'Sin 2 1' diaporamas de présentation

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?. ?. ??? ???? ?????. The Daya Bay Reactor Neutrino Experiment and ? 13. Manfred Jeitler HEPHY 19 October 2012. Material from Observation of Electron Anti-neutrino Disappearance at Daya Bay. Yifang Wang Institute of High Energy Physics CERN ? March 20, 2012

983 views • 78 slides

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?. ?. ??? ???? ?????. The Daya Bay Reactor Neutrino Experiment and ? 13. Manfred Jeitler HEPHY 19 October 2012. Material from Observation of Electron Anti-neutrino Disappearance at Daya Bay. Yifang Wang Institute of High Energy Physics CERN ? March 20, 2012

780 views • 78 slides

CKM Phases: ? 1 /?

CKM Phases: ? 1 /?. Tom Browder (University of Hawaii). Belle and BaBar results. Measurements of large CPV in b ?c c s modes Studies in b ?c c d modes Search for New Physics: CPV in b?s penguin modes. _. _. KM ansatz: CPV is due to a complex phase in the quark mixing matrix:.

858 views • 72 slides

Is there evidence for a peak in this data?

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Is there evidence for a peak in this data?

690 views • 61 slides

Observation of Electron Anti-neutrino Disappearance at Daya Bay

Observation of Electron Anti-neutrino Disappearance at Daya Bay. Yifang Wang Institute of High Energy Physics CERN ? March 20, 2012. Outline. Introduction Data set & quality control Calibration and Event reconstruction Event selection Backgrounds & uncertainties

670 views • 58 slides

Measuring sin 2 2 q 13 with the Daya Bay nuclear power reactors

Measuring sin 2 2 q 13 with the Daya Bay nuclear power reactors. Yifang Wang Institute of High Energy Physics. Neutrinos. Basic building blocks of matter ? Tiny mass, neutral, almost no interaction with matter, very difficult to detect.

659 views • 57 slides

Measuring sin 2 2 q 13 with the Daya Bay nuclear power reactors

Measuring sin 2 2 q 13 with the Daya Bay nuclear power reactors. Yifang Wang Institute of High Energy Physics. Neutrinos. Basic building blocks of matter ? Tiny mass, neutral, almost no interaction with matter, very difficult to detect.

669 views • 57 slides

p-values and Discovery

p-values and Discovery. Louis Lyons Oxford l.lyons@physics.ox.ac.uk. KEK, May 2007. TOPICS. Discoveries H0 or H0 v H1 p-values: For Gaussian, Poisson and multi-variate data Goodness of Fit tests Why 5 σ ? Blind analyses What is p good for?

619 views • 55 slides

p-values and Discovery

p-values and Discovery. Louis Lyons Oxford l.lyons@physics.ox.ac.uk. SLUO Lecture 4, February 2007. TOPICS. Discoveries H0 or H0 v H1 p-values: For Gaussian, Poisson and multi-variate data Goodness of Fit tests Why 5 ? ? Blind analyses What is p good for?

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Conference Summary

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New Physics and Rare B Decays

571 views • 46 slides

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481 views • 38 slides

Towards Future Neutrino Activities

Towards Future Neutrino Activities. Alain Blondel, Alessandro Bravar Fanny Dufour, Yordan Karadhzov, Alex Korzenev, Etam Noah, Mark Rayner, Nicolas Abgrall, Ruslan Asfandiyarov, Alexis Haesler, Carlos Martin, Melody Ravonel, Enrico Scantamburlo.

510 views • 37 slides

JHF-Kamioka Neutrino Oscillation Experiment using JHF 50 GeV PS

333 views • 22 slides

JHF n experiment (Requirements for Electronics)

KEK Electronics Wroskhop October 4-5, 2001. JHF n experiment (Requirements for Electronics). Introduction to JHF n Requirement to Front n detectors Example-1: K2K Upgrade Electronics Example-2: Super-K upgrade (FADC) General Comments Summary. T. Nakaya (Kyoto Univ.).

193 views • 19 slides

268 views • 15 slides

n e search @ SK (update with 40GeV flux)

n e search @ SK (update with 40GeV flux). S.Mine (UCI). cf.) original report with 50GeV flux http://jnusrv01.kek.jp/jhfnu/NP04nu/PresenFiles/sk/ explanation of 40GeV flux by A.K.Ichikawa http://jnusrv01.kek.jp/jhfnu/internal/OfficialPlots/flux/.

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1 John 1:7

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Integration

93 views • 9 slides