Implications of a Light Gluino

Details Implications of a Light Gluino Implications of a Light Gluino

1993-11-05

arxiv.org/abs/hep-ph/9311231v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

talk given at the XVI Kazimierz Meeting on Elementary Particle Physics, Kazimierz (Poland) 24-28 May 1993, 4 pages in LATEX +

Scientific paper

We show that the possibility of having light gluinos is not in conflict with recent LEP measurements and also that cosmology does not rule it out in any convincing way. In unified N=1 supergravity models, one expects that also the "photino" will be light. Moreover it leads to $upper$ limits on the masses of the other supersymmetric fermions, for example, the lightest chargino should be lighter than about 75 GeV, an thus detectable at LEP200.

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