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Is a Light Gluino Compatible with N=1 Supersymmetry?

1994/08/18 by M. A. Díaz, Marco Aurelio Diaz, Diaz, Marco Aurelio
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #Particle physics theoretical and experimental studies #hep-ph

paper · pdf · doi:10.48550/arxiv.hep-ph/9408329

15 pages, plain tex, 5 figures not included, VAND-TH-94-13

arxiv created 1994/08/18 · openalex publication_date 1994/08/18 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

Using the new CLEO bound on the branching ratio of the decay mode b\longrightarrow sγ given by 1×10-4< B(b\longrightarrow sγ)<4×10-4 at 95% c.l., and the experimental bounds on the masses of the lightest chargino, the second lightest neutralino, and the light CP-odd Higgs, we find that a light gluino is incompatible with a class of supergravity models defined by N=1 supergravity, with a radiatively broken electroweak symmetry group and universality of scalar and gaugino masses at the unification scale. We also find in this scenario strong constraints on the parameter space due to the new CLEO bounds on B(b\longrightarrow sγ). Presented in the International Workshop ``SUSY-94'', University of Michigan, Ann Arbor MI, May 14-17, 1994.

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