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Bartol and Honda fluxes. Zenith angle distribution(1D) For En a few GeV, ... Best fit (Dm2=2.0x10-3eV2, sin22q=1.00) Sub-GeV muti-ring m-like sample ...
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Title: Results in Neutrino Oscillations from Super-Kamiokande I Author: mini Last modified by: mini Document presentation format: (4:3)
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The Search for Proton Decay at Super-Kamiokande ASTR-007 Theodore Liu Proton Decay overview Protons not infinitely stable, as once thought Required for grand ...
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How to solve the octant degeneracy? H. Minakata, T2KK06 ... Octant of q23. not resolved. Mass hierarchy not determined ... Octant ambiguity of q23 can be ...
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Recent results of atmospheric observation in SuperKamiokande
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... counted in proportional counters (using additional information on ... Rate = 0.48 0.16(stat) 0.03(syst) argon atoms/day. Flux = 2.56 0.16 0.16 SNU ...
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The Ghostly Neutrino Steve Boyd, University of Warwick JPARC Facility JPARC Facility TARGET nm 295 km Super-Kamiokande nm ne Super-Kamiokande Water Cerenkov Electron ...
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Also probe with 'long baseline' accelerator and reactor experiments ... First 'long baseline' accelerator experiment. Beam from KEK PS to Kamiokande, 250 km away ...
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Test exotic models (decay, extra dimensions,....) Sign of ... Designed and optimized after the knowledge of Super-Kamiokande/K2K results. Primary goal: ne app. ...
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Interaction Meeting on Linear Collider and Neutrino Physics. Delhi, India. Nov 12, 2003 ... A large detector of mass 500 kT natural extension of Super Kamiokande. ...
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It is apparently stable, but its mass and coupling strength are not yet known. ... 10 kpc away from us goes off, and 3,000 events are observed in Super-Kamiokande. ...
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... zenith angle. Oscillation to e = See excess of e vs zenith ... Deficit of vs zenith angle. Super Kamiokande Results. Interpreted as. Neutrinos from the Sun ...
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Mont Blanc neutrino telescope 1987. Kamiokande neutrino telescope 1987. Hirata et al. ... Mont Blanc 1:45 - 3:45 ( 5-neutrinos at 2:56 U.T.) F 1.2 (second) n. C(-1.1) ...
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Alec Habig, Univ. of Minnesota Duluth. For the Super-Kamiokande Collaboration. July 29, 2003. Alec Habig, Chiba UHE v Telescope Workshop. S. K. Upward-going m ...
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To date, the only astronomical source beside the Sun to be observed in neutrinos ... Mistery: 5 events in Mt. Blanc ~5h earlier. 11 Kamiokande events and 8 IMB events ...
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Neutrinos from supernova and gamma-ray burst. Long baseline K2K neutrino experiment ... Gamma Ray Bursts (GRB) Search for neutrinos correlated with 1371 GRBs ...
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Title: Prototype Design for SK trigger upgrade Author: DengZhi Last modified by: Shaomin Chen Created Date: 8/3/2005 1:44:02 AM Document presentation format
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Guido Pizzella. Universita' di Roma Tor Vergata. INFN- Frascati. SN1987A revisited. May the Supernova Bang more than ... Galileo nel 1612 a Federico Cesi. end ...
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Il mistero dei neutrini Gilardoni Simone CERN - PS/PP Division Universit de Gen ve - DPNC Perch i neutrini? (prologo...) I neutrini solari: reazione di fusione ...
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For more details, see my review article; 'Observational Neutrino Astrophysics' ... of Cerenkov photons, while the bottom m-event has a crisp ring image. ...
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neutrino puzzles Ulrich Heintz Boston University http://physics.bu.edu/quarknet/2002/neutrinos.ppt outline the neutrino atmospheric neutrinos solar neutrinos ...
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Neutrino Jeopardy - University of Minnesota ... Neutrino
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Frontiers in Neutrino Astrophysics
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Collaborators: John Beacom, Manoj Kaplinghat, Gary Steigman, ... Gadolinium Enhanced Super-K (GADZOOKS!) Neutron Tagging. Reduction of Invisible Muon Background ...
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The Solar Neutrino Problem Barbara Sylwester Zak ad Fizyki S o ca CBK PAN One page story - the short story Fusion reactions in the core of the Sun produce a huge ...
