PPT-The Neutrino Anomalies NS2016

Outline The 3 n oscillation framework The current 4 anomalies that dont fit this framework LSND MiniBoone The Gallium Anomaly The Reactor Neutrino Anomaly Summary The majority of experimental results on . Naba. K . Mondal. Tata Institute of Fundamental Research. Mumbai 400005, India. Brief History. Atmospheric neutrino experiments study neutrinos produced by cosmic ray interactions in the atmosphere.. 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. mass. Stuart . Freedman memorial symposium. Berkeley, Jan 11, 2014. Hamish Robertson, University of Washington. a long wait for a little weight. 2. Neutrinos oscillate, have mass. Super-. Kamiokande. COSMOLOGY. EVIDENCE FOR NEW PHYSICS?. STEEN . HANNESTAD, Aarhus . University. NuHorizons. 2011. n. e. n. m. n. t. Fermion Mass Spectrum. 10. 100. 1. 10. 100. 1. 10. 100. 1. 10. 100. 1. Alan Bross. N u F a c t 0 9. From . SuperBeams. to Neutrino Factories. Pre-Ramble. Neutrino Factory means different things to different people. Not so much for . SuperBeams. I will be talking about a muon-based Neutrino Factory as opposed to a . ass: Facts and Fancy. Francesco Vissani. LNGS and GSSI. Introduction. Baryon and lepton numbers and their status in the standard model of particles and interactions. L. epton and baryon number. In all known transformations among particles,. Essential 4 - Anomalies v2.0, August 31, 2012. Who’s Supposed to Be Here. Individuals . a. ssigned to. CALPADS maintenance. Supervisor of staff. assigned to CALPADS. 2. Essential 4 - Anomalies v2.0, August 31, 2012. –. . COBAND. . Experiment –. Continuous. . Spectra. l. . Measurement. . in Far-Infrared Region using STJ. Shin-Hong Kim. 　. （. University of Tsukuba, . TCHoU. ）. for COBAND collaboration. 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 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. 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