Direct and indirect detections of dark matter in the Littlest Higgs model with T-parity

Details Direct and indirect detections of dark matter in the Littlest Higgs model with T-parity Direct and indirect detections of dark matter in the Littlest Higgs model with T-parity

Nov 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..878..188m&link_type=abstract

THE DARK SIDE OF THE UNIVERSE: 2nd International Conference on The Dark Side of the Universe DSU 2006. AIP Conference Proceedin

Mathematics

Logic

Dark Matter

Scientific paper

The Littlest Higgs model with T-parity is one of the scenario which describes physics beyond the standard model of particle physics. Recently, this model attracts attention, because it can solve the Little hierarchy problem without supersymmetry. Furthermore, this model provides the WIMP dark matter candidate, thus it can also solve the cosmological dark matter problem. In this letter, we discuss the possibility to detect the dark matter in direct and indirect detection measurements. We point out that the most promising way to detect the dark matter is the use of the cosmic positrons. In future experiments such as the PAMELA and AMS-02, the dark matter will be found when its mass is O (100) GeV.

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