Searching for Dark Matter Annihilation in the Smith High-Velocity Cloud
arXiv:1405.1030 · doi:10.1088/0004-637X/790/1/24
Abstract
Recent observations suggest that some high-velocity clouds may be confined by massive dark matter halos. In particular, the proximity and proposed dark matter content of the Smith Cloud make it a tempting target for the indirect detection of dark matter annihilation. We argue that the Smith Cloud may be a better target than some Milky Way dwarf spheroidal satellite galaxies and use gamma-ray observations from the Fermi Large Area Telescope to search for a dark matter annihilation signal. No significant gamma-ray excess is found coincident with the Smith Cloud, and we set strong limits on the dark matter annihilation cross section assuming a spatially-extended dark matter profile consistent with dynamical modeling of the Smith Cloud. Notably, these limits exclude the canonical thermal relic cross section () for dark matter masses GeV annihilating via the or channels for certain assumptions of the dark matter density profile; however, uncertainties in the dark matter content of the Smith Cloud may significantly weaken these constraints.
7 pages, 5 figures. Published in ApJ
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- The Mopra Southern Galactic Plane CO Survey - Data Release 3
- Search for -ray emission from dark matter particle interactions from Andromeda and Triangulum Galaxies with the Fermi Large Area Telescope
- Simplified Dark Matter Models Confront the Gamma Ray Excess
- Strong Optimized Conservative Fermi-LAT Constraints on Dark Matter Models from the Inclusive Photon Spectrum
- TeV Dark Matter Searches in the Extragalactic Gamma-Ray Sky
- Search for gamma-ray line features from Milky Way satellites with Fermi-LAT Pass 8 data
- Dark matter properties implied by gamma ray interstellar emission models