{ "id": "1310.8230", "version": "v1", "published": "2013-10-30T17:00:28.000Z", "updated": "2013-10-30T17:00:28.000Z", "title": "Cosmic Rays from Heavy Dark Matter from the Galactic Center", "authors": [ "Jose A. R. Cembranos", "Viviana Gammaldi", "Antonio L. Maroto" ], "comment": "Proceedings of the European Physical Society Conference on High Energy Physics EPS-HEP2013, 18-24 July 2013, Stockholm (Sweden)", "categories": [ "astro-ph.HE", "hep-ph" ], "abstract": "The gamma-ray fluxes observed by the High Energy Stereoscopic System (HESS) from the J1745-290 Galactic Center source is well fitted by the secondary photons coming from Dark Matter (DM) annihilation in particle-antiparticle standard model pairs over a diffuse power-law background. The spectral features of the signal are consistent with different channels: light quarks, electro-weak gauge bosons and top-antitop production. The amount of photons and morphology of the signal localized within a region of few parsecs, require compressed DM profiles as those resulting from baryonic contraction, which offer large enhancements in the signal over DM alone simulations. The fits return a heavy WIMP, with a mass above 10 TeV, but well below the unitarity limit for thermal relic annihilation. The fitted background spectral index is compatible with the Fermi-Large Area Telescope (LAT) data from the same region. This possibility can be potentially tested with the observations of other high energy cosmic rays.", "revisions": [ { "version": "v1", "updated": "2013-10-30T17:00:28.000Z" } ], "analyses": { "keywords": [ "heavy dark matter", "galactic center", "high energy stereoscopic system", "high energy cosmic rays", "particle-antiparticle standard model pairs" ], "tags": [ "conference paper" ], "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1262679, "adsabs": "2013ehep.confE.103C" } } }