Determining the WIMP mass using the complementarity between direct and indirect searches and the ILC

Details Determining the WIMP mass using the complementarity between direct and indirect searches and the ILC Determining the WIMP mass using the complementarity between direct and indirect searches and the ILC

2008-04-14

arxiv.org/abs/0804.1976v2

JCAP 0901:046,2009

Physics

High Energy Physics

High Energy Physics - Phenomenology

32 pages, new figures and a more detailed statistical analysis. Final version to appear in JCAP

Scientific paper

10.1088/1475-7516/2009/01/046

We study the possibility of identifying dark matter properties from XENON-like 100 kg experiments and the GLAST satellite mission. We show that whereas direct detection experiments will probe efficiently light WIMPs, given a positive detection (at the 10% level for $m_{\chi} \lesssim 50$ GeV), GLAST will be able to confirm and even increase the precision in the case of a NFW profile, for a WIMP-nucleon cross-section $\sigma_{\chi-p} \lesssim 10^{-8}$ pb. We also predict the rate of production of a WIMP in the next generation of colliders (ILC), and compare their sensitivity to the WIMP mass with the XENON and GLAST projects.

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