Study of the cosmic ray primary composition at E0 ≡ 1000 TeV by EAS-TOP and MACRO at Gran Sasso.

Details Study of the cosmic ray primary composition at E0 ≡ 1000 TeV by EAS-TOP and MACRO at Gran Sasso. Study of the cosmic ray primary composition at E0 ≡ 1000 TeV by EAS-TOP and MACRO at Gran Sasso.

May 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994nuphs..35..257e&link_type=abstract

Nuclear Physics B, Proc. Suppl., Vol. 35, p. 257 - 258

Physics

Nuclear Physics

Cosmic Rays: Composition, Air Showers: Muons

Scientific paper

An analysis of the coincident deep underground muon data and of the e.m. component of Extensive Air Showers (EAS) as measured by the MACRO and EAS-TOP experiments at Gran Sasso is presented. Constraints on the primary cosmic ray composition are obtained, with the use of an interaction model that is based on collider data. The possibility of extrapolating the directly measured energy spectra to the energy range is tested.

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