Sep 12 – 16, 2016
Europe/Zurich timezone
There is a live webcast for this event.

Ultra High Energy Cosmic Ray radioactivity in flight painting TeV anisotropy sky.

Sep 14, 2016, 2:00 PM
500/1-201 - Mezzanine (CERN)

500/1-201 - Mezzanine


Show room on map
Poster Contributions Neutrinos Poster Session (coffee at 15:00) & CERN Visit


Prof. Daniele Fargion (Rome University 1 Sapienza and INFN)


The presence of large scale TeVs anisotropy in Milagro, ARGO, ICECUBE
and today Hawc sky remain a mistery: how may charged cosmic rays at tens
TeV remain correlated while being bent by local solar and galactic
magnetic fields in an expected smeared nearly homogeneous maps? We
considered UHECR as mostly light (or partial heavy) radioactive nuclei
whose decay in flight may feed by alfa and neutron as well as gamma
secondaries the TeVs anisotropy. We show in the overlapped UHECR and TeV
sky remarkable correlation, whose presence might point for nearby
galactic sources as Crab, Vela, Cygnus X3 and maybe nearest AGN as Cen
A. The ARGO multi-energy gamma-CR sky is somehow the most telling in
this source search connection.

Primary author

Prof. Daniele Fargion (Rome University 1 Sapienza and INFN)

Presentation materials