Comments on stochastic acceleration of cosmic rays

Details Comments on stochastic acceleration of cosmic rays Comments on stochastic acceleration of cosmic rays

Nov 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...241.1195c&link_type=abstract

Astrophysical Journal, Part 1, vol. 241, Nov. 1, 1980, p. 1195-1198.

Astronomy and Astrophysics

Astrophysics

36

Cosmic Rays, Energy Spectra, Interstellar Matter, Magnetohydrodynamic Waves, Molecular Clouds, Particle Acceleration, Carbon, Oxygen Spectra, Particle Collisions, Stochastic Processes, Supernova Remnants

Scientific paper

The spectrum of particles subjected to second-order Fermi acceleration is studied, and the spectra of both the primary particles such as C and O and their nuclear secondaries such as Li, Be, and B are derived explicitly. The second-order term is seen to be of prime importance in the acceleration process. The secondary-to-primary ratio is shown to increase logarithmically with energy contrary to observation. These considerations are extended to arbitrary stochastic processes, and it is concluded that cosmic rays are not accelerated in the interstellar medium.

Affiliated with

Also associated with

No associations

Rating

Comments on stochastic acceleration 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 Comments on stochastic acceleration of cosmic rays, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Comments on stochastic acceleration of cosmic rays will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1390244