Extreme energy gamma rays and neutrinos and their observation in JEM-EUSO Mission

Details Extreme energy gamma rays and neutrinos and their observation in JEM-EUSO Mission Extreme energy gamma rays and neutrinos and their observation in JEM-EUSO Mission

Jun 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1238..377s&link_type=abstract

TOURS SYMPOSIUM ON NUCLEAR PHYSICS AND ASTROPHYSICS-VII. AIP Conference Proceedings, Volume 1238, pp. 377-379 (2010).

Physics

Nuclear Physics

Cosmic Rays, Gamma-Rays, Neutral Currents, Cosmic Ray Showers, Protons, Cosmic Rays, Gamma-Ray, Neutral Currents, Extensive Air Showers, Protons And Neutrons

Scientific paper

The origin of the extreme energy cosmic rays (EECRs) is a mystery in the contemporary astrophysics. The JEM-EUSO Mission that mainly aims establishing astronomy using such EECRs with very high statistics will also have realistic capability of detecting gamma rays and neutrinos with ~1020 eV energies. Aboard the International Space Station, the JEM-EUSO mission also provides a unique platform to detect and study the air showers from extreme energy gamma rays and neutrinos. In the present paper, we discuss a part of results from our study on properties of gamma ray and neutrino induced air showers and the advantage for space-based observation.

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