Search for charginos, neutralinos and gravitinos at LEP
1998
An update of the searches for
charginosand
neutralinosin DELPHI is presented, based mainly on recent data collected at centre-of-mass energies of 161 GeV and 172 GeV. No signal is found. For a sneutrino with mass above 300 GeV/c2 and a mass difference between the
charginoand the lightest
neutralinoabove 10 GeV/c2, the lower limit at 95% confidence level on the
charginomass ranges from 84.3 GeV/c2 to the kinematical limit (86.0 GeV/c2), depending on the mixing parameters. The limit decreases for lower
chargino-
neutralinomass differences. The limit in the case of a light sneutrino is 67.6 GeV/c2, provided that that there is no light sneutrino with a mass within 10 GeV/c2 below the
charginomass. Upper limits on
neutralino
pair productioncross-sections of about a picobarn are derived. The (μ,M2) domain excluded in the MSSM-GUT scenario is determined by combining the
neutralinoand
charginosearches. These results imply a limit on the mass of the lightest
neutralinowhich, for a heavy sneutrino, is constrained to be above 24.9 GeV/c2 for tans >- 1. The search has also been extended to the case where the lightest
neutralinois unstable and decays into a photon and a
gravitino. imply a limit on the mass of the lightest
neutralinowhich, for a heavy sneutrino, is constrained to be above 24.9 GeV/c2 for tans >- 1. The search has also been extended to the case where the lightest
neutralinois unstable and decays into a photon and a
gravitino.
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