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CONSTRAINTS ON THE GALACTIC HALO DARK MATTER FROM FERMI-LAT DIFFUSE MEASUREMENTS
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Number of Authors: 1412012 (English)In: Astrophysical Journal, ISSN 0004-637X, E-ISSN 1538-4357, Vol. 761, no 2, article id 91Article in journal (Refereed) Published
Abstract [en]

We have performed an analysis of the diffuse gamma-ray emission with the Fermi Large Area Telescope (LAT) in the Milky Way halo region, searching for a signal from dark matter annihilation or decay. In the absence of a robust dark matter signal, constraints are presented. We consider both gamma rays produced directly in the dark matter annihilation/decay and produced by inverse Compton scattering of the e(+)/e(-) produced in the annihilation/decay. Conservative limits are derived requiring that the dark matter signal does not exceed the observed diffuse gamma-ray emission. A second set of more stringent limits is derived based on modeling the foreground astrophysical diffuse emission using the GALPROP code. Uncertainties in the height of the diffusive cosmic-ray halo, the distribution of the cosmic-ray sources in the Galaxy, the index of the injection cosmic-ray electron spectrum, and the column density of the interstellar gas are taken into account using a profile likelihood formalism, while the parameters governing the cosmic-ray propagation have been derived from fits to local cosmic-ray data. The resulting limits impact the range of particle masses over which dark matter thermal production in the early universe is possible, and challenge the interpretation of the PAMELA/Fermi-LAT cosmic ray anomalies as the annihilation of dark matter.

Place, publisher, year, edition, pages
2012. Vol. 761, no 2, article id 91
Keywords [en]
dark matter, Galaxy: halo, gamma rays: diffuse background, methods: statistical
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:su:diva-161716DOI: 10.1088/0004-637X/761/2/91ISI: 000312090300010OAI: oai:DiVA.org:su-161716DiVA, id: diva2:1262921
Available from: 2018-11-13 Created: 2018-11-13 Last updated: 2018-11-13Bibliographically approved

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Ajello, M.Baldini, L.Bastieri, D.Buehler, R.Caraveo, P. A.Conrad, Jan M.Cuoco, AlessandroCutini, S.do Couto e Silva, E.Fukazawa, Y.Funk, S.Gargano, F.Gasparrini, D.Giroletti, M.Johannesson, G.Garde, M. LlenaLoparco, F.Mazziotta, M. N.Morselli, A.Moskalenko, I. V.Pesce-Rollins, M.Rando, R.Reimer, A.Reimer, O.Spandre, G.Takahashi, H.Tibaldo, L.Tosti, G.Vianello, G.Yang, ZhaoyuZaharijas, GabrijelaZimmer, Stephan
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Department of PhysicsThe Oskar Klein Centre for Cosmo Particle Physics (OKC)
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