SUPERSYMMETRIC SIGNALS AT THE TEVATRON

Abstract
The possibility of detecting SUSY signals arising from Wino and Zino production at the Tevatron is examined. If the Tevatron is operated at peak luminosity of 1031cm−2 sec −1 with full lepton detection capabilities, we estimate for a UA1 type apparatus that the trilepton signal is sensitive to Winos with mass up to ≈70–80 GeV , the dilepton signal up to ≈50–60 GeV and the monojet signal up to ≈45–50 GeV .

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