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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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T2K (Tokai to Kamioka Neutrino Oscillation Experiment) ... Experiences in K2K with Harp measurement. 11. Muon monitors @ ~140m ...
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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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LS only. Used for detecting gammas from prompt and delayed events. Double Chooz. Buffer ... Kamioka Mine in northwestern Japan (main island) Spherical geometry ...
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Title: PowerPoint Presentation Author: ESR Last modified by: ESR Created Date: 1/1/1601 12:00:00 AM Document presentation format: (4:3)
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Dark Matter Search with Direction Sensitive Scintillators The10th ICEPP Symposium February 16, 2004, Hakuba H. Sekiya University of Tokyo
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Fermilab, May, 2003
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T2KK sensitivity as a function of L and Dm2. Kimihiro Okumura (ICRR Univ. of Tokyo) ... Fanny's talk. Improvement of analysis method ...
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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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Extend to make MC calculation more efficient, but do not want to extend in ... Shortcut in 1D, since ?P = ?D, generate primaries flat in cos?P, weight by cos?P ...
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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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Title: KLG4sim: A Full Monte Carlo Simulation for KamLAND Author: Lauren Hsu Last modified by: Lauren Hsu Created Date: 6/19/2005 1:56:37 PM Document presentation format
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The Latest Status of the KAGRA Cryogenics N. KIMURA A, D. CHEN B, T. KUME A, S. KOIKE A, Y. SAKAKIBARA B, T. SUZUKI A, C. TOKOKU B, K. YAMAMOTO B, M. OHASHI B, and K ...
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Establish 3 flavor framework (or find something new) Discovery ... Give hint on Matter/Anti-matter asymmetry in the universe. What's super muon-neutrino beam? ...
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Big World of Small Neutrinos
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Physics with Neutrinos ICU Nov'12th, 2003
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n from decay of p, K and m produced by interactions of cosmic rays in the atmosphere ... Bending of muons in geomagnetic field important for n from m decay ...
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Title: PowerPoint Presentation Author: ohtani Last modified by: Ohtani-Pana Created Date: 1/1/1601 12:00:00 AM Document presentation format: (4:3)
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456789:CDEFGHIJSTUVWXYZcdefghijstuvwxyz GpSs tFTO Z ... ( ( ( ( ( ( ( ( ( ( ( ( ( ( ( ( ( ( ( ( ( ( ( ( ( ( ( ...
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PN junction in epitaxy layer provides a depletion region with high electric field where Geiger mode discharge occurs with incoming photons.
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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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M.Levi. B. Cortez. G.W. Foster. Location: Harvard. Michigan. IMB Collab. Proposal. Construction ... Site selection : Morton Salt Mine outside Cleveland ...
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Title: PowerPoint Presentation Last modified by: hiro Created Date: 1/1/1601 12:00:00 AM Document presentation format: Other titles
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Title: Development of photodetection system based on multipixel avalanche Geiger photodiodes with WLS for Lxe low-background detectors Author:
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K2K and JHF near detectors. NuFact02, July 2002, London. Takaaki Kajita, ICRR, U.Tokyo ... Fraction of non-quasi-elastic events must be understood well. 1kton ...
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1. NOvA experiment. Teppei Katori, Indiana ... 2 goals for T2K and NOvA experiments ... MiniBooNE (Mini-Booster Neutrino Experiment) status: ongoing - ~800MeV ...
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LENA LENA Delta Low Energy Neutrino Astrophysics EL SUD Meeting Garching, April 24th L. Oberauer, Technische Universit t M nchen www.e15.physik.tu-muenchen.de ...
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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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Super Beam Experiments
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constellation Cygnus. (R.A. 21h12.0', Dec 48.19 ) WIMP ... ( Cygnus )and the galactic center ( Sagittarius ). Set the crystals on the. driving system like ...
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Detection of the Diffuse Supernova Neutrino Background in LENA & Study of Scintillator Properties E15 Michael Wurm DPG Spring Meeting, 30.3.06 Neutrinos from ...
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SIP. SIP. SIP. SIP. SIP. SIP. SLP. SLP. Based on the 3GPP specification. 10 ms. Constant. Processing Time in MT ...
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In the Quark Sector, CP is violated. Then, also in the Lepton Sector? Leptogenesys ... CP Measurement is a final goal of flavor physics. Dec. 13, 2001 ...
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... V V V V V V V V V V V V V V V V V V V V V V V V V V V V V V V ... 456789:CDEFGHIJSTUVWXYZcdefghijstuvwxyz GpSs tFTO ...
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Getting the most in neutrino oscillation experiments
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Largest low-energy anti-neutrino detector built so far ... Photosensitive coverage ~ 34% 3mm thick acrylic wall: Rn barrier. Water Cherenkov outer detector ...
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Status of TAMA data analysis Hideyuki Tagoshi (Osaka Univ.) on behalf of the TAMA collaboration Data taking run (1) - Observation runs - Inspiral analysis (1 ...
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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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Title: Cosmic-ray spectrum and compositionmeasurement by direct Author: Toru SHIBATA Last modified by: Toru SHIBATA
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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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Low background gamma spectrometry at the Laboratoire Souterrain de Modane The LSM laboratory HPGe detectors development at LSM LSM HPGe detectors s performance
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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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Prospects for 7Be Solar Neutrino Detection with KamLAND
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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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Title: T2K Near Detector SiPM Author: Last modified by: Created Date: 9/2/2005 4:28:11 AM
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High Energy Physics in Japan from KEK point of view
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MRD and SciFi: Fine Grained Precise ? Detector. MRD: Massive and Large Solid Angle ? Detector ... SciFi. Lead Glass. Muon Range Detector. Front Detector as ...
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The n Odyssey 2002: SNO
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Development of a 100-W,single-frequency Nd:YAG laser for large-scale cryogenic ... 2003 Friedrich-Schiller (MOPA,118W) 2004 LZH (87W) ...
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SNO Liquid Scintillator Project NOW 2004 17 September 2004 Mark Chen Queen s University & The Canadian Institute for Advanced Research Fall 04 to Dec 06: SNO Phase ...
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Big World of Small Neutrinos
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A lot of baffles are put inside the tubes to block the scattered light in large ... Scattered light noise with baffles 4x10-22 m/Hz1/2 (margin: 150) ...
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Title: NEUTRINO MASSES AND OSCILLATIONS Triumphs and Challenges Author: BMCK Last modified by: Robert McKeown Created Date: 3/29/2004 6:59:07 PM Document presentation ...
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Goals for the future. Establish q13 non-zero. Measure CP ... Subdominant 13 Oscillation. ne Disappearance. Reactor Experiment Sensitivity (Huber et al. ...
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RECENT RESULTS IN K2K EXPERIMENT Shimpei YAMAMOTO (Kyoto Univ.) 10th ICEPP Symposium @Hakuba 16-FEB-2004
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