{ "id": "astro-ph/0307209", "version": "v2", "published": "2003-07-10T13:12:14.000Z", "updated": "2003-11-17T11:34:00.000Z", "title": "On Dark Matter Annihilation in the Local Group", "authors": [ "Lidia Pieri", "Enzo Branchini" ], "comment": "11 pages, 10 figures. Accepted for publication in Phys. Rev. D.; added a new paragraph on the detectability of Galactic sub-halos in our Galaxy; added a discussion on their model dependence. The relation of our results with the \"CDM crisis\" issue has also been added", "journal": "Phys.Rev.D69:043512,2004", "doi": "10.1103/PhysRevD.69.043512", "categories": [ "astro-ph", "hep-ph" ], "abstract": "Under the hypothesis of a Dark Matter composed by supersymmetric particles like neutralinos, we investigate the possibility that their annihilation in the haloes of nearby galaxies could produce detectable fluxes of $\\gamma$-photons. Expected fluxes depend on several, poorly known quantities such as the density profiles of Dark Matter haloes, the existence and prominence of central density cusps and the presence of a population of sub-haloes. We find that, for all reasonable choices of Dark Matter halo models, the intensity of the $\\gamma$-ray flux from some of the nearest extragalactic objects, like M31, is comparable or higher than the diffuse Galactic foreground. We show that next generation ground-based experiments could have the sensitivity to reveal such fluxes which could help us unveiling the nature of Dark Matter particles.", "revisions": [ { "version": "v2", "updated": "2003-11-17T11:34:00.000Z" } ], "analyses": { "subjects": [ "98.70.Rz", "98.56.-p", "95.35.+d" ], "keywords": [ "dark matter annihilation", "local group", "dark matter halo models", "nearest extragalactic objects", "dark matter particles" ], "tags": [ "journal article" ], "publication": { "publisher": "APS", "journal": "Phys. Rev. D" }, "note": { "typesetting": "TeX", "pages": 11, "language": "en", "license": "arXiv", "status": "editable", "inspire": 623177 } } }