kamiokande Introduction neutrino oscillations mixing matrices Introduction neutrino oscillations mixing matrices
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26 free parameters including 8 for neutrinos electron neutrino
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c = cos s = sin ? ≈ The last mixing angle 13 was missing before 2012 The complex phase δ is still unknow The last mixing angle 13 was missing before 2012 The complex phase δ is still unknow
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Measurements of the matrix elements θ 12 = 33.6 ◦ ± 1.0 ◦ θ 23 = 45 ◦ ± 6 ◦
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CP violation δ 0 " for the discovery of the origin of the broken symmetry which predicts the existence of at least three families of quarks in nature". 3 generations of particles 3 mixing angles, all different from zero. masse states flavor states
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World (new) baseline oscillation experiments
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beam beam Intense beam Near detectors Huge far detector
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sin 2 2 disappearance m 23 2 sin 2 2 e appearance T2K main physics goals Probe ν μ to ν e oscillations with sensitivity improvement Precise measurement of the “atmospheric” parameters 23, m 32 2
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How do we detect neutrinos ? Neutrino interaction with some unrelated muon (“rock muon”) Charge current quasi elastic neutrino interaction n p e e n p e e e n p e e n p e n p e e n p e e e n p e e n p e n p n p
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Feb. 3, 2009 Target Station
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Feb. 3, 2009 HornsHorns
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16 Inside the decay tunnel
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Non accelerator experiments (reactor)
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Exclusion for non zero - number of sin 2 (2 13 sin 2 (2 13 ) “appearance” θ 13 = 9.1 ◦ ± 0.6 ◦ 2010 - 2012
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e appearance e appearance Discovery of neutrino appearance in flavor oscillations New results
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e disappearance e disappearance
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New results 2013
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First indication for strong CP violation in the lepton sector ? New results 2013
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NOVA CP phase δ Perspectives Perspectives
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Is CP violated “strongly” in neutrino oscillation ? Is the source of the violation due to complex phase associated with 3 generations ? Only 3 generations for leptons ? Sterile neutrinos ? Unitary triangle and physics beyond the standard model
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High power accelerator and huge detector needed Asymmetry of neutrino and anti-neutrino induced by interaction in matter is large
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Measurement of 13 C=cos S=sin
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Merci beaucoup Joe !
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