On the primary cosmic ray nuclei spectra behaviour in the 1016 eV energy region

Details On the primary cosmic ray nuclei spectra behaviour in the 1016 eV energy region On the primary cosmic ray nuclei spectra behaviour in the 1016 eV energy region

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990esasp.311..115b&link_type=abstract

In ESA, Plasma Astrophysics p 115-120 (SEE N91-15046 06-90)

Physics

Nuclear Physics

Dark Matter, Interstellar Matter, Muons, Primary Cosmic Rays, Destruction, Elementary Particles, Energy Spectra, Nuclei (Nuclear Physics), X Ray Astronomy

Scientific paper

On the basis of the investigation of muon group parameters, the conclusion is made on existence of the primary cosmic ray nuclei energy spectra cutoff in the energy range approximately greater than 10 to the 16th power eV. As a mechanism responsible for the effect, the destruction of the nuclei of some objects (elementary particles) of interstallar media is proposed. The mass of these particles is approximately less than 30 eV. The possibility of the identification of these objects with the dark matter is discussed.

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