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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 energy cosmic 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...

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Bibliografski detalji
Izdano u:Brazilian Journal of Physics
Glavni autori: Beatriz B. Siffert, B. Lazarotto, J. R. T. de Mello Neto, Angela Olinto
Format: Artigo
Jezik:Inglês
Izdano: Sociedade Brasileira de Física 2007
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Online pristup:https://www.redalyc.org/articulo.oa?id=46413544016
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