Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2011-10-27
JCAP 1201:041,2012
Physics
High Energy Physics
High Energy Physics - Phenomenology
19 pages, 5 figures; v3: Matches JCAP version; includes discussion of numerical studies of the density profile of MW-type halo
Scientific paper
10.1088/1475-7516/2012/01/041
We examine the constraints on models of weakly interacting massive particle (WIMP) dark matter from the recent observations of the Galactic center by the High Energy Spectroscopic System (HESS) telescope. We analyze canonical WIMP annihilation into Standard Model particle final states, including b/b-bar, t/t-bar and W^+ W^-. The constraints on annihilation into b/b-bar is within an order of magnitude of the thermal cross section at ~3 TeV, while the tau^+/tau^- channel is within a factor of ~2 of thermal. We also study constraints on Sommerfeld-enhanced dark matter annihilation models, and find that the gamma-ray observational constraints here rule out all of the parameter space consistent with dark matter annihilation interpretations of PAMELA and the Fermi-LAT e^+/e^- spectrum, in specific classes of models, and strongly constrains these interpretations in other classes. The gamma-ray constraints we find are more constraining on these models, in many cases, than current relic density, cosmic microwave background, halo shape and naturalness constraints.
Abazajian Kevork N.
Harding Patrick J.
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