The on-going programme. 3-family oscillation matrix (Pontecorvo, Maki, Nakagawa, Sakata) S = sine c = cosine CP violation phase. drives SOLAR.
X-Ray image of Crab Nebula Pulsar Credit: NASA/CXC/ASU/J. Hester et al.) Liliana Caballero With Pf. Horowitz Molecular Dynamics Simulations of Non-uniform.
Casimir - Milano - 30 giugno 2003 1 SPIN-OFFS OF NUCLEAR AND SUBNUCLEAR PHYSICS Ugo Amaldi University of Milano Bicocca and TERA Foundation.
The km3 code C.W.James, Bologna, April 25 th 2012.
The OPERA experiment at LNGS
MINERvA Overview MINERvA is studying neutrino interactions in unprecedented detail on a variety of different nuclei Low Energy (LE) Beam Goals: – Study.
Solar Neutrinos: The Puzzle, its Resolution Prof. Tim Chupp 03 July 1991: 10Å Ca-K Image Source: National Solar Observatory (J. Harvey)
BETA-BEAMSBETA-BEAMS Piero Zucchelli On leave of absence from: High Energy Physics and INFN - Sezione di Ferrara M. Mezzetto D. Casper M. Lindroos A. Blondel.
High energy neutrino astronomy with Cherenkov telescopes L. Moscoso CEA/Irfu/SPP & APC – Paris Rive Gauche XI ICATPP Conference Villa Olmo, Como, Italy,
T2K: Contribution of Bern and general prospect
Meeting of the APS Division of Particles and Fields Brown University August 13, 2011
P5 interim report Bill Carithers Sept 11, 2006. Abe couldn’t make it today Special Workshop on Tracking September 11th Honoring Abe Seiden's 60th birthday.