Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/102357
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Type: Journal article
Title: Constraints on an annihilation signal from a core of constant dark matter density around the milky way center with H.E.S.S.
Author: Abramowski, A.
Aharonian, F.
Ait Benkhali, F.
Akhperjanian, A.
Angüner, E.
Backes, M.
Balenderan, S.
Balzer, A.
Barnacka, A.
Becherini, Y.
Becker Tjus, J.
Berge, D.
Bernhard, S.
Bernlöhr, K.
Birsin, E.
Biteau, J.
Böttcher, M.
Boisson, C.
Bolmont, J.
Bordas, P.
et al.
Citation: Physical Review Letters, 2015; 114(8):081301-1-081301-6
Publisher: American Physical Society
Issue Date: 2015
ISSN: 0031-9007
1079-7114
Statement of
Responsibility: 
A. Abramowski … G. Rowell … et al. (for the H.E.S.S. Collaboration)
Abstract: An annihilation signal of dark matter is searched for from the central region of the Milky Way. Data acquired in dedicated on-off observations of the Galactic center region with H.E.S.S. are analyzed for this purpose. No significant signal is found in a total of ∼9 h of on-off observations. Upper limits on the velocity averaged cross section, hσvi, for the annihilation of dark matter particles with masses in the range of ∼300 GeV to ∼10 TeV are derived. In contrast to previous constraints derived from observations of the Galactic center region, the constraints that are derived here apply also under the assumption of a central core of constant dark matter density around the center of the Galaxy. Values of hσvi that are larger than 3 × 10−24 cm3=s are excluded for dark matter particles with masses between ∼1 and ∼4 TeV at 95% C.L. if the radius of the central dark matter density core does not exceed 500 pc. This is the strongest constraint that is derived on hσvi for annihilating TeV mass dark matter without the assumption of a centrally cusped dark matter density distribution in the search region.
Keywords: (H.E.S.S. Collaboration)
Rights: © 2015 American Physical Society
RMID: 0030025837
DOI: 10.1103/PhysRevLett.114.081301
Published version: http://journals.aps.org/prl/abstract/10.1103/PhysRevLett.114.081301
Appears in Collections:Physics publications

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