Excess of EGRET Galactic Gamma Ray Data interpreted as Dark Matter Annihilation
W. de Boer, M. Herold, C. Sander, V. Zhukov, A.V. Gladyshev, D.I., Kazakov

TL;DR
The paper interprets the excess gamma ray data from EGRET as a potential signal of Dark Matter annihilation, constraining WIMP mass, halo structure, and supporting the supersymmetric dark matter hypothesis with high statistical significance.
Contribution
It provides a detailed analysis linking gamma ray excess to Dark Matter annihilation, constraining WIMP mass, halo shape, and correlating with galactic structures, which is a novel comprehensive interpretation.
Findings
Gamma ray excess consistent with Dark Matter annihilation spectrum
Halo structure is a triaxial isothermal profile with a DM ring at 14 kpc
Supports supersymmetric dark matter models with boost factors above 20
Abstract
The diffuse galactic EGRET gamma ray data show a clear excess for energies above 1 GeV in comparison with the expectations from conventional galactic models. The excess is seen with the same spectrum in all sky directions, as expected for Dark Matter (DM) annihilation. This hypothesis is investigated in detail. The energy spectrum of the excess is used to limit the WIMP mass to the 50-100 GeV range, while the sky maps are used to determine the halo structure, which is consistent with a triaxial isothermal halo with additional enhancement of Dark Matter in the disc. The latter is strongly correlated with the ring of stars around our galaxy at a distance of 14 kpc, thought to originate from the tidal disruption of a dwarf galaxy. It is shown that this ring of DM with a mass of causes the mysterious change of slope in the rotation curve at and…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Astrophysics and Cosmic Phenomena · Galaxies: Formation, Evolution, Phenomena
