Position and antiproton abundances as a test for cosmic ray propagation models

Details Position and antiproton abundances as a test for cosmic ray propagation models Position and antiproton abundances as a test for cosmic ray propagation models

Aug 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975icrc....2..489l&link_type=abstract

Presented at 14th Intern. Cosmic Ray Conf., Munich, West Germany, 15-29 Aug. 1975

Computer Science

3

Antiprotons, Cosmic Rays, Positrons, Wave Propagation, Concentration (Composition), Flux Density, Particle Energy, Trapped Particles

Scientific paper

The observed variations with energy of the ratio L/M for cosmic rays with energy in the range 1 to 100 GeV/nucl. are well accounted for by three kinds of models: cosmic rays are trapped in the galaxy, where their mean path length is energy dependent; cosmic rays are trapped in their sources, and escape from them in an energy dependent fashion. The mean galactic path length is energy independent; high energy cosmic rays spend less time in dense clouds than low energy cosmic rays. The positron and antiproton fluxes predicted by these models are discussed.

Affiliated with

Also associated with

No associations

Rating

Position and antiproton abundances as a test for cosmic ray propagation models does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Position and antiproton abundances as a test for cosmic ray propagation models, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Position and antiproton abundances as a test for cosmic ray propagation models will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1539076