Possible cosmological origin of the ultra high energy cosmic rays

Details Possible cosmological origin of the ultra high energy cosmic rays Possible cosmological origin of the ultra high energy cosmic rays

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984hea..meet...87h&link_type=abstract

High energy astrophysics, p. 87 - 93

Statistics

Computation

Anisotropy, Astronomical Models, Cosmic Rays, Cosmology, Mathematical Models, Spectrum Analysis, Computation, Curve Fitting, Data Acquisition, Neutrinos, Statistical Analysis

Scientific paper

Using improved spectrum evolution results for nucleons propagation through the 3(0)K microwave background, a model of the UHE cosmic rays above 10 (18) eV presented, assuming a universal cosmological component associated with bright phase activity and a semilocal component assocxiated with the Virgo cluster. The results for the spectrum and anisotropy are in good agreement with the Haverah Park EAS observations. An unambiguous and potentially detectable electron neutrino spectrum is derived.

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