'Fiducial volume' diaporamas de présentation

Updated Oscillation Results from MiniBooNE

Updated Oscillation Results from MiniBooNE . R.G. Van de Water Los Alamos National Laboratory P-25. Outline. The LSND oscillation signal. The MiniBooNE experiment: Testing LSND. Tuning the Monte Carlo Original oscillation results. New results on low energy anomaly.

1.09k views • 94 slides

Experimental Review of Supernova Relic Neutrinos

842 views • 73 slides

Supernova relic neutrinos

Supernova relic neutrinos. Kirk Bays December 8, 2011 UC Irvine. OUTLINE. 1) Theory and background: supernovae, SN neutrinos, and what has come before 2) Super-K: what is it, how does it work 3) Tools: software used to study neutrinos 4) Event selection: cut out the backgrounds!

837 views • 67 slides

NEXT A High-pressure Xenon Gas TPC: How superior energy resolution benefits both 0- ? ?? decay in 136 Xe and WIMP sea

583 views • 58 slides

KamLAND Update

KamLAND Update. Fermi National Accelerator Laboratory January 16, 2007. Lauren Hsu Lawrence Berkeley National Laboratory. Outline. I. Reactor Experiments & Neutrino Oscillations II. KamLAND overview III. KamLAND Results iV. The Future of KamLAND. The Solar Neutrino Problem.

763 views • 58 slides

Detection Methods at Reactor N eutrino E xperiments

Jun Cao Institute of High Energy Physics (Beijing). Detection Methods at Reactor N eutrino E xperiments. Feb. 11-15, 2013. Outline. A better title: Liquid Scintillator Detector for High Precision (Reactor) Neutrino Studies. Reactor n eutrino experiments

650 views • 46 slides

First Results from BOREXINO and Prospects of Low Energy Neutrino Astronomy

495 views • 42 slides

Design Considerations for a ? 13 Reactor Neutrino Experiment with Multiple Detectors

Design Considerations for a ? 13 Reactor Neutrino Experiment with Multiple Detectors. Karsten M. Heeger Lawrence Berkeley National Laboratory. Issues of Interest. Baseline Detector Locations Detector Size and Volume Detector Shape Detector Target and Detection Method

501 views • 39 slides

LAGUNA and Neutrino Physics

562 views • 35 slides

L arge U nderground X enon Dark Matter Search

L arge U nderground X enon Dark Matter Search. Matthew Szydagis, University of California at Davis. The LUX Collaboration. The most recent collaboration meeting was held in Lead, SD in March 2011. Brown. Collaboration was formed in 2007 and fully funded by DOE and NSF in 2008.

405 views • 27 slides

Status XMASS experiment

374 views • 25 slides

Overview of Reactor q 13 Experiments

Overview of Reactor q 13 Experiments. Michael Shaevitz, Columbia University SAGENAP Meeting April 16,2004 Experimental challenges for reaching sin 2 2 q 13 ? 0.01 Experiments and sites being considered Near term plans and requests.

359 views • 24 slides

Noble Liquid Tracking Detectors

366 views • 22 slides

Dark matter search at XMASS

324 views • 20 slides

XAX 10 ton Noble-Liquid Double-Phase TPC for Rare Processes

XAX 10 ton Noble-Liquid Double-Phase TPC for Rare Processes. Katsushi Arisaka. University of California, Los Angeles Department of Physics and Astronomy arisaka@physics.ucla.edu. XAX Detector (Option A). 2 m. 7m. 40 Ar (6 ton). 129/131 Xe (14 ton). 136 Xe (14 ton). 1.5 m. 7 m.

366 views • 19 slides

Results from the Full Analysis of 1998-1999 CDMS Data Runs

Results from the Full Analysis of 1998-1999 CDMS Data Runs. Richard Schnee Case Western Reserve University. CDMS Collaboration. Santa Clara University B.A. Young Stanford University L. Baudis, P.L. Brink, B. Cabrera , C. Chang, T. Saab University of California, Berkeley

278 views • 18 slides

Umut Kose

Umut Kose. Neutrino interaction location in the OPERA Experiment. Nagoya University. New Development of Flavor Physics, 10.03.2009, Tennomaru, Gamagor i. Vertex location method. CSD found. direct VTX hunting method. scan back location method. scan back. volume scan

344 views • 18 slides

Optimization for disappearance searches at the VLENF (Very Low Energy Neutrino Factory)

256 views • 16 slides

Dark Matter Search with SuperCDMS

268 views • 15 slides

nm ? nm oscillation sensitivity

nm ? nm oscillation sensitivity. K. Hiraide (Kyoto Univ.). Condition off-axis 2.5deg (04b, 40GeV) NEUT4.5 # of nm int. ~ 2200 events/22.5kt/yr 5yr exposure. Event selection criteria. Standard SK cuts: Fully contained in fiducial volume of 22.5kt Evis>30MeV 1ring m -like.

149 views • 7 slides