HIGH-ENERGY COSMIC-RAY PHYSICS WITH UNDERGROUND MUONS IN MACRO .1. ANALYSIS-METHODS AND EXPERIMENTAL RESULTS

Citation
M. Ambrosio et al., HIGH-ENERGY COSMIC-RAY PHYSICS WITH UNDERGROUND MUONS IN MACRO .1. ANALYSIS-METHODS AND EXPERIMENTAL RESULTS, Physical review. D. Particles and fields, 56(3), 1997, pp. 1407-1417
Citations number
27
Categorie Soggetti
Physics, Particles & Fields
ISSN journal
05562821
Volume
56
Issue
3
Year of publication
1997
Pages
1407 - 1417
Database
ISI
SICI code
0556-2821(1997)56:3<1407:HCPWUM>2.0.ZU;2-E
Abstract
In this paper, the first of a two-part work, we present the reconstruc tion and measurement of muon events detected underground by the MACRO experiment at Gran Sasso (E-mu greater than or equal to 1.3 TeV in atm osphere). The main aim of this work is to discuss the muon multiplicit y distribution as measured in the detector. The data sample analyzed c onsists of 4.4 x 10(6) muon events, of which similar to 263 000 are mu ltiple muons, corresponding to a total live time of 5850 h. In this sa mple, the observed multiplicities extend above N-mu = 35, with intermu on separations up to 50 m and beyond. Additional complementing measure ments, such as the inclusive muon Aux, the angular distribution, and t he muon separation distribution (decoherence), are also included. The physical interpretation of the results presented here is reported in t he following companion paper.