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Borexino detects CNO neutrinos Experimental evidence of neutrinos produced in the CNO fusion cycle in the Sun
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Overview of Neutrino Physics Challenges - Alexander Friedland
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- 1 Intro
- 2 A few basic observations upfront
- 3 T2K claims signs of CPV Constraint on the matter antimatter symmetry violating phase in neutrino oscillations
- 4 Borexino detects CNO neutrinos Experimental evidence of neutrinos produced in the CNO fusion cycle in the Sun
- 5 IceCUBE sees the Glashow resonance Detection of a particle shower at the Glashow
- 6 KATRIN reports the latest neutrino mass limit
- 7 Discovery era precision era
- 8 Goal: precision studies of neutrino oscillations as a function of energy
- 9 Measuring neutrino energy at DUNE/NOVA
- 10 Calorimetry challenge
- 11 Does this really matter for oscillation measurements?
- 12 Electron scattering tests
- 13 Decisive test: comparison to hydrogen and deuterium
- 14 MINERVA experiment sees corresponding problems in neutrinos for all generators Model variations and generator predictions
- 15 Needed: solid theoretical framework
- 16 Another ingredient is the nucleon axial FF
- 17 Putting experiments together: NOVA vs T2K appearance tension
- 18 A gravity-powered neutrino bomb
- 19 SN v oscillations: physics cartoon
- 20 Next galactic supernova at DUNE and Hyperk
- 21 Interested? KITP Neutrino22 program
