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Latest results from the Pierre Auger Observatory

High Energy Astrophysical Phenomena 2015-03-17 v1 High Energy Physics - Phenomenology

Abstract

Recent results obtained with the Pierre Auger Observatory are described. These include measurements of the spectrum, anisotropies and composition of ultra-high energy cosmic rays. The ankle of the spectrum is measured at 4×10184\times 10^{18}~eV and a suppression above 3×10193\times 10^{19}~eV consistent with the GZK effect is observed. At energies above 5.5×10195.5\times 10^{19}~eV a correlation with the distribution of nearby extragalactic objects is found, including an excess around the direction of Centaurus~A, the nearest radio loud active galaxy. Measurements of the depth of shower maximum and its fluctuations suggest a gradual change in the average mass of the primary cosmic rays (under standard extrapolations of hadronic interaction models), being the results consistent with a light composition consisting mostly of protons at few×1018\times 10^{18}~eV and approaching the expectations from iron nuclei at 4×10194\times 10^{19}~eV. Upper bounds on the photon fraction and the neutrino fluxes are also obtained.

Keywords

Cite

@article{arxiv.1101.1825,
  title  = {Latest results from the Pierre Auger Observatory},
  author = {Esteban Roulet},
  journal= {arXiv preprint arXiv:1101.1825},
  year   = {2015}
}

Comments

Talk given at Quarks, Strings and the Cosmos, Hector Rubinstein Memorial Symposium, August 9-11 2010