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Results in Neutrino Oscillations from SuperKamiokande I
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Results in Neutrino Oscillations from SuperKamiokande I
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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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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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Recent results of atmospheric observation in SuperKamiokande
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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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Nuclear reactions Using the strong nuclear force to produce useful energy Micro-world Macro-world Lecture 17 Strong Nuclear Force It is very strong It overcomes the ...
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... dei neutrini Nel 1940 Pontecorvo aveva applicato gli studi svolti nel gruppo di Roma inventando il neutron log uno strumeno ancora oggi usato per le ...
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D, 3He, 4He and 7Li primordial abundances. abundances range over ... LEP (Aleph) from 2939 events 2 22.3 MeV/c2. and 52 events 3 2 ( ) 21.5 MeV/c2 ...
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Title: PowerPoint Author: masaaki Last modified by: Iye Created Date: 8/1/2001 4:09:57 PM Document presentation format
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Big World of Small Neutrinos
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Licence de Physique Universit des Sciences Montpellier II PLAN TES ET EXOBIOLOGIE module Culture g n rale cours IV Etoiles Pr. Denis Puy
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INT & UW department of Physics, Seattle ... Subdominant effects calculable (in part): q13, 'solar' parameters, emt, 3-neutrino effects, ...
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1960's muon neutrino observed, V-A physics & neutrino oscillations suggested ... The sun does not shine without Antimatter. 6. Solar Neutrino Experiments ...
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Title: Slide 1 Last modified by: pcpaoloni2 Document presentation format: Custom Other titles: Times New Roman Nimbus Roman No9 L HG Mincho Light J;MS Gothic;HG ...
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MiniBooNE and NuMI Why do they need so many protons? Eric Prebys Fermilab Accelerator Division/MiniBooNE
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Why should neutrinos oscillate? How can we search for neutrino oscillations? What is the Main Injector? How do we search for neutrino oscillations in MINOS?
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The Fermilab Neutrino Program Status and Challenges Ahead Eric Prebys* Fermilab Accelerator Division/MiniBooNE *with acknowledgements to everyone who leaves talks ...
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... scraper collimators and beam dump Slow resonance extraction for K-ARENA (Nuclear and Physics ... Length 0.7 m Number 72 Quadrupole Magnet (11 families ...
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The European Long Baseline Program Les Houches, 21 June 2001 Dario Autiero CERN/EP nm nt ? Many thanks to A. Rubbia for providing material about ICARUS
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Gravitational Wave Detectors Course in Inflation, Structure formation and CMB 7 November 2002 Silvio Orsi GW: My presentation GW production Upper bounds on GW ...
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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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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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Title: A Deep Ocean Anti-Neutrino Observatory Subject: Hanohano Author: John Learned Last modified by: John Learned Created Date: 9/4/2006 1:57:58 AM
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Cosmogenic isotopes. 214Bi and 208Tl from 238U and 232Th bulk contamination. Raw Spectrum ... Residual short-lived cosmogenic rate: 3x10-3 c/d. Dead-time: 23.4 ...
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Title: iThemba 25-11-05 Author: Rob de Meijer Last modified by: Software Group Created Date: 10/20/2004 12:52:25 PM Document presentation format: On-screen Show
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Bezneutrinowy podw jny rozpad b (lata 30) Maria Goeppert-Mayer: s j dra parzysto-parzyste, ... Maria Fia kowska Last modified by: DSW Created Date:
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At these temperatures, nuclear fusion can occur which transforms 4 Hydrogen ... Located in the Gran Sasso laboratory (LNGS) in Italy. ...
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1960's muon neutrino observed, V-A physics & neutrino ... Gallium. John Bahcall. The sun does not shine without Antimatter. 6. Solar Neutrino Experiments ...
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MiniBooNE: Status and Prospects Eric Prebys, FNAL/BooNE Collaboration
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Galactic Supernova neutrino detection with Lena. Electron Antineutrino spectroscopy ... Geo - neutrinos and LENA. what is the source of the terrestrial heat flow ? ...
