Present status of neutrino mixing and masses from oscillation experiments: what future ? Antonio Ereditato (INFN Napoli) Neuchatel Meeting 21-22 June 2004.
Precision Neutrino Oscillation Measurements & the Neutrino Factory Scoping Study for a Future Accelerator Neutrino Complex – Discussion Meeting Steve Geer,
Non-standard physics and user- defined priors in GLoBES Workshop on physics and applications of the GLoBES software Workshop on physics and applications.
Neutrino emission =0.27 MeV E=0.39,0.86 MeV =6.74 MeV ppI loss: ~2% ppII loss: 4% note: /Q= 0.27/26.73 = 1% ppIII loss: 28% Total loss: 2.3%
Solar neutrino results from Super-Kamiokande Satoru Yamada for the Super-Kamiokande collaboration Institute of cosmic ray research, University of Tokyo.
Elisabeth Falk Harris University of Sussex On behalf of the MINOS Collaboration SNOW 2006, Stockholm, 2-6 May 2006 First MINOS Results from the NuMI Beam.
CP violation searches with Neutrino Factories and Beta Beams Neutrinos in Particle, in Nuclear and in Astrophysics Trento, Italy November 20, 2008 Walter.
Prospects for 7 Be Solar Neutrino Detection with KamLAND Stanford University Department of Physics Kazumi Ishii.
MICE Ionization Cooling Channel and Phase II Construction Michael S. Zisman Center for Beam Physics Accelerator & Fusion Research Division Lawrence Berkeley.
Energy Reconstruction Algorithms for the ANTARES Neutrino Telescope J.D. Zornoza 1, A. Romeyer 2, R. Bruijn 3 on Behalf of the ANTARES Collaboration 1.
Junpei Shirai Research Center for Neutrino Science Tohoku University (for the KamLAND Collaboration) Neutrino experiments: Review of Recent Results Tau04,
The OPERA Experiment 12 th Topical Seminar on Innovative Particle and Radiation Detectors (IPRD10) 7-10 June 2010, Siena, Italy Jonas Knüsel Albert Einstein.