Upper limit to antiproton flux in cosmic radiation above 100 GeV using muon charge ratio

Details Upper limit to antiproton flux in cosmic radiation above 100 GeV using muon charge ratio Upper limit to antiproton flux in cosmic radiation above 100 GeV using muon charge ratio

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....9..167s&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Late Papers. Volume 9 (A85-22801 0

Physics

Antiprotons, Cosmic Rays, Energetic Particles, Muons, Constraints, Flux Quantization, Incident Radiation, Maxima

Scientific paper

Upper limits to the fraction of antiprotons in cosmic radiation have
been estimated from the observed charge ratio of muons at sea-level.
Using these values, it is shown that constraints can be set on the
extragalactic hypothesis of the observed antiprotons in the framework of
energy-dependent confinement of cosmic rays in the galaxy.

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