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Title: Searching for dark matter annihilation in the Smith high-velocity cloud

Journal Article · · Astrophysical Journal
 [1];  [2];  [3];  [4];  [5]
  1. Center for Particle Astrophysics, Fermi National Accelerator Laboratory, Batavia, IL 60510 (United States)
  2. Departamento de Fisíca, Pontificia Universidad Católica de Chile, Avenida Vicuña Mackenna 4860, Santiago (Chile)
  3. CRESST, University of Maryland, Baltimore County, Baltimore, MD 21250 (United States)
  4. The Kavli Institute for Cosmological Physics, University of Chicago, Chicago, IL 60637 (United States)
  5. W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305 (United States)

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 γ-ray observations from the Fermi Large Area Telescope to search for a dark matter annihilation signal. No significant γ-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 (∼ 3 × 10{sup –26} cm{sup 3} s{sup –1}) for dark matter masses ≲ 30 GeV annihilating via the b b-bar or τ{sup +}τ{sup –} 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.

OSTI ID:
22365627
Journal Information:
Astrophysical Journal, Vol. 790, Issue 1; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 0004-637X
Country of Publication:
United States
Language:
English

Cited By (10)

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The Mopra Southern Galactic Plane CO Survey—Data Release 3 journal January 2018
Wavelet-based techniques for the gamma-ray sky journal July 2016
Strong optimized conservative Fermi-LAT constraints on dark matter models from the inclusive photon spectrum journal April 2015
Search for γ -ray emission from dark matter particle interactions from the Andromeda and Triangulum galaxies with the Fermi Large Area Telescope journal June 2019
Selection Rule for Enhanced Dark Matter Annihilation journal June 2017
Wimp searches with gamma rays in the Fermi era: Challenges, methods and results journal December 2015
WIMP searches with gamma rays in the Fermi era: challenges, methods and results text January 2015
Strong Optimized Conservative Fermi-LAT Constraints on Dark Matter Models from the Inclusive Photon Spectrum text January 2015
Model-independent analysis of the DAMPE excess text January 2017

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