Galactic propagation model, the modified proton spectrum and an estimation of the positron flux

Details Galactic propagation model, the modified proton spectrum and an estimation of the positron flux Galactic propagation model, the modified proton spectrum and an estimation of the positron flux

Apr 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ncimc..10..227b&link_type=abstract

Nuovo Cimento C, Serie 1 (ISSN 0390-5551), vol. 10 C, Mar.-Apr. 1987, p. 227-234.

Astronomy and Astrophysics

Astronomy

1

Astronomical Models, Milky Way Galaxy, Particle Flux Density, Positrons, Protons, Secondary Cosmic Rays, Dynamic Models, Particle Energy, Pions

Scientific paper

Positron flux at high energies is evaluated within the framework of the simple leaky box model (SLBM) and a dynamical model of multiple production of pions in high-energy proton-proton collisions. It is seen that, if the proton spectrum is modified a bit in accordance with the primary electron spectrum as proposed by Mauger and Ormes, the theoretical estimations tally nicely with the experimental measurements of the positron flux. This work highlights, once again, the role and merit of the simple leaky box model for galactic propagation.

Affiliated with

Also associated with

No associations

Rating

Galactic propagation model, the modified proton spectrum and an estimation of the positron flux 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 Galactic propagation model, the modified proton spectrum and an estimation of the positron flux, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Galactic propagation model, the modified proton spectrum and an estimation of the positron flux will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1349407