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Comment la matière a-t-elle évolué juste après le big bang ? WMAP Wilkinson Microwave Anisotropy Probe ∑mν < ( 1.6 − 3.1) eV (95% CL) FAAQ2006 Alain Bellerive 96
Conclusion • Plusieurs défis en astrophysique des particules • Le neutrino en est un bon exemple • Futur: ATLAS - SNOLAB - ILC • Plusieurs applications en haute technologie • Opportunités pour les jeunes (et les moins jeunes) scientifiques FIN FAAQ2006 Alain Bellerive 97
Page 1 and 2:
Le neutrino, particule fantomatique
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Les grandes questions du 21 ième s
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The First Piece: - Fundamental Forc
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Scope of Particle Physics FAAQ2006
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History of the Neutrino • Disover
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Elementary Particles electron & neu
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Open Questions in Neutrino Physics
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2) Underground laboratories: e.g. S
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Electroweak Interactions L ( em NC)
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• Define a quark mixing matrix wh
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Evidence for Neutrino Oscillations
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Macroscopic Properties of the Sun M
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Neutrino Production in the Sun Ligh
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Solar Neutrino Experiments • Revi
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Chlorine Measurements: Homestake (U
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Gallium Measurements: SAGE (on-goin
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Water Detector: Super-Kamiokande (J
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Solar ν Flux Measurement Results C
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Solar Neutrino Problem • Historic
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Neutrino Oscillations Neutrino Stat
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Solar Neutrino Oscillations P ee =
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Matter-Enhanced Neutrino Oscillatio
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