Dark Matter Annihilation Induced Gamma Ray Emission from Galaxy Cluster 1E0657-56

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Based on minimal supersymmetric standard model, neutralino dark matter annihilation induced gamma ray emission from galaxy cluster 1E0657-56 is calculated. The merge of bullet-like subcluster with the main cluster is also investigated.

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High Energy Astrophysical Phenomena

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http://salesiana.dossiersoluciones.com/handle/123456789/216614

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/0901.0059
 http://arxiv.org/abs/0901.0059

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arXiv