Computer Science
Scientific paper
Feb 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ncimc...8...76b&link_type=abstract
Nuovo Cimento C, Serie 1 (ISSN 0390-5551), vol. 8 C, Jan.-Feb. 1985, p. 76-92.
Computer Science
21
Cosmic Ray Showers, Energetic Particles, Energy Spectra, Heavy Nuclei, Muons, Primary Cosmic Rays, Composition (Property), Feynman Diagrams, High Energy Interactions, Monte Carlo Method, Nucleons, Particle Flux Density, Radiation Counters
Scientific paper
The multiple-muon rates measured in the NUSEX experiment at a vertical depth of 5000 hg/sq cm s.r. are compared with some current models of the primary cosmic-ray composition. Monte Carlo simulations as well as analytical formulas which take into account the geometrical and acceptance features of the apparatus have been used in calculations. A good agreement is found with a model in which the relative fraction of primary heavy nuclei does not increase significantly up to about 10 to the 16th eV. This model reproduces very well both the all-nucleon flux measured in the range (10 to the 13th - 10 to the 14th) eV and the all-particle spectrum up to 10 to the 16th eV.
Bologna G.
Castagnoli Carlo
Castellina Antonella
Ciocio A.
Dettorre Piazzoli B.
No associations
LandOfFree
Primary cosmic-ray spectrum at energies of 10 to the 13th - 10 to the 16th eV from multiple muon events in NUSEX experiment does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Primary cosmic-ray spectrum at energies of 10 to the 13th - 10 to the 16th eV from multiple muon events in NUSEX experiment, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Primary cosmic-ray spectrum at energies of 10 to the 13th - 10 to the 16th eV from multiple muon events in NUSEX experiment will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1594006