Complementarity between direct and indirect searches of Dark Matter and the ILC
Yann Mambrini, Shaaban Khalil
Abstract
Yann Mambrini, Shaaban Khalil
Abstract
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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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.
Key concepts: WIMP, Dark matter, Physics, Xenon, Weakly interacting massive particles, Complementarity (molecular biology), Particle physics, Sensitivity (control systems)