New Precision Electroweak Tests of SU(5) x U(1) Supergravity
arXiv:hep-ph/9311277 · doi:10.1103/PhysRevD.49.4835
Abstract
We explore the one-loop electroweak radiative corrections in supergravity via explicit calculation of vacuum-polarization and vertex-correction contributions to the and parameters. Experimentally, these parameters are obtained from a global fit to the set of observables , and . We include -dependent effects, which induce a large systematic negative shift on for light chargino masses ($m_{χ^\pm_1}\lsim70\GeV$). The (non-oblique) supersymmetric vertex corrections to $\Zbb$, which define the parameter, show a significant positive shift for light chargino masses, which for can be nearly compensated by a negative shift from the charged Higgs contribution. We conclude that at the 90\%CL, for $m_t\lsim160\GeV$ the present experimental values of and do not constrain in any way supergravity in both no-scale and dilaton scenarios. On the other hand, for $m_t\gsim160\GeV$ the constraints on the parameter space become increasingly stricter. We demonstrate this trend with a study of the $m_t=170\GeV$ case, where only a small region of parameter space, with $\tanβ\gsim4$, remains allowed and corresponds to light chargino masses ($m_{χ^\pm_1}\lsim70\GeV$). Thus supergravity combined with high-precision LEP data would suggest the presence of light charginos if the top quark is not detected at the Tevatron.
LaTeX, 11 Pages+4 Figures(not included), the figures available upon request as an uuencoded file(0.4MB) or 4 PS files from [email protected], CERN-TH.7078/93, CTP-TAMU-68/93, ACT-24/93
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- Constraints on the Minimal and Supergravity Models
- Precision Electroweak Tests on the Model
- Probing Supergravity Models with Indirect Experimental Signatures
- New Precision Electroweak Tests in Supergravity Models