Journal ArticleWe have measured the proton-air inelastic cross section at s 1/2 = 30 TeV by observing the distribution of extensive-air-shower maxima as a function of atmospheric depth. This distribution has an exponential tail whose slope is λ = 72 ±9 g c m - 2 which implies that σ inel p-air = 530 ± 66 mb. Using Glauber theory and assuming that the elastic-scattering slope parameter b is proportional to σ tot pp, we infer a value of σ tot pp= 120 ± 15 mb which lies between a logs and a log2s extrapolation of the total /across section as measured at lower energies
Detecting Ultra High Energy Cosmic Rays (UHECRs) enables us to measure the proton-air inelastic cros...
There are both theoretical and experimental uncertainties in using data from cosmic-ray air showers ...
Ultra high energy cosmic rays provide the highest known energy source in the universe to measure pro...
The distribution of the maxima of high energy cosmic ray induced extensive air showers in the atmosp...
The proton-air inelastic cross section (σp-airinel) is measured at √s≈2 TeV at the EAS-TOP extensiv...
The proton-air inelastic cross section (σp-airinel) is measured at s≈2TeV at the EAS-TOP extensive a...
The attenuation length of proton primaries and the proton-air inelastic cross section are studied at...
See paper for full list of authors - 9 pages, 4 figures, Accepted at PRLWe report a measurement of t...
Ultrahigh energy cosmic rays provide the highest known energy source in the Universe to measure prot...
p. 1-9We report a measurement of the proton-air cross section for particle production at the center-...
Detecting Ultra High Energy Cosmic Rays (UHECRs) enables us to measure the proton-air inelastic cros...
There are both theoretical and experimental uncertainties in using data from cosmic-ray air showers ...
Ultra high energy cosmic rays provide the highest known energy source in the universe to measure pro...
The distribution of the maxima of high energy cosmic ray induced extensive air showers in the atmosp...
The proton-air inelastic cross section (σp-airinel) is measured at √s≈2 TeV at the EAS-TOP extensiv...
The proton-air inelastic cross section (σp-airinel) is measured at s≈2TeV at the EAS-TOP extensive a...
The attenuation length of proton primaries and the proton-air inelastic cross section are studied at...
See paper for full list of authors - 9 pages, 4 figures, Accepted at PRLWe report a measurement of t...
Ultrahigh energy cosmic rays provide the highest known energy source in the Universe to measure prot...
p. 1-9We report a measurement of the proton-air cross section for particle production at the center-...
Detecting Ultra High Energy Cosmic Rays (UHECRs) enables us to measure the proton-air inelastic cros...
There are both theoretical and experimental uncertainties in using data from cosmic-ray air showers ...
Ultra high energy cosmic rays provide the highest known energy source in the universe to measure pro...