PPT-Origin of neutrino mass:

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 dont know and want to know. 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 . Arman Ballado. Advisor: Mike Miller. Neutrino mass measurement. Beta Decay .  . Griffiths. Tritium Beta Decay . Endpoint energy of 18.575 . keV. J.A. . Formaggio. . Project 8 Concept. Use cyclotron frequency to measure energy . 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. 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 . . . 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. 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,. 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-. 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.