Homogeneous Metagalactic Origin of Cosmic Rays

Details Homogeneous Metagalactic Origin of Cosmic Rays Homogeneous Metagalactic Origin of Cosmic Rays

Mar 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970ap%26ss...6..415l&link_type=abstract

Astrophysics and Space Science, Volume 6, Issue 3, pp.415-419

Astronomy and Astrophysics

Astrophysics

Scientific paper

Starting with the hypothesis that cosmic rays are evenly distributed in the metagalaxy, it is shown that the flux of the electron-positron component, which is produced through π-μ-e decays, following the nuclear collisions of the cosmic ray beam with the intergalactic medium, takes <-4×1016 sec to reach steady state. The corresponding value of the flux of thepositron component and its implications regarding the homogeneous model of the metagalactic origin of cosmic rays are discussed.

Affiliated with

Also associated with

No associations

Rating

Homogeneous Metagalactic Origin of Cosmic Rays 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 Homogeneous Metagalactic Origin of Cosmic Rays, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Homogeneous Metagalactic Origin of Cosmic Rays will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1451896