New limit on the low-energy antiproton/proton ratio in the Galactic cosmic radiation

Details New limit on the low-energy antiproton/proton ratio in the Galactic cosmic radiation New limit on the low-energy antiproton/proton ratio in the Galactic cosmic radiation

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988phrvl..61..145a&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 61, July 11, 1988, p. 145-148. Research supported by Boston University, Indiana U

Physics

61

Antiprotons, Galactic Cosmic Rays, Milky Way Galaxy, Protons, Balloon-Borne Instruments, Mass Spectra, Particle Energy, Upper Atmosphere

Scientific paper

Results are presented from a balloon-borne apparatus searching for
low-energy antiprotons in the Galactic cosmic rays. For energies less
than 640 MeV at the top of the atmosphere, no cosmic-ray antiprotons
were observed. This yields an upper limit to the antiproton/proton ratio
of 0.000046 at the 85-percent confidence level.

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