{ "id": "1507.06129", "version": "v1", "published": "2015-07-22T11:13:20.000Z", "updated": "2015-07-22T11:13:20.000Z", "title": "Towards a realistic astrophysical interpretation of the Galactic center excess", "authors": [ "Daniele Gaggero", "Marco Taoso", "Alfredo Urbano", "Mauro Valli", "Piero Ullio" ], "comment": "24 pages, 10 figures", "categories": [ "astro-ph.HE", "hep-ph" ], "abstract": "A spherical-symmetric gamma-ray emission from the central region of the Galaxy has been recently identified in Fermi-LAT data, and initially associated to dark matter particle annihilations. Guided by the evidence for a high gas density in the inner kpc of the Galaxy correlated with a very large Supernova rate, and hence with ongoing cosmic-ray acceleration, we investigate instead the possibility of addressing this excess in terms of ordinary cosmic-ray sources and standard steady-state diffusion. We introduce the new ingredient in the context of the template-fitting algorithm, treating the new contribution as correlated to the conventional Inverse Compton emission. We analyze in detail the overall goodness of the fit of our framework, and perform a detailed direct comparison against data examining profiles in different directions.", "revisions": [ { "version": "v1", "updated": "2015-07-22T11:13:20.000Z" } ], "analyses": { "keywords": [ "galactic center excess", "realistic astrophysical interpretation", "conventional inverse compton emission", "dark matter particle annihilations", "spherical-symmetric gamma-ray emission" ], "publication": { "doi": "10.1088/1475-7516/2015/12/056", "journal": "Journal of Cosmology and Astro-Particle Physics", "year": 2015, "month": "Dec", "volume": 2015, "number": 12, "pages": "056" }, "note": { "typesetting": "TeX", "pages": 24, "language": "en", "license": "arXiv", "status": "editable", "adsabs": "2015JCAP...12..056G", "inspire": 1384253 } } }