Pierre Auger Enhancements: Transition from Galactic to Extragalactic Cosmic Ray Sources

Details Pierre Auger Enhancements: Transition from Galactic to Extragalactic Cosmic Ray Sources Pierre Auger Enhancements: Transition from Galactic to Extragalactic Cosmic Ray Sources

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..917..210e&link_type=abstract

PARTICLES AND FIELDS: Proceedings of the VI Latin American Symposium on High Energy Physics and the XII Mexican School of Partic

Other

Cosmic Rays, Neutrino, Muon, Pion, And Other Elementary Particle Detectors, Cosmic Ray Detectors

Scientific paper

The Pierre Auger Collaboration has decided to include detector enhancements in order to have unitary detection efficiencies down to 1017 eV in cosmic rays detection. These enhancements consist in high elevation telescopes and an infill area with both surface detectors and underground muon counters thus allowing a detailed study of the spectrum region where the cosmic rays sources are assumed to change from galactic to extragalactic origins.

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