The Sun and the Particle Physics
New developments in FLUKA Paola Sala INFN Milano On behalf of the FLUKA collaboration ≈ 50 members from several institutions around the world Varenna,
The Celebration of Undergraduate Research Valparaiso University Spring 2009 Expect Surprises! Donald D. Koetke Department of Physics and Astronomy.
Simulation and Modelling of Non- Destructive Testing Methods Utilising Cosmic Ray Muon Flux Craig Stone HMS Sultan Nuclear Department.
Neutrinos and the Universe E=10 15 GeV/particle LEPTOGENESIS Heavy neutrinos may generate matter-antimatter asymmetry E= 1 MeV/particle massive neutrinos.
Neutrino physics -- Alain Blondel Alain Blondel University of Geneva Neutrino Physics 1. What are neutrinos and how do we know ? 2. The neutrino questions.
Umut Kose Neutrino interaction location in the OPERA Experiment New Development of Flavor Physics, 10.03.2009, Tennomaru, Gamagori Nagoya University.
Deep-sea neutrino telescopes Prof. dr. Maarten de Jong Nikhef / Leiden University.
Results from Sudbury Neutrino Observatory
Askaryan Radio Array. 2 T. Gaisser 2005 Atmospheric neutrinos: AMANDA, IceCube Galactic neutrino flux model: e.g., Ingelman & Thunman Cosmogenic neutrino.
1 The Nuclear Emulsion Technology and the Analysis of the OPERA Experiment Data Tsutomu Fukuda Nagoya University, JAPAN On behalf of the OPERA Collaboration.
More Nuclear Physics Neutrons and Neutrinos. More Nuclear Physics Neutrons and Neutrinos Nucleon – particles that can be found in the nucleus of an atom.