'Long baseline' diaporamas de présentation

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Neutrino Physics

Neutrino Physics. Hitoshi Murayama (Berkeley + I P M U ) NNN 2007, Hamamatsu Oct 3, 2007. Outline. Past: Why Neutrinos? Present: Era of Revolution Near Future: Bright Prospect Big Questions: Need Synergies Astrophysical Probe Conclusion. Past. Why Neutrinos?.

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Astrometry from Long-Baseline OIR Interferometers

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Neutrino Oscillation

Neutrino Oscillation. Hitoshi Murayama (Berkeley) PRC-US Meeting @ IHEP June 12, 2006. Outline. Past: Why Neutrinos? Present: Era of Revolution Future Conclusion. Past. Why Neutrinos?. Interest in Neutrino Mass. So much activity on neutrino mass already. Why am I interested in this?

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New Large * Neutrino Detectors

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Very Long Baseline experiment with a Super Neutrino Beam Brookhaven National Laboratory

Very Long Baseline experiment with a Super Neutrino Beam Brookhaven National Laboratory Presented to the NuFact04, Osaka University Stephen Kahn Brookhaven National Laboratory For the Brookhaven Neutrino Working Group References: Phys Rev D 68, 012002 (2003)

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Particle Physics and Astrophysics with Large Neutrino Detectors

Particle Physics and Astrophysics with Large Neutrino Detectors. Irina Mocioiu . Pennsylvania State University. Experiments. IceCube/DeepCore : Cherenkov light in ice (South Pole) PINGU Antares : Cherenkov light in water ( Mediteraneen ) Pierre Auger : air showers (Argentina)

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Project X Physics Opportunities

Project X Physics Opportunities. A.J. Lankford UC Irvine Fermilab Physics Advisory Committee Nov. 1, 2007. Introduction. Beyond its synergy with the ILC, the case for a major project such as Project X must be based on its physics impact. Primarily its discovery potential

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The NO n A Experiment ( N uMI O ff-Axis n e A ppearance Experiment)

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Status of Neutrino Science

Status of Neutrino Science. Hitoshi Murayama LBNLnu April 11, 2003. Two Main Directions. Neutrino Properties Neutrino Masses Neutrino Mixings Nature of Neutrinos Neutrino as a Probe Parton Distribution Function Precision Electroweak Physics Neutrino Astrophysics. Outline.

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Antineutrino Detector of Dayabay Reactor Neutrino Experiment

Antineutrino Detector of Dayabay Reactor Neutrino Experiment. Yuekun Heng, hengyk@ihep.ac.cn IHEP, Beijing On Behalf of the DayaBay Collaboration. 11 th Pisa meeting on advanced detectors, Italy, May 24-30, 2009. Outline. Motivation and design of DYB reactor experiment <0.01

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Physics with a very long neutrino factory baseline

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Very Long Baseline experiment with a 1 MW Neutrino Beam Brookhaven National Laboratory

Very Long Baseline experiment with a 1 MW Neutrino Beam Brookhaven National Laboratory (work of the BNL neutrino working group Upenn, Utexas, StonyBrook, Princeton) Presented to the BSA Review committee (Ref: Diwan et al., PRD68, 012002, 2003) Milind V. Diwan

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Outlook on Underground Science

Outlook on Underground Science. Thomas Bowles Los Alamos National Laboratory / University of Washington American Physical Society Meeting Philadelphia April 5, 2003. Nuclear Physics. The Reach of Underground Science. A Remarkably Wide Range of Science and

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Probing the Octant of ? 23 with very long baseline neutrino oscillation experiments

CYCU Oct. 17 2006. Probing the Octant of ? 23 with very long baseline neutrino oscillation experiments. G.-L. Lin National Chiao-Tung U. Taiwan. Work done with Y. Umeda. What we know about the neutrino oscillation parameters. Super-K I+II Preliminary.

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John Learned, University of Hawaii at Manoa (& other colleagues at UH and elsewhere)

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Future Prospects of KamLAND & q 13

sin 2 2 q may be shown to <1??. (No official plot. Just to get a sense.). 2005 fall: 4 p calibration ( s fid : 4.7%->3%). error (%). KL-II:. Solar 7 Be n. Future Prospects of KamLAND & q 13. KL is still only long baseline reactor n experiment in near future. KL-III:.

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