Particle Dark Matter Searches Outside the Local Group
Journal
Date Issued
2015
Author(s)
Regis, Marco
•
Xia, Jun-Qing
•
Cuoco, Alessandro
•
•
Fornengo, Nicolao
•
Abstract
If dark matter (DM) is composed by particles which are nongravitationally coupled to ordinary matter, their annihilations or decays in cosmic structures can result in detectable radiation. We show that the most powerful technique to detect a particle DM signal outside the Local Group is to study the angular cross-correlation of nongravitational signals with low-redshift gravitational probes. This method allows us to enhance the signal to noise from the regions of the Universe where the DM-induced emission is preferentially generated. We demonstrate the power of this approach by focusing on GeV-TeV DM and on the recent cross-correlation analysis between the 2MASS galaxy catalogue and the Fermi-LAT γ -ray maps. We show that this technique is more sensitive than other extragalactic γ -ray probes, such as the energy spectrum and angular autocorrelation of the extragalactic background, and emission from clusters of galaxies. Intriguingly, we find that the measured cross-correlation can be well fitted by a DM component, with a thermal annihilation cross section and mass between 10 and 100 GeV, depending on the small-scale DM properties and γ -ray production mechanism. This solicits further data collection and dedicated analyses.
Volume
114
Issue
24
Start page
241301
Issn Identifier
0031-9007
Ads BibCode
2015PhRvL.114x1301R
Rights
open.access
File(s)![Thumbnail Image]()
Loading...
Name
1503.05922.pdf
Size
596.64 KB
Format
Adobe PDF
Checksum (MD5)
f50cfe04ebe73abc6e12c08ec362576d