Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/69076
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Type: Journal article
Title: Search for a dark matter annihilation signal from the galactic center halo with H.E.S.S.
Author: Maxted, N.
Nicholas, B.
Rowell, G.
Citation: Physical Review Letters, 2011; 106(16):161301-1-161301-5
Publisher: American Physical Soc
Issue Date: 2011
ISSN: 0031-9007
1079-7114
Statement of
Responsibility: 
A. Abramowski... N. Maxted... B. Nicholas... G. Rowell... et al. (H.E.S.S. Collaboration)
Abstract: A search for a very-high-energy (VHE;≥ 100 GeV) γ-ray signal from self-annihilating particle dark matter (DM) is performed towards a region of projected distance r∼45–150 pc from the Galactic center. The background-subtracted -ray spectrum measured with the High Energy Stereoscopic System (H.E.S.S.) γ-ray instrument in the energy range between 300 GeVand 30 TeV shows no hint of a residual γ-ray flux. Assuming conventional Navarro-Frenk-White and Einasto density profiles, limits are derived on the velocity-weighted annihilation cross section (σv)as a function of the DM particle mass. These are among the best reported so far for this energy range and in particular differ only little between the chosen density profile parametrizations. In particular, for the DM particle mass of 1 TeV, values for h (σv) above 3x10⁻²⁵ cm³ s⁻1 are excluded for the Einasto density profile.
Keywords: H.E.S.S. Collaboration
Rights: ©2011 American Physical Society
RMID: 0020106665
DOI: 10.1103/PhysRevLett.106.161301
Appears in Collections:IPAS publications

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