Properties of hadronic interactions at≈106GeV: Clues from cosmic-ray air showers
Author:
Publisher
American Physical Society (APS)
Link
http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.9.3083/fulltext
Reference46 articles.
1. Extensive air showers and Feynman scaling above 1000 GeV
2. Muon Charge-Ratio Measurement and Comparison with Prediction from Hadronic Scaling
3. Evidence for Rapidly Risingρ−ρTotal Cross Section from Cosmic-Ray Data
4. Comment on the Evidence for Rapidly Risingp−pTotal Cross Section from Cosmic-Ray Data
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1. Flux of light antimatter nuclei near Earth, induced by cosmic rays in the Galaxy and in the atmosphere;Physical Review D;2005-04-26
2. Feynman scaling and hadron–muon density in air showers;Canadian Journal of Physics;1985-07-01
3. Calculation of the equilibrium antiproton spectrum;Journal of Physics G: Nuclear Physics;1983-02
4. Cosmic ray showers and particle physics at energies1015-1018eV;Reviews of Modern Physics;1978-10-01
5. Investigation of Multiparticle Production above 1014 eV through an Analysis of Gamma-Ray Families by the Monte-Carlo Method;Journal of the Physical Society of Japan;1978-04
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