The Influence of Reacceleration on the Antiproton Abundance in the Interstellar Medium and its attenuation in the Atmosphere

Details The Influence of Reacceleration on the Antiproton Abundance in the Interstellar Medium and its attenuation in the Atmosphere The Influence of Reacceleration on the Antiproton Abundance in the Interstellar Medium and its attenuation in the Atmosphere

Aug 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999icrc....3...73s&link_type=abstract

Proceedings of the 26th International Cosmic Ray Conference. August 17-25, 1999. Salt Lake City, Utah, USA. Under the auspices o

Physics

Scientific paper

An estimation has been made on the influence o reacceleration about the abundance of secondary p flux in the Inter Stellar Medium duly initiated by primary cosmic ray proton collisions in the confined p+He gases in the medium. The present derivation is based on the production of antiprotons in the atmosphere by primary protons at different small depths.

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