{ "id": "1512.04966", "version": "v1", "published": "2015-12-15T21:17:21.000Z", "updated": "2015-12-15T21:17:21.000Z", "title": "The Gamma-Ray Luminosity Function of Millisecond Pulsars and Implications for the GeV Excess", "authors": [ "Dan Hooper", "Gopolang Mohlabeng" ], "comment": "10 pages, 8 figures", "categories": [ "astro-ph.HE", "astro-ph.CO", "astro-ph.GA", "hep-ph" ], "abstract": "It has been proposed that a large population of unresolved millisecond pulsars (MSPs) could potentially account for the excess of GeV-scale gamma-rays observed from the region surrounding the Galactic Center. The viability of this scenario depends critically on the gamma-ray luminosity function of this source population, which determines how many MSPs Fermi should have already detected as resolved point sources. In this paper, we revisit the gamma-ray luminosity function of MSPs, without relying on uncertain distance measurements. Our determination, based on a comparison of models with the observed characteristics of the MSP population, suggests that Fermi should have already detected a significant number of sources associated with such a hypothesized Inner Galaxy population. We cannot rule out a scenario in which the MSPs residing near the Galactic Center are systematically less luminous than those present in the Galactic Plane or within globular clusters.", "revisions": [ { "version": "v1", "updated": "2015-12-15T21:17:21.000Z" } ], "analyses": { "keywords": [ "gamma-ray luminosity function", "millisecond pulsars", "gev excess", "implications", "galactic center" ], "publication": { "doi": "10.1088/1475-7516/2016/03/049", "journal": "Journal of Cosmology and Astro-Particle Physics", "year": 2016, "month": "Mar", "volume": 2016, "number": 3, "pages": "049" }, "note": { "typesetting": "TeX", "pages": 10, "language": "en", "license": "arXiv", "status": "editable", "adsabs": "2016JCAP...03..049H", "inspire": 1409878 } } }