Secondary to primary ratio and the continuous acceleration

Details Secondary to primary ratio and the continuous acceleration Secondary to primary ratio and the continuous acceleration

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....3..234g&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 3 p 234-237 (SEE N85-34862 23-93)

Astronomy and Astrophysics

Astronomy

2

Interstellar Matter, Particle Acceleration, Primary Cosmic Rays, Secondary Cosmic Rays, Astronomical Models, Celestial Bodies, Particle Production

Scientific paper

A general formula for the sec/prim ratio, independently of any details of the propagation and acceleration model is presented. In the limit of equal fragmentation paths for primaries and secondaries, this ratio at a given momentum nucleon is proportional only to the mean path of the observed primaries at that moment. It is shown that it is unlikely to get a decreasing sec/prim ratio with energy if an acceleration process takes place during particle propagation in the interstellar medium (ISM).

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