Orateur
Dr
Hernan Wahlberg
(IFLP - Universidad Nacional de La Plata)
Description
Authorship: The Pierre Auger Collaboration
The mass composition of ultra-high energy cosmic rays is a critical issue to understand their origin and nature. The Pierre Auger Observatory is a hybrid instrument which
provides a powerful environment for the determination of the primary mass, being able to discriminate between photons, neutrinos and hadrons. Results on limits of photon
and neutrino fluxes together with hadronic identification are presented. The dependence of average primary mass with energy by comparison with current predictions from
models is finally discussed.
Auteur principal
Dr
Hernan Wahlberg
(IFLP - Universidad Nacional de La Plata)
Co-auteur
Full author list: http://www.auger.org/archive/authors [www.auger.org] 2011 05.html For the Pierre Auger Collaboration
(Observatorio Pierre Auger, Av. San Martin Norte 304, 5613 Malargue, Argentina)
