Astronomy and Astrophysics – Astrophysics
Scientific paper
2000-05-04
Mon.Not.Roy.Astron.Soc. 323 (2001) 391
Astronomy and Astrophysics
Astrophysics
Submitted for publication
Scientific paper
10.1046/j.1365-8711.2001.04246.x
We explore the possibility that the diffuse gamma-ray background radiation (GBR) at high galactic latitudes could be dominated by inverse Compton scattering of cosmic ray (CR) electrons on the cosmic microwave background radiation and on starlight from our own galaxy. Assuming that the mechanisms accelerating galactic CR hadrons and electrons are the same, we derive simple and successful relations between the spectral indices of the GBR above a few MeV, and of the CR electrons and CR nuclei above a few GeV. We reproduce the observed intensity and angular dependence of the GBR, in directions away from the galactic disk and centre, without recourse to hypothetical extragalactic sources.
Dar Arnon
de Rujula Alvaro
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