U. Becker
CERN
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Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 1990
B. Adeva; M. Aguilar-Benitez; A. Aloisio; M.G. Alviggi; D. Antreasyan; L. Baksay; U. Becker; J. Berdugo; G. J. Bobbink; J. G. Branson; C. Burgos; J.D. Burger; D. Campana; F. Carbonara; M. Cerrada; Y.H. Chang; Min Chen; G. Chiefari; N. Colino; E. Drago; P. Duinker; I. Duran; F.C. Erné; R. Fabbretti; S. Fabre; S. Feher; S.S. Gau; M. Gettner; E. Gonzalez; H. van der Graaf
Abstract Measurements of cosmic rays in the L3 multisampling chambers are presented. The study of tracks with polar angles from 30° θ
Archive | 1989
U. Becker
The “art of detection” and the strategy of physics will be the focus of this presentation. Firstly, why γ, e, and μ ? Because they are fundamental; directly detectable in unique ways, hence at high energies easy to distinguish from hadrons. The physical background is small and the production rate rare. If we consider: n n
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