Computer Science – Sound
Scientific paper
Jan 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...349...78s&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 349, Jan. 20, 1990, p. 78-90. Research supported by Boston University, Indi
Computer Science
Sound
45
Antiprotons, Elementary Particle Interactions, Interstellar Matter, Protons, Secondary Cosmic Rays, Astronomical Spectroscopy, Balloon Sounding, Interstellar Magnetic Fields, Mass Spectra, Monte Carlo Method
Scientific paper
A search for antiprotons (p-bars) in the cosmic radiation with energies below 1580 MeV at the top of the atmosphere was performed using the PBAR balloon-borne magnetic spectrometer. No antiprotons were observed in 124,000 proton events. For the energy interval 100-640 MeV, an upper limit is reported to the p-bar/p ratio of 2.8 x 10 to the -5th at the top of the atmosphere, after correcting for instrumental efficiencies and contributions from secondary particles. No antiproton was observed in the energy interval 640-1580 MeV, which yields an upper limit to the p-bar/p ratio of 6.1 x 10. By combining both data sets, the limits on the p-bar/p ratio can be improved to 2.0 x 10 to the -5th. The detector performance and instrumental efficiencies of the individual detector components are discussed. A detail Monte Carlo calculation was used to evaluate the instrumental efficiency for both antiprotons and protons as a function of momentum.
Ahlen Steven P.
Barwick Steve W.
Beatty James J.
Bower Charles R.
Buford Price P.
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