Search for dark matter annihilations towards the inner Galactic halo from 10 years of observations with H.E.S.S

Abstract

The inner region of the Milky Way halo harbors a large amount of dark matter (DM). Given its proximity, it is one of the most promising targets to look for DM. We report on a search for the annihilations of DM particles using $\gamma$-ray observations towards the inner 300 parsecs of the Milky Way, with the H.E.S.S. array of ground-based Cherenkov telescopes. The analysis is based on a 2D maximum likelihood method using Galactic center (GC) data accumulated by H.E.S.S. over the last 10 years (2004-2014), and does not show any significant $\gamma$-ray signal above background. Assuming Einasto and Navarro-Frenk-White DM density profiles at the GC, we derive upper limits on the annihilation cross section $⟨\sigma v⟩$. These constraints are the strongest obtained so far in the TeV DM mass range and improve upon previous limits by a factor 5. For the Einasto profile, the constraints reach $⟨\sigma v⟩$ values of $6\times 10^{-26}\mathrm{c}{\mathrm{m}}^3{\mathrm{s}}^{-1}$ in the $W^{+}{W}^{-}$ channel for a DM particle mass of 1.5 TeV, and $2\times 10^{-26}\mathrm{c}{\mathrm{m}}^3{\mathrm{s}}^{-1}$ in the ${\tau }^{+}{\tau }^{-}$ channel for 1 TeV mass. For the first time, ground-based $\gamma$-ray observations have reached sufficient sensitivity to probe $⟨\sigma v⟩$ values expected from the thermal relic density for TeV DM particles.

arXiv commentAccepted by PRL. Includes Supplemental Material. 7+4 pages, 2+4 figures, 1 table

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