Abstract
We propose that the 3.2 sigma excess at ~150 GeV in the dijet mass spectrum of W + jets reported by CDF is the technipion of low-scale technicolor. Its relatively large cross section is due to production of a narrow resonance, the technirho, which decays to W + . We discuss ways to enhance and strengthen the technicolor hypothesis and suggest companion searches at the Tevatron and LHC.
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