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STUDY OF THE ULTRAHIGH-ENERGY PRIMARY-COSMIC-RAY COMPOSITION WITH THE MACRO EXPERIMENT
Journal article   Open access

STUDY OF THE ULTRAHIGH-ENERGY PRIMARY-COSMIC-RAY COMPOSITION WITH THE MACRO EXPERIMENT

S Ahlen, M Ambrosio, R Antolini, G Auriemma, A Baldini, B B Bam, G C Barbarino, B C Barish, G Battistoni, R Bellotti, …
Physical review. D, Particles and fields, v 46(3), pp 895-902
01 Aug 1992
PMID: 10015004
url
https://hdl.handle.net/1969.1/183481View
url
https://doi.org/10.1103/PhysRevD.46.895View
Published, Version of Record (VoR) Open

Abstract

Astronomy & Astrophysics Physics, Particles & Fields Science & Technology Physical Sciences Physics
We present the analysis of multiple-muon events collected with one supermodule (1013 h live time) and two supermodules (1195 h live time) of the MACRO detector at Gran Sasso, Italy. Multimuon rates are shown to be sensitive to primary-cosmic-ray energies between approximately 50 TeV and several thousand TeV. Experimental data are compared with the expected rates from two composition models: a light (i.e., proton-rich) and a heavy (i.e., Fe-rich) composition. The predictions are based on a Monte Carlo simulation of the hadronic interactions of cosmic-ray nuclei, followed by a detailed tracking of the muons through the rock and the experimental apparatus. The results show good sensitivity of the MACRO detector to primary composition. The data exhibit a preference towards the light composition model.

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Domestic collaboration
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Web of Science research areas
Astronomy & Astrophysics
Physics, Particles & Fields
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