PPT-Reactor Neutrino Results

Jun Cao Institute of High Energy Physics ICHEP Melbourne July 11 2012 Neutrino Mixing 23 45 Atmospheric Accelerator 1 2 34 Solar Reactor 0 1 3. J. Brunner. 17/04/2013. APC. Outline. Oscillation Probabilities. Neutrino Cross Sections. The Proton Accelerator . The Neutrino Beam. Detector Performance. Event Rates / Result. Oscillation Probabilities. 1. May, 5th 2015. Vertical/. Floor. . big. . beams. . connection. with. an angle . stiffener. Neutrino. 2. May, 5th 2015. Vertical/. Floor. . big. . beams. . connection. with. an angle . stiffener. R. e. l. d. The. d. i. A. Yu. Smirnov. Max-Planck Institute. for Nuclear Physics,. Heidelberg, Germany . NOW 2014 . September 8– 13, 2014 . . The riddle of neutrino mass:. strongly suppresses . . . Neutrinos Are Very Elusive!. We now understand that neutrinos are produced in nuclear reactions, but they were actually . predicted several decades before they were finally discovered. . O. n what basis was that prediction made?. t. elescope . Simone . Biagi. on behalf of the ANTARES collaboration. INFN, . Laboratori. . Nazionali. del . Sud. RICH 2016 – Bled 8 Sept 2016. ANTARES: the largest Northern neutrino telescope. Scientific goals. Neutrino Oscillations in Susan Cartwright Neutrino Oscillations Principles Experimental techniques Neutrino oscillations: Principles The Standard Model contains three neutrinos These can be labelled by flavour as Are we close to measuring the neutrino hierarchy? Filipe B. Abdalla ν Loureiro , Moraes , Abdalla et al. arXiv:1809.07204 Loureiro , Cuceu , Abdalla et al. arXiv:1811.02578 Outline Cosmology background 1. The basis of the potential of . muon. beams. Muon. mass:. 200. . m. e. ~ . m. m. ~ 0.1. . m. p. Muon. decay:. n. e. , . n. m. Precisely known energy spectrum. Energy frontier:. No . brem. -/beam-. Mandate. “Rapid progress in neutrino oscillation physics, with significant European involvement, has established a strong scientific case for a long-baseline neutrino programme exploring CP violation and the mass hierarchy in the neutrino sector. CERN should develop a neutrino program to . properties from COHERENT elastic neutrino - nucleus scattering Speaker: Yiyu Zhang Institute of High Energy Physics, CAS 2021/3/16 Yiyu Zhang IHEP 1 M. Cadeddu et al. Phys.Rev.D 102 (2020) 1, properties from COHERENT elastic neutrino-nucleus scatteringSpeakerYiyu ZhangInstitute of High Energy Physics CAS2021/2/19Yiyu Zhang IHEP 1M Cadedduet al PhysRevD10220201015030Based on a work in http://www.darkenergysurvey.org. . . . Outline. DES: what is it and update + probes used. Dark energy from DES.. Neutrino masses from DES. Filipe . Batoni. . Abdalla. Future Dark Energy Surveys. 1. John Beacom, The Ohio State University. High Energy . Neutrino . Astronomy. Topic: Impossible. Requires. : sources that reach high energies. . sources that are luminous. . sources of different types. Outline. The 3. n. oscillation framework. The current 4 anomalies that don’t fit this framework. LSND. MiniBoone. The Gallium Anomaly. The Reactor Neutrino Anomaly. Summary . The . majority of experimental results on .