B.Satyanarayana Department of High Energy Physics Tata Institute of Fundamental Research, Mumbai E: [email protected], W: bsn.
George M. Fuller Department of Physics & Center for Astrophysics and Space Science University of California, San Diego Supernova Physics and DUSEL UCLA/UCSD.
X The values of all neutrino oscillation parameters in the 3ν scheme can now be extracted from global fits of available data with a precision better than.
Beta decay experiments Fabrice Piquemal CENBG, University Bordeaux 1 CNRS/IN2P3 and LSM (CEA – CNRS) Double beta decay and tritium experiments, current.
Type II Seesaw Portal and PAMELA/Fermi LAT Signals
ASPERA WP 2: Neutrino Mass
Large Liquid Argon Detector R&D in the US David Finley / Fermilab
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1 MEMPHYS Simulation & Performance A. Tonazzo, N. Vassilopoulos * / APC for MEMPHYS ECFA Review Panel, Dansbury May 2011 * now at IPHC, Strasbourg.
Neutrino mass hierarchy, status of the flavor problem (discussion session)
Future Neutrino Physics Mitch Soderberg Fermilab Institutional Review June 6-9, 2011
Accelerator Neutrino Oscillation Physics Lecture I
