{ "id": "1006.1628", "version": "v1", "published": "2010-06-08T18:03:25.000Z", "updated": "2010-06-08T18:03:25.000Z", "title": "Fermi-LAT Sensitivity to Dark Matter Annihilation in Via Lactea II Substructure", "authors": [ "Brandon Anderson", "Michael Kuhlen", "Robert Johnson", "Piero Madau", "Juerg Diemand" ], "comment": "16 pages, 6 figures", "categories": [ "astro-ph.HE" ], "abstract": "We present a study of the ability of the Fermi Gamma-ray Space Telescope to detect dark-matter annihilation signals from the Galactic subhalos predicted by the Via Lactea II N-body simulation. We implement an improved formalism for estimating the boost factor needed to account for the effect of dark-matter clumping on scales below the resolution of the simulation, and we incorporate a detailed Monte Carlo simulation of the response of the Fermi-LAT telescope, including a simulation of its all-sky observing mode integrated over a ten year mission. We find that for WIMP masses up to about 150 GeV in standard supersymmetric models with velocity-averaged cross section 3*10^-26 cm^3 s^-1, a few subhalos could be detectable with >5 standard deviations significance and would likely deviate significantly from the appearance of a point source.", "revisions": [ { "version": "v1", "updated": "2010-06-08T18:03:25.000Z" } ], "analyses": { "keywords": [ "dark matter annihilation", "fermi-lat sensitivity", "fermi gamma-ray space telescope", "detect dark-matter annihilation signals", "substructure" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/0004-637X/718/2/899", "journal": "The Astrophysical Journal", "year": 2010, "month": "Aug", "volume": 718, "number": 2, "pages": 899 }, "note": { "typesetting": "TeX", "pages": 16, "language": "en", "license": "arXiv", "status": "editable", "inspire": 857564, "adsabs": "2010ApJ...718..899A" } } }