PPT-Review of Linear Algebra Applications in Some Neutrino Experiments

Xin Qian BNL 1 Introduction Linear Algebra LA has a very long history First appears in The Nine Chapters on the Mathematical Art Systematically i ntroduced by Rene Descartes Application of LA is very broad. 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.. 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 . 25/09/2014. Day 1 review. Neutrino Cryogenics Requirements Meeting. 25/09/2014. Good / open presentations. Neutrino Cryogenics Requirements Meeting. 25/09/2014. Points to be discussed further:. Maximum temperature gradients allowed in the sensitive volume. (what is that?). What . is linear algebra? Functions and equations that arise in the "real world" often involve many tens or hundreds or thousands of variables, and one can only deal with such things by being much more organized than one typically is when treating equations and functions of a single variable. Linear algebra is essentially a ". 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 . . . 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. 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. 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,. in collapsing phase. ～. towards comprehensive neutrino studies . Waseda. . univ.. . Yamada lab.. D1 Chinami Kato. Collaboration with . S. Yamada(. Waseda. ), H. . Nagakura. . (Caltech), W. . Iwakami. PPAP Meeting. Birmingham. 15 July 2009. Elisabeth Falk. University of Sussex. Def. current: running or under construction. Outline. Neutrino-oscillation experiments:. what to measure, and how. Accelerator-based experiments. Xiaomei. Zhang. IHEP Computing . Center. Outline. Overview of IHEP experiments. General Challenges . Challenges and practice of software. JUNO Neutrino experiment . Status and challenges of computing. 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 .