UHE neutrons in Galactic Cosmic Rays

Details UHE neutrons in Galactic Cosmic Rays UHE neutrons in Galactic Cosmic Rays

Aug 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999icrc....4..176w&link_type=abstract

Proceedings of the 26th International Cosmic Ray Conference. August 17-25, 1999. Salt Lake City, Utah, USA. Under the auspices o

Physics

Scientific paper

The upper limit on the neutrons fraction in the primary cosmic ray spectrum have been evaluated, on the base of new measurements of anisotropy of high energy of cosmic rays. The trajectories of neutrons are straight line in Galaxy. The contribution of galactic UHE neutrons to the cosmic ray flux should provide some anisotropy. The coefficient of anisotropy has bean evaluated as function energy for given percentage portion of neutrons in cosmic ray flux. From the comparison with measurement of the anisotropy coefficient the upper limit on the portion of galactic neutrons in the cosmic ray flux is estimated.

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