Dark Matter Halos and the Anisotropy of Ultra-High Energy Cosmic Rays in the Pierre Auger Observatory
We analyze the cosmic ray arrival direction map that would be observed if the source of ultra high energycosmic rays were the decay of dark matter particles in the halos of our galaxy and of the Andromeda galaxy(M31). To model the dark matter distribution throughout the halos we use two different de...
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| Publicat a: | Brazilian Journal of Physics |
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| Autors principals: | , , , |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Sociedade Brasileira de Física
2007
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| Matèries: | |
| Accés en línia: | https://www.redalyc.org/articulo.oa?id=46437116 |
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