Gamma ray line production from cosmic ray spallation reactions

Details Gamma ray line production from cosmic ray spallation reactions Gamma ray line production from cosmic ray spallation reactions

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....1..369s&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 1 p 369-372 (SEE N85-33902 22-93)

Computer Science

Cosmic Rays, Gamma Rays, Nuclear Interactions, Particle Collisions, Accretion Disks, Atomic Excitations, Binary Stars, Clouds, Galactic Radiation, Line Spectra, Pulsars

Scientific paper

The gamma-ray line intensities due to cosmic-ray spallation reactions in clouds, the galactic disk and accreting binary pulsars are calculated. With the most favorable plausible assumptions, only a few lines may be detectable at the level of 10-6per cm2sec. The intensites are compared with those generated in nuclear excitation reactions.

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