1. MiniBooNE 2. Beam 3. Detector MiniBooNE Anomaly and Nuclear physics 4. Oscillation 5. Discussion PRL121(2018)221801 outline 1. MiniBooNE neutrino experiment 2. Nucleon correlations 3. Pion puzzle 4. NC single photon production 5. Conclusions Teppei Katori Queen Mary University of London ECT* workshop, Trento, Italy, April 15, 2019 Teppei Katori,
[email protected] 15/04/19 1 1. MiniBooNE 2. Beam 3. Detector 4. Oscillation 5. Discussion 1. MiniBooNE neutrino experiment 2. Nucleon correlations 3. Pion puzzle 4. NC single photon production 5. Discussions Teppei Katori,
[email protected] 15/04/19 2 1. MiniBooNE 2. Beam 3. Detector 4. Oscillation 5. Discussion Teppei Katori,
[email protected] 15/04/19 3 1. MiniBooNE 2. Beam 3. Detector 4. Oscillation 5. Discussion The most visible particle physics result of the year Teppei Katori,
[email protected] 15/04/19 4 https://physics.aps.org/articles/v11/122 PHYSICAL REVIEW LETTERS 120, 141802 (2018) signature of dark matter annihilation in the Sun [5,6]. 1. MiniBooNE Despite the importance of the KDAR neutrino, it has never MiniBooNE 2. Beam been isolated and identified. 3. Detector 86 m 4. Oscillation In the charged current (CC) interaction of a 236 MeV νμ background KDAR 12 − NuMI 5. Discussion (νμ C → μ X), the muon kinetic energy (Tμ) and closely beam decay pipe related neutrino-nucleus energy transfer (ω E − E ) horns ν μ target distributions are of particular interest for benchmarking¼ absorber neutrino interaction models and generators, which report widely varying predictions for kinematics at these tran- 5 m 675 m sition-region energies [7–14].