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

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dc.creatorZhang, C.
dc.creatorLiu, G. -C.
dc.date2008-12-31
dc.date.accessioned2026-07-07T12:31:55Z
dc.date.available2026-07-07T12:31:55Z
dc.descriptionBased 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.
dc.identifierhttps://arxiv.org/abs/0901.0059
dc.identifierhttp://arxiv.org/abs/0901.0059
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/216614
dc.subjectHigh Energy Astrophysical Phenomena
dc.titleDark Matter Annihilation Induced Gamma Ray Emission from Galaxy Cluster 1E0657-56
dc.typetext

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