Vector WIMP miracle |
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Authors: | Tomohiro Abe Mitsuru Kakizaki Shigeki Matsumoto Osamu Seto |
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Affiliation: | 1. Institute of Modern Physics and Center for High Energy Physics, Tsinghua University, Beijing 100084, China;2. Department of Physics, University of Toyama, Toyama, Japan;3. IPMU, TODIAS, University of Tokyo, Kashiwa, Japan;4. Department of Architecture and Building Engineering, Hokkai-Gakuen University, Sapporo, Japan |
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Abstract: | Weakly interacting massive particle (WIMP) is well known to be a good candidate for dark matter, and it is also predicted by many new physics models beyond the standard model at the TeV scale. We found that, if the WIMP is a vector particle (spin-one particle) which is associated with some gauge symmetry broken at the TeV scale, the Higgs mass is often predicted to be 120–125 GeV, which is very consistent with the result of Higgs searches recently reported by ATLAS and CMS Collaborations at the Large Hadron Collider experiment. In this Letter, we consider the vector WIMP using a non-linear sigma model in order to confirm this result as general as possible in a bottom-up approach. Near-future prospects to detect the vector WIMP at both direct and indirect detection experiments of dark matter are also discussed. |
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