Gamma Rays from the Galactic Halo

Details Gamma Rays from the Galactic Halo Gamma Rays from the Galactic Halo

Jun 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000nuphs..87..430j&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 87, Issue 1-3, p. 430-432.

Physics

Nuclear Physics

Scientific paper

A re-analysis of the EGRET data by Dixon et al. [1] has shown the existence of a statistically significant diffuse γ-ray emission from the galactic halo. This emission is naturally explained within a previously-proposed model for baryonic dark matter, in which γ-rays are produced through the interaction of high-energy cosmic-ray protons with cold gas clouds clumped along with brown dwarfs into dark clusters. These dark clusters supposedly populate the outer galactic halo and can show up in microlensing observations

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