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ne appearance search Yoshihisa OBAYASHI (KEK - IPNS) nm to ne oscillation search Three Active Neutrino & Mass Degeneration Scenario (Dm212
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A Yu Smirnov ''... annus mirabilis'' Ceremony of the Nobel Prize award: ``for pioneering ... `First Results from KamLAND: Evidence for Reactor ...
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Double Beta Decay and Neutrino Masses Amand Faessler Tuebingen 1. Solution of the Solar Neutrino Problem by SNO. 2. Neutrino Masses and the Neutrinoless Double
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Discovery of oscillation of atmospheric neutrinos (1998) ... Construction of SciFi. Cher. light calibration. Particle identification. PhD student on site ...
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Production of atmospheric neutrinos
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How neutrinos fit into the 'Standard Model' Grand ... Clyde Cowan. Fred Reines. Reines and Cowan's neutrinos produced in reaction: Observed reaction was: ...
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(a) Israel Cosmic Ray and Space Weather Center and Emilio Segre' Observatory, ... and the total correlation for 1970 1994 became very weak (Walther, 1999) ...
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Weak interactions, P, C and CP Introduction Need of neutral currents Electroweak and Higgs Parity in weak interactions Helicity of the neutrino, C and CP
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The 1st long baseline n experiment. Atmospheric n. Discovery of nm oscillations ... 50,000 ton water Cherenkov detector (22.5 kton fiducial volume) ...
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F.Pierre - neutrino-France - 27 novembre 2003 K2K et JPARC-? ... JHF-? adopte le principe du faisceau angle : 44. F.Pierre neutrino-France - 27 ...
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He was so unsure of this that he didn't even name his own particle. ... If you were in a Jupiter-type orbit a billion kilometers from SN1987A when it ...
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Oscila o de neutrinos em neutrinos de reactores (KamLAND), aceleradores (K2K) y atmosf ricos (S_K). Telesc pios de neutrinos (AMANDA, IceCube) ...
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LeptonPhoton 2003 Plenary Talk
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Super Beam Experiments
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LeptonPhoton 2003 Plenary Talk
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Antiparticles. 18. Standard model. 3 families of particles. 4 fundamental forces ... if the neutrino is its own antiparticle (like the photon, but different from the ...
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Big World of Small Neutrinos
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System division makes streak camera, high resolution digital camera, oxygen monitor for premature baby and so on. This picture shows body line scanner, ...
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Title: 1 Author: Last modified by: Koichiro Nishikawa Created Date: 3/19/2006 7:42:20 AM Document presentation format
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Neutrino Flux is almost the same between and beams. q. Target. Horns ... Only the difference of rs,re between neutrino and anti neutrino appear in the asymmetry ...
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speziell gegen dem Ende zu. W.A. Kamioka. neutrinos from upper atmosphere. SNO. Sudbury ... Atmospheric angle about 40 degrees. Neutrinoless double beta decay: ...
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Title: PDP for NSS Phys. Curriculum: The Stars and the Sun II Subject: Basic properties of the sun Author: Chu Ming-chung Last modified by: PHY Created Date
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1. The OPERA emulsion detector for a. long-baseline neutrino ... nm CC st/sm et x BR evert. sin2 2qmt ( large Dm2 ) 2 x 2.3 / (14930 x 0.48 x 0.36 x 0.90) ...
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Photons are created in the nuclear fusion cycle. ... The loops rising into the chromosphere or corona may appear as solar prominences. ...
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1920 Nuclear Astrophysics is born with Sir Arthur Eddington remarks in his ... (Rolfs and Rodney) 18. Electron capture decay of 7Be. Why electron capture: QEC=862 keV ...
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DESIGN AND CONSTRUCTION OF A MODULAR MASSIVE DETECTOR AT THE HOMESTAKE LAB
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The 'Dark Side' of solar neutrinos. Two 'flavors' are involved in ... HERON. CC. 60 t In load in scint. LENS ~250 keV. ES ~600 t liq scint. KamLAND ~250 keV ...
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Title: Disegno del sistema generale di trigger dell esperimento ICARUS, progettazione e realizzazione della scheda di primo livello Author
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Dustmaids Down a Drafty Hall: Neutrinos at the Sudbury Neutrino ... by John Updike. In. Telephone Poles. And. Other Poems (1960) e- n. Detecting Neutrinos ...
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Fermilab, May, 2003
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