Leading change
September 20, 2002 NeSS 2002 Adam Para, Fermilab Physics Opportunities with NuMI Beam Physics Motivation Off-axis NuMI Beam Backgrounds and Detector Issues.
Neutrino mass matrix in triplet Higgs Models with A_4 Symmetry Myoung Chu Oh Miami 2008, Dec. 17, 2008 Based on work with Seungwon Baek.
Presented by John G. Learned University of Hawaii at Manoa with thanks for help from many colleagues at UH, in KamLAND, and others Hanohano Particle Physics.
Neutrino Flavor ratio on Earth and at Astrophysical sources K.-C. Lai, G.-L. Lin, and T. C. Liu, National Chiao Tung university Taiwan INTERNATIONAL SCHOOL.
Working Group 1 Summary: D. Casper * M. Lindner K. Nakamura Oscillation Physics (mostly) - Part 3 -
GERDA: GERmanium Detector Array Searching for 0 2 decay Xiang Liu Max-Planck-Institut für Physik 1.0 2 introduction 2.GERDA setup & detectors 3. Low.
Leading Change Karen Sledge. Objectives Background Transformation Through Change Describe the 8 stages Examine the actions needed for change Give.
WIMPS & Neutrinos
Cosmological Matter-Antimatter Asymmetry and Neutrino Oscillations
Atmospheric Neutrinos Stefan Söldner-Rembold University of Manchester 19 December 2013 1.
GERDA: GERmanium Detector Array Searching for 0 2 decay
