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Constraints on WIMP annihilation for contracted dark matter in the inner Galaxy with the Fermi-LAT

Gómez-Vargas, G.A.; Sanchez-Conde, M.A.; Huh, J.H.; Peiró, M.; Prada, F.; Morselli, A.; Klypin, A.; Cerdeno, D.G.; Mambrini, Y.; Munoz, C.

Constraints on WIMP annihilation for contracted dark matter in the inner Galaxy with the Fermi-LAT Thumbnail


Authors

G.A. Gómez-Vargas

M.A. Sanchez-Conde

J.H. Huh

M. Peiró

F. Prada

A. Morselli

A. Klypin

D.G. Cerdeno

Y. Mambrini

C. Munoz



Abstract

We derive constraints on parameters of generic dark matter candidates by comparing theoretical predictions with the gamma-ray emission observed by the Fermi-LAT from the region around the Galactic Center. Our analysis is conservative since it simply requires that the expected dark matter signal does not exceed the observed emission. The constraints obtained in the likely case that the collapse of baryons to the Galactic Center is accompanied by the contraction of the dark matter are strong. In particular, we find that for bbar b and τ+τ− or W+W− dark matter annihilation channels, the upper limits on the annihilation cross section imply that the thermal cross section is excluded for a Weakly Interacting Massive Particle (WIMP) mass smaller than about 700 and 500 GeV, respectively. For the μ+μ− channel, where the effect of the inverse Compton scattering is important, depending on models of the Galactic magnetic field the exclusion of the thermal cross-section is for a WIMP mass smaller than about 150 to 400 GeV. The upper limits on the annihilation cross section of dark matter particles obtained are two orders of magnitude stronger than without contraction. In the latter case our results are compatible with the upper limits from the Galactic halo analysis reported by the Fermi-LAT collaboration for the case in which the same conservative approach without modeling of the astrophysical background is employed.

Citation

Gómez-Vargas, G., Sanchez-Conde, M., Huh, J., Peiró, M., Prada, F., Morselli, A., …Munoz, C. (2013). Constraints on WIMP annihilation for contracted dark matter in the inner Galaxy with the Fermi-LAT. Journal of Cosmology and Astroparticle Physics, 2013(10), Article 029. https://doi.org/10.1088/1475-7516/2013/10/029

Journal Article Type Article
Acceptance Date Sep 5, 2013
Online Publication Date Oct 16, 2013
Publication Date Oct 16, 2013
Deposit Date Nov 27, 2016
Publicly Available Date Dec 1, 2016
Journal Journal of Cosmology and Astroparticle Physics
Publisher IOP Publishing
Peer Reviewed Peer Reviewed
Volume 2013
Issue 10
Article Number 029
DOI https://doi.org/10.1088/1475-7516/2013/10/029
Public URL https://durham-repository.worktribe.com/output/1392317
Related Public URLs https://arxiv.org/abs/1308.3515

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Copyright Statement
This is an author-created, un-copyedited version of an article published in Journal of cosmology and astroparticle physics. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at 10.1088/1475-7516/2013/10/029






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