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Supersymmetry, Supergravity and $R_b$ revisited in the light of LEP 2

A previous study of supersymmetric models has indicated that they are unlikely to make a large contribution to R_b. We revisit this analysis, taking into account the improved lower limits on sparticle masses provided recently by LEP 2 and the Tevatron, finding that a generic supersymmetric model can...

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Detalles Bibliográficos
Autores principales: Ellis, John R., Lopez, Jorge L., Nanopoulos, Dimitri V.
Lenguaje:eng
Publicado: 1996
Materias:
Acceso en línea:https://dx.doi.org/10.1016/S0370-2693(97)00156-1
http://cds.cern.ch/record/317020
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author Ellis, John R.
Lopez, Jorge L.
Nanopoulos, Dimitri V.
author_facet Ellis, John R.
Lopez, Jorge L.
Nanopoulos, Dimitri V.
author_sort Ellis, John R.
collection CERN
description A previous study of supersymmetric models has indicated that they are unlikely to make a large contribution to R_b. We revisit this analysis, taking into account the improved lower limits on sparticle masses provided recently by LEP 2 and the Tevatron, finding that a generic supersymmetric model cannot contribute more than about one-and-a-half current experimental standard deviations to R_b. We then specialize this analysis to minimal supergravity models with universal high-energy boundary conditions, and find a much more stringent upper bound R^{susy}_b < 0.0003. We discuss in detail why such models can only attain values of R^{susy}_b that are considerably smaller even than those obtainable in more general supersymmetric models.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1996
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spelling cern-3170202023-03-15T19:10:52Zdoi:10.1016/S0370-2693(97)00156-1http://cds.cern.ch/record/317020engEllis, John R.Lopez, Jorge L.Nanopoulos, Dimitri V.Supersymmetry, Supergravity and $R_b$ revisited in the light of LEP 2Particle Physics - PhenomenologyA previous study of supersymmetric models has indicated that they are unlikely to make a large contribution to R_b. We revisit this analysis, taking into account the improved lower limits on sparticle masses provided recently by LEP 2 and the Tevatron, finding that a generic supersymmetric model cannot contribute more than about one-and-a-half current experimental standard deviations to R_b. We then specialize this analysis to minimal supergravity models with universal high-energy boundary conditions, and find a much more stringent upper bound R^{susy}_b < 0.0003. We discuss in detail why such models can only attain values of R^{susy}_b that are considerably smaller even than those obtainable in more general supersymmetric models.A previous study of supersymmetric models has indicated that they are unlikely to make a large contribution to R_b. We revisit this analysis, taking into account the improved lower limits on sparticle masses provided recently by LEP 2 and the Tevatron, finding that a generic supersymmetric model cannot contribute more than about one-and-a-half current experimental standard deviations to R_b. We then specialize this analysis to minimal supergravity models with universal high-energy boundary conditions, and find a much more stringent upper bound R~{susy}_b < 0.0003. We discuss in detail why such models can only attain values of R~{susy}_b that are considerably smaller even than those obtainable in more general supersymmetric models.A previous study of supersymmetric models has indicated that they are unlikely to make a large contribution to R b ≡ Γ(Z 0 → b b) Γ(Z 0 → hadrons ) . We revisit this analysis, taking into account the improved lower limits on sparticle masses provided recently by LEP 2 and the Tevatron, finding that a generic supersymmetric model cannot contribute more than about one-and-a-half current experimental standard deviations to R b . We then specialize this analysis to minimal supergravity models with universal high-energy boundary conditions, and find a much more stringent upper bound R b susy < 0.0003. We discuss in detail why such models can only attain values of R b susy that are considerably smaller than those obtainable in more general supersymmetric models.hep-ph/9612376CERN-TH-96-354DOE-ER-40717-37CTP-TAMU-64-96ACT-18-96ACT-1996-18CERN-TH-96-354CTP-TAMU-96-64DOE-ER-40717-37oai:cds.cern.ch:3170201996-12-16
spellingShingle Particle Physics - Phenomenology
Ellis, John R.
Lopez, Jorge L.
Nanopoulos, Dimitri V.
Supersymmetry, Supergravity and $R_b$ revisited in the light of LEP 2
title Supersymmetry, Supergravity and $R_b$ revisited in the light of LEP 2
title_full Supersymmetry, Supergravity and $R_b$ revisited in the light of LEP 2
title_fullStr Supersymmetry, Supergravity and $R_b$ revisited in the light of LEP 2
title_full_unstemmed Supersymmetry, Supergravity and $R_b$ revisited in the light of LEP 2
title_short Supersymmetry, Supergravity and $R_b$ revisited in the light of LEP 2
title_sort supersymmetry, supergravity and $r_b$ revisited in the light of lep 2
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1016/S0370-2693(97)00156-1
http://cds.cern.ch/record/317020
work_keys_str_mv AT ellisjohnr supersymmetrysupergravityandrbrevisitedinthelightoflep2
AT lopezjorgel supersymmetrysupergravityandrbrevisitedinthelightoflep2
AT nanopoulosdimitriv supersymmetrysupergravityandrbrevisitedinthelightoflep2