Particle Physics and Astrophysics with Large Neutrino Detectors Pennsylvania State University Irina Mocioiu.
Present and future of VHE gamma astronomy Manel Martinez 43 rd Winter Meeting March 2015-Benasque.
The GRI Laue-lens and lens spacecraft - configuration options - lens performance calculations Niels Lund Danish National Space Center.
Dedicated as a tribute to Jean Tran Thanh Van and Kim who step aside after initiating and organizing the past 44 Rencontres de Moriond in order to promote.
NsFFAGs and ADSRs what they are and why you need them 1. The current nsFFAG programme 2. Thorium ADSRs and their advantages 3. Matching the two Roger Barlow.
Auger FB review, Malargüe, October 2001. DPA – R. Shellard & S. J. Sciutto1 PIERRE AUGER OBSERVATORY Finance Board Review Data Processing and Analysis.
Energy Band View of Semiconductors Conductors, semiconductors, insulators: Why is it that when individual atoms get close together to form a solid – such.
1 SLAC National Accelerator Laboratory Amber Boehnlein October 18, 2011.
Mini-Symposium: Centre for Cosmological Physics 4 October 2002 Status of the Pierre Auger Observatory and Future Prospects Alan Watson University of Leeds.
Neutrinos and Ultra-High Energy Cosmic Rays Dmitry Semikoz MPI, Munich & INR, Moscow in collaboration with F.Aharonian, O.Kalashev, V.Kuzmin, A.Neronov.
A. BELIAS, NESTOR Institute, Pylos, Greece TeVPA 2009, July 13-17, SLAC1 KM3NeT, a deep sea neutrino telescope in the Mediterranean Sea KM3NeT objectives.
Searching for Small-Scale Anisotropies in the Arrival Directions of Ultra-High Energy Cosmic Rays with the Information Dimension Eli Visbal (Carnegie Mellon.
