PPT-Neutrino-induced meson production model

for neutrino oscillation experiments Satoshi Nakamura Nuclear Theory Group Contents Introduction nN scattering for neutrino exp Dynamical coupledchannels DCC model for . 林貴林. IOP, NCTU. (1). F.-F. Lee and GLL, Phys. Rev. D85, 023529 (2012). (2). F.-F. Lee, GLL, . Sming. Tsai, Phys. Rev. D87, 025003 (2013). (3). . . F. .-F. Lee, GLL, . Sming. Tsai, . Phys. . Rev. D89, . 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 . CLAS and CLAS11. Paul Stoler-RPI. Measure . electroproduction. of mesons above the. resonance region (W > 2 . GeV. ) over a large range of. of . Q. 2. and . t. in the valence quark region of . x. 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. 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. Dan Watts. University of Edinburgh. Outline. Many proton knockout. Nuclear tagging using nuclear gamma decay photons. Recoil nucleon spin . polarimetry. – first crude look at possibilities. Many nucleon knockout from nuclei. 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?. 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,. 孙宝玺. . 北京工业大学. . . 合作者. : . 吕晓夫 四川大学. . . FHNP’15. String Fragmentation in the Exclusive Limit. Mac . Mestayer. 1. Does the quark model work for exclusive production?. - compared to an hadronic current approach.. What are ‘constituent quarks’?. What is the ‘flux-tube’?. 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 Maurizio . Spurio, . maurizio.spurio@unibo.it. . Università. di Bologna e INFN. 1. M. Spurio - Galactic template neutrino searches. Propagation induces accidents. M. Spurio - Galactic template neutrino searches.