Status of Top-Down Models for the Origin of Ultra-High Energy Cosmic Rays I. Observation of ultra-high energy cosmic rays before the Pierre Auger Observatory.
What we (don’t) know about UHECRs We know: their energies (up to 10 20 eV). their overall energy spectrum We don’t know: where they are produced how.
The cosmic ray luminosity of the nearby active galactic nuclei
+ LHCf: status and future programs Oscar Adriani University of Florence & INFN Firenze With introduction and summary for ‘young newcomers’
A Cherenkov Radiation Detector for the Auger Project Katarzyna Oldak Research Adviser: Corbin Covault Department of Physics The purpose of this project.
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Astroparticles (CR’s & ) in the nearby universe & Virtual Observatory … one Universe, two worlds Giuseppe Longo 1,2,3 & Gennaro Miele 1,2 1-Department.
Results from the Pierre Auger Observatory
Humberto Salazar (FCFM-BUAP) for the Pierre Auger Collaboration, CTEQ- Fermilab School Lima, Peru, August 2012 Ultrahigh Cosmic Rays: The highest energy.
Research at VATLY P.N. Diep for P.T. Anh, P. Darriulat, P.N. Dong, D.T. Hoai, P.T. Nhung, N.T. Phuong and N.T. Thao (Institute for Nuclear Science and.
The Auger Observatory for High-Energy Cosmic Rays G.Matthiae University of Roma II and INFN For the Pierre Auger Collaboration The physics case Pierre.
Articles Siempre imaginé que el Paraíso sería algún tipo de biblioteca (Borges)
