Lars Bergström1, Torsten Bringmann, Martin Eriksson
1Department of Physics, Stockholm University, AlbaNova University Center, SE-106 91 Stockholm, Sweden. lbe@physto.se
Kaluza-Klein (KK) dark matter annihilations may explain the TeV gamma-ray signal from the Galactic center. A 1 TeV KK particle fits HESS data, while a 10 TeV particle explains relic density and the full photon spectrum.
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