1990
DOI: 10.1103/physrevd.42.1709
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Supersymmetric contribution to the electroweakρparameter

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Cited by 121 publications
(127 citation statements)
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“…Of course, squark contributions are not the only supersymmetric corrections to ∆ρ. However, they are the only potentially large ones, when the present direct exclusion bounds are taken into account, and the other contributions have in general the same sign [78]. As the relative experimental accuracy for these quantities is 5×10 −4 and 7 × 10 −4 , respectively, it is easy to realize that the present sensitivity to ∆ρ is at the level of 1×10 −3 .…”
Section: Constraints From Electroweak Precision Testsmentioning
confidence: 80%
See 1 more Smart Citation
“…Of course, squark contributions are not the only supersymmetric corrections to ∆ρ. However, they are the only potentially large ones, when the present direct exclusion bounds are taken into account, and the other contributions have in general the same sign [78]. As the relative experimental accuracy for these quantities is 5×10 −4 and 7 × 10 −4 , respectively, it is easy to realize that the present sensitivity to ∆ρ is at the level of 1×10 −3 .…”
Section: Constraints From Electroweak Precision Testsmentioning
confidence: 80%
“…This universal contribution enters the Z 0 boson couplings and the relation between M W , G µ and α and is therefore significantly constrained by present data. Following the assumptions of section 2, the contribution of the squarks to ∆ρ = 1 − 1/ρ is given at one-loop order by the simple expression [77,78] 20) with the function F given by…”
Section: Constraints From Electroweak Precision Testsmentioning
confidence: 99%
“…• R-Higgs sector: the contributions from the R-Higgs sector have a structure similar to the stop-sbottom contribution [74],…”
Section: To Fulfill the Tree-level Tadpole Equations Is Given Asmentioning
confidence: 99%
“…With such an operator one can achieve a first-order electroweak phase transition [30] that may be relevant for the problem of baryogenesis. It was shown that one needs f √ c 6 > 550 GeV (35) to ensure that the expansion of the universe does not disallow percolation of bubbles of metastable vacuum. This corresponds to c 6 ξ < 0.2.…”
Section: Higher-dimensional Operators and Composite Modelsmentioning
confidence: 99%