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- W2089338177 abstract "We explore the one-loop electroweak radiative corrections in the minimal SU(5) and the no-scale flipped SU(5) supergravity models via explicit calculation of vacuum polarization contributions to the ${ensuremath{epsilon}}_{1,2,3}$ parameters. Experimentally, ${ensuremath{epsilon}}_{1,2,3}$ are obtained from a global fit to the CERN LEP observables, and $frac{{M}_{W}}{{M}_{Z}}$ measurements. We include ${q}^{2}$-dependent effects which have been neglected in most previous model-independent analyses of this type. These effects induce a large systematic negative shift on ${ensuremath{epsilon}}_{1,2,3}$ for light chargino masses (${m}_{{ensuremath{chi}}_{1}^{ifmmodepmelsetextpmfi{}}}ensuremath{lesssim}70$ GeV). In agreement with previous general arguments we find that for increasingly large sparticle masses the heavy sector of both models rapidly decouples; i.e., the values for ${ensuremath{epsilon}}_{1,2,3}$ quickly become asymptotic to the standard model values with a light Higgs boson (${m}_{{H}_{mathrm{SM}}}ensuremath{sim}100$ GeV). Specifically, at present the 90% C.L. upper limit on the top-quark mass is ${m}_{t}ensuremath{lesssim}175$ GeV in the no-scale flipped SU(5) supergravity model. These bounds can be strengthened for increasing chargino masses in the 50-100 GeV interval. In particular, for ${m}_{t}ensuremath{gtrsim}160$ GeV, the Fermilab Tevatron may be able to probe through gluino ($stackrel{ifmmode tilde{}else ~{}fi{}}{g}$) and squark ($stackrel{ifmmode tilde{}else ~{}fi{}}{q}$) production up to ${m}_{stackrel{ifmmode tilde{}else ~{}fi{}}{g}}ensuremath{approx}{m}_{stackrel{ifmmode tilde{}else ~{}fi{}}{q}}ensuremath{approx}250$ GeV, exploring at least half of the parameter space in this model." @default.
- W2089338177 created "2016-06-24" @default.
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- W2089338177 date "1993-10-01" @default.
- W2089338177 modified "2023-09-23" @default.
- W2089338177 title "Precision electroweak tests of the minimal and flipped SU(5) supergravity models" @default.
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- W2089338177 doi "https://doi.org/10.1103/physrevd.48.3297" @default.
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