PPT-Are we close to measuring the neutrino hierarchy?

Are we close to measuring the neutrino hierarchy Filipe B Abdalla ν Loureiro Moraes Abdalla et al arXiv180907204 Loureiro Cuceu Abdalla et al arXiv181102578 Outline Cosmology background. 1 716 60 382 16 73 18 18 20 25 D4110 98 91 58 10 45 14 29 D4111 47 279 241 170 22 92 12 32 D4112 315 851 213 428 121 276 37 80 D4117 947 2358 1105 1357 647 823 95 493 86 86 D4124 283 494 152 358 173 499 296 3471 35 35 D4125 381 754 74 304 17 140 83 O 1 716 60 382 16 73 18 18 20 25 D4110 98 91 58 10 45 14 29 D4111 47 279 241 170 22 92 12 32 D4112 315 851 213 428 121 276 37 80 D4117 947 2358 1105 1357 647 823 95 493 86 86 D4124 283 494 152 358 173 499 296 3471 35 35 D4125 381 754 74 304 17 140 83 O Oscillations. Collective Neutrino Oscillations. Georg G. Raffelt. 3. rd. Schr. ödinger Lecture, Thursday 19 May 2011. Neutrino Oscillations in Matter. 3300 citations. Lincoln Wolfenstein. Neutrinos in a medium suffer . Satoshi Nakamura. Osaka University, Japan. Collaborators : H. . Kamano. (RCNP, Osaka Univ.), T. Sato (Osaka Univ.). T.-S.H. Lee (Argonne Nat’l Lab). Contents. Introduction . 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. 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. 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 . 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 . 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. 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,. 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-. Jun Cao. Institute of High Energy Physics. Gordon Research Conference on “New . Tools for the Next Generation of Particle Physics and . Cosmology”, HKUST, Hong Kong, Jun.30-Jul.4, 2019. Neutrino Mixing. will we ever know?. Ray Volkas. School of Physics. The University of Melbourne. CERN Theory Colloquium at “Neutrinos: the quest for a new physics scale”, 29 March 2017.. What we know, don’t know and want to know.. 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.