Muons from high-energy cosmic photino

Details Muons from high-energy cosmic photino Muons from high-energy cosmic photino

Aug 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ncimc..11..387b&link_type=abstract

Nuovo Cimento C, Serie 1 (ISSN 0390-5551), vol. 11 C, July-Aug. 1988, p. 387-404.

Physics

Cosmic Rays, Energetic Particles, Muons, Particle Production, Atmospheric Radiation, Charm (Particle Physics), Hadrons, Photons, Quarks

Scientific paper

Muon production by photino-nucleon interactions for high-energy photino (E = 10 TeV or greater) is studied. The production of muons is the result of the creation and the subsequent decay of charmed hadrons. Muon fluxes from high-energy cosmic photinos absorbed in water (ground) and atmosphere are calculated. For muon energy above the ratio of equilibrium underground muon flux to photino flux decreases with a rise of energy E because of nuclear interactions of D-mesons at decay length, and at energy about 200 TeV the vertical muon flux created in the atmosphere becomes comparable with underground equilibrium flux.

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