Neutrino experiments

• 14.1 Nuclear reactors : KamLAND, Double-Chooz, Daya Bay, RENO………………………………………………………………………………..114
  • 14.1.1 Long baseline: KamLAND, $\mathbf{\delta m^2_{21}}$, $\mathbf{\theta_{12}}$…………………………………………………….114
  • 14.1.2 Short baseline: Double-Chooz, Daya Bay, RENO, $\mathbf{\delta m^2_{31}}$, $\mathbf{\theta_{13}}$…………………………………115
• 14.2 Neutrinos from accelerators: T2K, NO$\nu\!$A and OPERA~; $\mathbf{\delta m^2_{32}}$, $\mathbf{\theta_{23}}$, $\mathbf{\delta}$…………..116
• 14.3 Atmospheric neutrinos: Super-Kamiokande~; $\mathbf{\delta m^2_{32}}$, $\mathbf{\theta_{23}}$, $\mathbf{\delta}$………………………….120
• 14.4 Solar neutrinos: SNO~; $\mathbf{\delta m^2_{12}}$, $\mathbf{\theta_{12}}$……………………………………………………………..124
• 14.5 Ultra-high energy or cosmic neutrinos…………………………………………………………………………………………………129
• 14.6 Problems?………………………………………………………………………………………………………………………….135
• 14.7 Neutrinos: conclusions………………………………………………………………………………………………………………137

This lecture can be downloaded here (last change 7 Feb 2020)