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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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Argitaratua izan da:Brazilian Journal of Physics
Egile Nagusiak: Beatriz B. Siffert, B. Lazarotto, J. R. T. de Mello Neto, Angela Olinto
Formatua: Artigo
Hizkuntza:Inglês
Argitaratua: Sociedade Brasileira de Física 2007
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Sarrera elektronikoa:https://www.redalyc.org/articulo.oa?id=46413544016
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