Abstract
By taking the mixing of the neutralinos into account, we discuss the production of the lightest neutralinos Ñ's in e + e − → γ N ̃ N ̃ . We find that, due to the radiative decay of the next lightest neutralino, the supersymmetric signal in “γ + unobserved neutrals” events in e +e − annihilation — even near the Z 0 pole — may be clearly distinguished from the background coming from e +− → γυ υ .
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