On total inelastic cross-sections and the average depth of the maximum of extensive air showers
arXiv:astro-ph/0309010 · doi:10.1088/0954-3899/29/11/001
Abstract
The model dependence of the development of extensive air showers generated by high-energy cosmic-ray particles in the atmosphere is studied. The increase of proton-proton and proton-air inelastic cross-sections and values for the elasticity are varied in the hadronic interaction model QGSJET. Using the CORSIKA simulation program, the impact of these changes is investigated on air shower observables like the average depth of the shower maximum X_max and the number of muons and electrons at ground level. Calculating the mean logarithmic mass from experimental X_max values, it is found that a moderate logarithmic increase of the proton-proton inelastic cross-section from sigma_pp^inel=51 mb at E_0=10^6 GeV to sigma_pp^inel=64 mb at E_0=10^8 GeV and an elasticity, additionally increased by 10% to 15%, describes the data best. Using these parameters, the mean logarithmic mass lna derived from X_max measurements is compatible with the extrapolations of the results of direct measurements to high energies using the poly-gonato model.
Cited by in corpus (28)
- Cosmic Rays from the Knee to the Highest Energies
- Models of the Knee in the Energy Spectrum of Cosmic Rays
- New facts about muon production in Extended Air Shower simulations
- Spectrum of cosmic rays, produced in supernova remnants
- Cosmic-ray energy spectrum and composition up to the ankle - the case for a second Galactic component
- Proton-air cross section measurement with the ARGO-YBJ cosmic ray experiment
- Study of multi-muon bundles in cosmic ray showers detected with the DELPHI detector at LEP
- Cosmic rays from the knee to the second knee: 10^14 to 10^18 eV
- A review of experimental results at the knee
- Cosmic-ray composition and its relation to shock acceleration by supernova remnants
- The origin of galactic cosmic rays
- GCOS -- The Global Cosmic Ray Observatory
- Test of the hadronic interaction model EPOS with air shower data
- Very High Energy Cosmic Rays and Their Interactions
- Results from the KASCADE, KASCADE-Grande, and LOPES experiments
- Overview on direct and indirect measurements of cosmic rays - Some thoughts on galactic cosmic rays and the knee
- Muon Charge Information from Geomagnetic Deviation in Inclined Extensive Air Showers
- The end of the galactic cosmic-ray energy spectrum - a phenomenological view
- Cosmic ray spectrum by energy scattered by EAS particles in the atmosphere and galactic model
- Extensive Air Showers and the Physics of High Energy Interactions
- A new method to measure the attenuation of hadrons in extensive air showers
- Astronomy with ultra high-energy particles
- Between the cosmic-ray `knee' and the `ankle': Contribution from star clusters
- 'Sling effect' in the development of atmospheric cascades induced by primary cosmic ray nuclei
- Test of hadronic interaction models with air shower data
- On the deficit of calculated muon flux at sea level for energies GeV
- Experimental Efforts on Very High-Energy Cosmic Rays and their Interactions - Conference Summary
- Muon Charge Ratio of Ultrahigh Energy Cosmic Rays