PPT-New Physics and Neutrino M

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. 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.. Susan Cartwright. University of Sheffield. Introduction: . Massive neutrinos in the Standard Model. Dirac and . Majorana. masses. The mixing matrix and neutrino oscillations . Massive neutrinos in the . 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 . 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?. –. . COBAND. . Experiment –. Continuous. . Spectra. l. . Measurement. . in Far-Infrared Region using STJ. Shin-Hong Kim. 　. （. University of Tsukuba, . TCHoU. ）. for COBAND collaboration. 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 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. 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 . General Presentation – Zagreb (Croatia) – 23. rd. of October – 11h00 - 12h30. The Chair, Tord Ekelöf. Aysel. . Kayis. . Topaksu. Marcos Dracos. Georgios . Fanourakis. Eliane Bouquerel. Marie-Laure Schneider. 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. Learn how to excel in AP Physics with this comprehensive guide. Explore essential concepts, study strategies, and resources to ace your AP Physics exam.