A Deduction of the High Energy Spectrum of Cosmic-Ray Primary Nucleons from the Observed Muon Spectrum
- 15 December 1951
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review B
- Vol. 84 (6) , 1199-1203
- https://doi.org/10.1103/PhysRev.84.1199
Abstract
Fermi's theory of pion production is extended to treat collisions of nucleons with air nuclei. The energy distribution of the created pions and their daughter muons is approximately calculated, and is applied to correlate the observed muon spectrum in the energy range 10-100 Bev with the primary nucleon spectrum. The results and limitations of this procedure are discussed.Keywords
This publication has 13 references indexed in Scilit:
- Cosmic-Ray Nucleon-Nucleon Collisions in Photographic EmulsionsPhysical Review B, 1951
- Angular Distribution of the Pions Produced in High Energy Nuclear CollisionsPhysical Review B, 1951
- Evidence for the Multiple Production of Mesons in a Single Nucleon-Nucleon CollisionPhysical Review B, 1950
- Momentum Distribution of Charged Cosmic-Ray Particles at Sea LevelPhysical Review B, 1950
- The Barometric Effect for Large Cosmic-Ray Bursts under Thick Absorbers at 11,500 Feet Elevation and the Absorption Mean Free Path for Very High Energy Nuclear CollisionsPhysical Review B, 1950
- A Directional and Latitude Survey of Cosmic Rays at High AltitudesPhysical Review B, 1950
- Interpretation of Cosmic-Ray PhenomenaReviews of Modern Physics, 1948
- Extensive Cosmic-Ray Showers and the Energy Distribution of Primary Cosmic RaysPhysical Review B, 1941
- The Intensity of Cosmic Radiation under Thick LayersReviews of Modern Physics, 1939
- Die Absorptionskurve der harten Komponente der kosmischen UltrastrahlungThe European Physical Journal A, 1937