Complementarity between direct and indirect searches of Dark Matter and the ILC

Details Complementarity between direct and indirect searches of Dark Matter and the ILC Complementarity between direct and indirect searches of Dark Matter and the ILC

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1115..347m&link_type=abstract

THE DARK SIDE OF THE UNIVERSE: 4th International Workshop on the Dark Side of the Universe. AIP Conference Proceedings, Volume

Computer Science

Dark Matter, Supersymmetry, Cosmology

Scientific paper

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 mχ<~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 σχ-p<~10-8 pb. We also predict the production rate 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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