Supergravity Grand Unification, Proton Decay and Cosmological Constraints
Abstract
Properties and experimental predictions of a broad class of supergravity grand unified models possessing an SU(5)-type proton decay and R parity are described. Models of this type can be described in terms of four parameters at the Gut scale in addition to those of the Standard Model i.e. mo (universal scalar mass), m1/2 (universal gaugino mass), Ao (cubic soft breaking parameter) and β=<H2>/<H1>. Thus the 32 SUSY masses can be expressed in terms of mo, m1/2, Ao β and the as yet unknown t-quark mass mt. Gut thresholds are examined and a simple model leads to grand unification consistent with p-decay data when 0.114<α3 (Mz)<0.135, in agreement with current values of α3 (MZ).Proton decay is examined for the superheavy Higgs triplet mass MH3<10MG(MG 1.5 ×1016~GeV) and squarks and gluinos lighter than 1 TeV. Throughout most of the parameter space chargino-neutralino scaling relations are predicted to hold: 2mZ1 mW1 mZ2, mW1(1/4)mg (for μ>0) or mW1 (1/3)mg (for μ<0), while mW2 mZ3 mZ4>>mZ1. Future proton decay experiments combined with LEP2 lead to further predictions, e.g. for the entire parameter space either proton decay should be seen at these or theW1 seen at LEP2. Relic density constraints on the Z1 further constrain the parameter space e.g. so that mt<165~GeV, mh<105~GeV, mW1 <100~GeV and mZ1<50~GeV when MH3/MG < 6. (Invited talk at Les Rencontres de Physique de la Vallee D'Aoste
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