Proton collisions in cosmic ray sources

Details Proton collisions in cosmic ray sources Proton collisions in cosmic ray sources

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..83...75s&link_type=abstract

Astrophysics and Space Science, vol. 83, no. 1-2, Apr. 1982, p. 75-79.

Astronomy and Astrophysics

Astrophysics

3

Cosmic Rays, Elementary Particle Interactions, High Energy Interactions, Proton Scattering, Energy Dissipation, Energy Distribution, Neutrinos, Temperature Effects

Scientific paper

Possible proton collisions in cosmic ray sources are examined, and the operational domains of various proton collisions are suggested based on calculations of background temperature. The energy rate loss through the proton-neutrino process on protons is computed, and the energy distribution of the secondary particles involved in various collisions is discussed. Results are confirmed by the very high brightness temperature of 10 to the 23rd K, which has been recorded in pulsars.

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