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 10 31 cm −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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Nath et al. (1987) studied this question.