PPT-Current * Neutrino Oscillation Experiments

PPAP Meeting Birmingham 15 July 2009 Elisabeth Falk University of Sussex Def current running or under construction Outline Neutrinooscillation experiments what to measure and how Acceleratorbased experiments. 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 . 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 . MINERvA is studying neutrino interactions in unprecedented detail on a variety of different nuclei. Low . Energy (LE) . Beam Goals: . S. tudy . both signal and background reactions relevant . to oscillation experiments (current and future). Beta Beam: timetable and cost. EUROnu. meeting Paris 12-15 June. 2012-15-05. 1. European Strategy for Neutrino Oscillation Physics - II, Elena Wildner. 1. We consider the lengthiest item to define the time line . MiniBooNE. Robert . Cooper. 3-Flavor Neutrino Mixing Model. Mass . splittings. D. m. 21. 2. . ≅. . 7.6 × 10. -5. e. V. 2. . D. m. 31. 2. . ≅. 2.4 . × 10. -3. e. V. 2. Mixing angles. Exclude Light Majorana Neutrinos?. http://. physics.princeton.edu. /~. mcdonald/examples/majorana.pdf. KT . McDonald. Princeton U.. . (October 21, 2016). Sun . Yat. -Sen University. Guangzhou. Beta Decay. J WU, T Koettig, P Janickova, L . Zwalinski. Oscillation of the pump discharge pressure. Pressure [Bar]. At certain low discharge pressure of the pump, there is no oscillation. With increase of the pressure, the oscillation starts. The frequency of the oscillation is about . 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 Past and Present. Art McDonald. Queen’s University. And. SNOLAB. 1940’s to 1960’s:. Neutrino oscillations were proposed by . Pontecorvo. in 1957 motivated by initial reports of measurements by Davis with a Chlorine detector at a reactor. At that point, the transitions being considered were electron neutrino to electron anti-neutrino.. in Japan. T. Ishida. Neutrino Section, J-PARC Center, KEK. on behalf of the neutrino beam group . 1. Contents. Neutrino experimental facility at J-PARC. S. tatus of the facility since NBI2012. . Physics reach of T2K / J-PARC to Hyper-K. and . Simultaneous . Estimation of . Forced . Oscillations and . Modes. John . Pierre, U of Wyoming. pierre@uwyo.edu. Dan . Trudnowski. , Montana Tech. dtrudnowski@mtech.edu. Jim Follum, PNNL (formerly at U of Wyoming). 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 . Joint Session, Snowmass Energy Frontier. Jonathan Feng, UC Irvine, 8 July 2020. F. ORWARD . P. HYSICS . F. ACILITY. As the LHC extends the energy frontier to higher energies and much higher luminosities in the coming 15 years, how can its physics potential be maximally exploited?.