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Propagation of cosmic rays through the atmosphere in the quark-gluon strings model
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Erlykin, A. D. Shabelski, Y. M. Krutikova, N. P. |
| Copyright Year | 1985 |
| Description | The quark-gluon strings model succeeds in the description of multiple hadron production in the central rapidity region of nucleon-nucleon interctions. This model was developed for hadron-nucleus interactions and used for calculation of the cosmic ray propagation through the atmosphere. It is shown that at energies 10 to the 11th power to the 12th power eV, this model gives a satisfactory description of experimental data. But with the increase of the energy up to approximately 10 to the 14th power eV, results of calculations and of experiments begin to differ and this difference rises with the energy. It may indicate that the scaling violation in the fragmentation region of inclusive spectra for hadron-nucleus interactions is stronger than in the quark-gluon strings model. |
| File Size | 209189 |
| Page Count | 4 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19850027560 |
| Archival Resource Key | ark:/13960/t6tx86p53 |
| Language | English |
| Publisher Date | 1985-08-01 |
| Access Restriction | Open |
| Subject Keyword | Space Radiation Hadrons Earth Atmosphere Wave Propagation Gluons Particle Production Particle Interactions Nucleons Models Quarks Spectra Scale Ratio Cosmic Rays Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