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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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Title: No Slide Title Author: smirnov Last modified by: Gigliola Gori Created Date: 3/19/2002 2:01:14 AM Document presentation format: On-screen Show
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Big World of Small Neutrinos
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DESIGN AND CONSTRUCTION OF A MODULAR MASSIVE DETECTOR AT THE HOMESTAKE LAB
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Trieste 23-25 Sept. 2002 Nuclear reactions and solar neutrinos The basis of Nuclear Astrophysics The spies of nuclear reactions in the Sun The luminosity constraint ...
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Solar Neutrino Problem. Rosa Mar a Dur n Delgado. Contents. Origin of solar neutrinos ... Inferred flux 2 or 3 lower than the prediction. Solar neutrino problem ...
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Beta Spectrum. Central Endpoint Value (12.98 MeV) Half-Life:0.838 sec. Tagged by Alpha ... Blocks Betas. Tagging Efficiency 90 % Decay Rate 1-300 Hz ...
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is called the neutrino free-streaming. scale and roughly corresponds to the ... On scales much larger than the free streaming scale, on the other hand, ...
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Il paradosso del test diretto: perch rimasto per cos tanto tempo al di fuori delle nostre capacit di sperimentatori? Studiare le oscillazioni nm nt con ...
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Lincoln Wolfenstein. 2. Questions. Why do ... Pe a-Garay, Peres, Petcov, Rodejohann, Smirnov, Vissani, Whisnant, Wolfenstein, Review of Decay: Elliott & Vogel ...
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LENA. Low Energy Neutrino Astrophysics ... Possible locations for LENA. Underground mine ... The Kaon and the K-decay particles are visible in LENA ...
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Power and element generation in stars Astronomy 115 Higher temps, more massive nuclei Nuclei are fused at higher and higher temperatures in the core of a massive star ...
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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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... Atsuko Ichikawa, Carol Johnstone, Steve Kahn, Boris Kayser, Chiang Kee Jung, Bruce ... Zohreh Parsa, Bernard Pope, Stefano Rigolin, Lee Roberts, Andrea ...
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Detector Issues for Solar and Reactor Neutrinos. SLAC ... Poltergeist. CHOOZ. 6 m. 10% per year. KamLAND. 20 m. Long Baseline Reactor Neutrino Experiments ...
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Large-scale (under construction): LIGO, VIRGO (I,F), GEO600 (D), TAMA300 (Jap), AIGO (Aus) ... Description (see fig.) Sensitivity. Noise (seismic, resonances, ...
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Probe to High Energies. Effects of physics beyond the SM as ... EGRET down to =2 10-8cm-2sec-1. GLAST down to ~10-11cm-2sec-1. Neutrinos/km3: ~4 10-10cm-2sec-1 ...
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Effects of physics beyond the SM as effective operators ... Something even more wild and wacky? Murayama, IHEP, June 12, 2006. 22. What it would take ...
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What lowenergy betabeams can tell about supernova physics
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use large volumes of cheap materials. Detection techniques: radiochemical experiments ... colors time of every hit PMT corrected for photon flight time ...
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A MUON (m) IS LIKE AN ELECTRON, ONLY. 200 TIMES HEAVIER. THE ELECTRON (e) IS THE LIGHTEST ... CHEAPER HIGH ENERGY COLLIDERS, BECAUSE MUONS RADIATE LESS THAN ELECTRONS. ...
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Title: Diapositiva 1 Author: Decarli Last modified by: Guido Chincarini Created Date: 10/15/2005 4:30:14 PM Document presentation format: On-screen Show
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Doppler shifts indicate Sun is ringing like a bell 'Tones' of bell allow probing of solar interior to a point (fig 4.9 in textbook) ...
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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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with acknowledgements to everyone who leaves talks where I can find them ... In 1956, Bruno Pontecorvo first shows that it might be possible for neutrinos to ...
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