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Anti-Protons in the Primary Cosmic Radiation

Published online by Cambridge University Press:  14 August 2015

J. Szabelski ,
J. Wdowczyk  and
A. W. Wolfendale
J. Szabelski
Affiliation:
Institute of Nuclear Research, Uniwersytecka 5, Lodz, Poland
J. Wdowczyk
Affiliation:
Institute of Nuclear Research, Uniwersytecka 5, Lodz, Poland
A. W. Wolfendale
Affiliation:
Department of Physics, Durham University, U.K.

Extract

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A knowledge of the flux of antiprotons is of value in examining the manner in which cosmic rays propagate, assuming, as is conventional, that the antiprotons arise from interactions in the I.S.M. Golden et al. (1979) have recently measured the ratio in the region of 10 GeV and, although confirmatory measurements are needed, it is instructive to compare with expectation. In a recent paper (Szabelski et al., 1980) we presented results of a new calculation of the expected ratio using the standard (equilibrium) ‘leaky box model’.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 94: Origin of Cosmic Rays , 1981 , pp. 259 - 260
Copyright
Copyright © Reidel 1981 

References

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Szabelski, J., Wdowczyk, J., and Wolfendale, A.W.: 1980, Nature (in the press).Google Scholar