A new method of determining the spectral index for protons in the energy range about 1013 eV

Details A new method of determining the spectral index for protons in the energy range about 1013 eV A new method of determining the spectral index for protons in the energy range about 1013 eV

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005cosre..43...79g&link_type=abstract

Cosmic Research, Volume 43, Issue 2, pp.79-83

Physics

Scientific paper

We consider a relationship between the difference in spectral indices of the spectra of single hadrons and all hadrons (βsngl - βh) and the difference in the indices of the spectra of galactic cosmic ray (GCR) protons and nuclei. It is demonstrated that at the mountain level the ratio (βp - βZ)/(βsngl - βh) is always larger than unity, if (βsngl - βh) > 0.1. From the experimental value βsngl - βh = 0.4 ± 0.05 we derive that, in the vicinity of E = 10 TeV, βp - βZ ≥ 0.49 ± 0.06 , i.e., βp ≥ 3.09 ± 0.06.

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