Vulcano Workshop 2012

Session

The Challenge of Cosmic Ray Production

31 May 2012, 17:00

Vulcano Island, Sicily

58. Pierre Auger UHE CRs and Composition

Aurelio Grillo

31/05/2012, 17:25

Pierre Auger UHE CRs and Composition

60. Theoretical Models for the Propagation Ultra High Energy Cosmic Rays and the Auger observations

Roberto Aloisio

31/05/2012, 17:50

Theoretical Models for the Propagation Ultra High Energy Cosmic Rays and the Auger observations

59. The Influence of Results of UHE-CR Detection on LHC Experiments

Anatoly Petrukhin

31/05/2012, 18:10

The Influence of Results of UHE-CR Detection on LHC Experiments

9. Precise cosmic rays measurements with PAMELA

Dr Alessandro Bruno (INFN sezione di Bari, Bari, Italy)

31/05/2012, 18:35

The PAMELA experiment was launched on board of the Resurs-DK1 satellite on 15th of June 2006. The apparatus was designed to conduct precision studies of the charged cosmic radiation over a wide energy range, from tens of MeV up to several hundred GeV, with unprecedented statistics. In five years of continuous data taking in space, PAMELA accurately measured the energy spectra of cosmic ray...

7. UHECR event map and multiplets made by Lightest and Heaviest radioactive nuclei

Dr Daniele Fargion (ROMA1)

31/05/2012, 19:00

The puzzle of UHECR origination is related to their composition, spectra and maps. The main signal that srvived in last AUGER data is a clustering along Cen A. Very recent multiplet ar 20 EeV do cluster also along Cen A. These events fit a UHECR Lignt nuclei for extragalactic sources. Most of remanents UHECR may be heavy nuclei radioactive originated mostly by nearby SN-GRB whose traces are...