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Michel Gonin – Ecole Polytechnique – France. 1987 : SUPER NOVA SN1987A Super-Kamiokande Introduction neutrino oscillations mixing matrices Introduction.

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Presentation on theme: "Michel Gonin – Ecole Polytechnique – France. 1987 : SUPER NOVA SN1987A Super-Kamiokande Introduction neutrino oscillations mixing matrices Introduction."— Presentation transcript:

1 Michel Gonin – Ecole Polytechnique – France

2 1987 : SUPER NOVA SN1987A Super-Kamiokande Introduction neutrino oscillations mixing matrices Introduction neutrino oscillations mixing matrices

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4 26 free parameters including 8 for neutrinos electron neutrino

5 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

6 Measurements of the matrix elements θ 12 = 33.6 ◦ ± 1.0 ◦ θ 23 = 45 ◦ ± 6 ◦

7 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

8 World (new) baseline oscillation experiments

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10 beam  beam  Intense beam  Near detectors  Huge far detector

11 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

12 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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14 Feb. 3, 2009 Target Station

15 Feb. 3, 2009 HornsHorns

16 16 Inside the decay tunnel

17 Non accelerator experiments (reactor)

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19 Exclusion for non zero - number of  sin 2 (2  13 sin 2 (2  13 ) “appearance” θ 13 = 9.1 ◦ ± 0.6 ◦ 2010 - 2012

20 e appearance e appearance Discovery of neutrino appearance in flavor oscillations New results

21 e disappearance e disappearance

22 New results 2013

23 First indication for strong CP violation in the lepton sector ? New results 2013

24 NOVA CP phase δ Perspectives Perspectives

25  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

26  High power accelerator and huge detector needed  Asymmetry of neutrino and anti-neutrino induced by interaction in matter is large

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28 Measurement of  13 C=cos S=sin

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30 Merci beaucoup Joe !


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