XXX-th International Workshop on High Energy Physics “Particle and Astroparticle Physics, Gravitation and Cosmology: Predictions, Observations and New Projects”

Session

High energy cosmic rays

27 Jun 2014, 09:30

Conference Hall (IHEP, Protvino, Theoretical Division)

52. The Pierre Auger Observatory: latest results and future prospects

Fernando Arqueros (UCM)

27/06/2014, 09:30

53. Measurement of the Cosmic Ray Energy Spectrum and of the Muon content of EAS with the Pierre Auger Observatory

Mr Joao Espadanal (LIP, Lisbon)

27/06/2014, 09:55

54. Cosmic-ray research with AMS-02 on the International Space Station

Mr Henning Gast (I. Physikalisches Institut B, RWTH Aachen)

27/06/2014, 10:20

55. First Results from LUX Dark Matter Experiment

Vladimir Solovov (LIP)

27/06/2014, 11:05

56. Panel discussion on Cosmic Rays

27/06/2014, 11:30

Moderator: Alexandre Kisselev Panelists: Fernando Arqueros, Henning Gast, Vladimir Solovov Questions: 1. What is the origin of the GZK-like suppression of the cosmic ray (CR) flux? Is it due to energy loss during propagation or due to reaching maximum energy achievable in a source? 2. Are the data on mass composition of ultra- high energy CRs consistent with a hypothesis that primary...