The Influence of the Energy Dependence of the Diffusion Coefficient on the Spectrum of the Electron Component of Cosmic Rays and the Radio Background Radiation of the Galaxy

Details The Influence of the Energy Dependence of the Diffusion Coefficient on the Spectrum of the Electron Component of Cosmic Rays and the Radio Background Radiation of the Galaxy The Influence of the Energy Dependence of the Diffusion Coefficient on the Spectrum of the Electron Component of Cosmic Rays and the Radio Background Radiation of the Galaxy

Aug 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974ap%26ss..29..305b&link_type=abstract

Astrophysics and Space Science, Volume 29, Issue 2, pp.305-318

Astronomy and Astrophysics

Astrophysics

28

Scientific paper

The diffusion of electrons through interstellar space, and the energy dependence of the diffusion coefficient are considered. Apart from the caseD=const the spectral index for electrons with spectral index γ0 changes according to γ0+μ→γ0+½μ+½→γ0+1 (D(E)=D0(E/E0)μ) for μ<1; for μ>1 to γ0+1→γ0+½μ+½→γ0+μ. We consider the radio emission spectrum in such a case. From a comparison with observations the limit μ≤0.4 is obtained.

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