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The strongest experimental constraints on SU(5) x U(1) supergravity models
We consider a class of well motivated string-inspired flipped $SU(5)$ supergravity models which include four supersymmetry breaking scenarios: no-scale, strict no-scale, dilaton, and special dilaton, such that only three parameters are needed to describe all new phenomena $(m_t,\tan\beta,m_{\tilde g...
Autores principales: | , , , |
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Lenguaje: | eng |
Publicado: |
1994
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Acceso en línea: | https://dx.doi.org/10.1103/PhysRevD.49.355 http://cds.cern.ch/record/252811 |
_version_ | 1780885640275034112 |
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author | Lopez, Jorge L. Nanopoulos, Dimitri V. Park, Gye T. Zichichi, A. |
author_facet | Lopez, Jorge L. Nanopoulos, Dimitri V. Park, Gye T. Zichichi, A. |
author_sort | Lopez, Jorge L. |
collection | CERN |
description | We consider a class of well motivated string-inspired flipped $SU(5)$ supergravity models which include four supersymmetry breaking scenarios: no-scale, strict no-scale, dilaton, and special dilaton, such that only three parameters are needed to describe all new phenomena $(m_t,\tan\beta,m_{\tilde g})$. We show that the LEP precise measurements of the electroweak parameters in the form of the $\epsilon_1$ variable, and the CLEOII allowed range for $\bsg$ are at present the most important experimental constraints on this class of models. For $m_t\gsim155\,(165)\GeV$, the $\epsilon_1$ constraint (at 90(95)\%CL) requires the presence of light charginos ($m_{\chi~\pm_1}\lsim50-100\GeV$ depending on $m_t$). Since all sparticle masses are proportional to $m_{\tilde g}$, $m_{\chi~\pm_1}\lsim100\GeV$ implies: $m_{\chi~0_1}\lsim55\GeV$, $m_{\chi~0_2}\lsim100\GeV$, $m_{\tilde g}\lsim360\GeV$, $m_{\tilde q}\lsim350\,(365)\GeV$, $m_{\tilde e_R}\lsim80\,(125)\GeV$, $m_{\tilde e_L}\lsim120\,(155)\GeV$, and $m_{\tilde\nu}\lsim100\,(140)\GeV$ in the no-scale (dilaton) flipped $SU(5)$ supergravity model. The $\bsg$ constraint excludes a significant fraction of the otherwise allowed region in the $(m_{\chi~\pm_1},\tan\beta)$ plane (irrespective of the magnitude of the chargino mass), while future experimental improvements will result in decisive tests of these models. In light of the $\epsilon_1$ constraint, we conclude that the outlook for chargino and selectron detection at LEPII and at HERA is quite favorable in this class of models. |
id | cern-252811 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 1994 |
record_format | invenio |
spelling | cern-2528112020-07-23T02:47:47Zdoi:10.1103/PhysRevD.49.355http://cds.cern.ch/record/252811engLopez, Jorge L.Nanopoulos, Dimitri V.Park, Gye T.Zichichi, A.The strongest experimental constraints on SU(5) x U(1) supergravity modelsParticle Physics - PhenomenologyWe consider a class of well motivated string-inspired flipped $SU(5)$ supergravity models which include four supersymmetry breaking scenarios: no-scale, strict no-scale, dilaton, and special dilaton, such that only three parameters are needed to describe all new phenomena $(m_t,\tan\beta,m_{\tilde g})$. We show that the LEP precise measurements of the electroweak parameters in the form of the $\epsilon_1$ variable, and the CLEOII allowed range for $\bsg$ are at present the most important experimental constraints on this class of models. For $m_t\gsim155\,(165)\GeV$, the $\epsilon_1$ constraint (at 90(95)\%CL) requires the presence of light charginos ($m_{\chi~\pm_1}\lsim50-100\GeV$ depending on $m_t$). Since all sparticle masses are proportional to $m_{\tilde g}$, $m_{\chi~\pm_1}\lsim100\GeV$ implies: $m_{\chi~0_1}\lsim55\GeV$, $m_{\chi~0_2}\lsim100\GeV$, $m_{\tilde g}\lsim360\GeV$, $m_{\tilde q}\lsim350\,(365)\GeV$, $m_{\tilde e_R}\lsim80\,(125)\GeV$, $m_{\tilde e_L}\lsim120\,(155)\GeV$, and $m_{\tilde\nu}\lsim100\,(140)\GeV$ in the no-scale (dilaton) flipped $SU(5)$ supergravity model. The $\bsg$ constraint excludes a significant fraction of the otherwise allowed region in the $(m_{\chi~\pm_1},\tan\beta)$ plane (irrespective of the magnitude of the chargino mass), while future experimental improvements will result in decisive tests of these models. In light of the $\epsilon_1$ constraint, we conclude that the outlook for chargino and selectron detection at LEPII and at HERA is quite favorable in this class of models.hep-ph/9308266CTP-TAMU-40-93ACT-15-93CERN-TH-6979-93ACT-1993-15CERN-TH-6979-93CTP-TAMU-93-40oai:cds.cern.ch:2528111994 |
spellingShingle | Particle Physics - Phenomenology Lopez, Jorge L. Nanopoulos, Dimitri V. Park, Gye T. Zichichi, A. The strongest experimental constraints on SU(5) x U(1) supergravity models |
title | The strongest experimental constraints on SU(5) x U(1) supergravity models |
title_full | The strongest experimental constraints on SU(5) x U(1) supergravity models |
title_fullStr | The strongest experimental constraints on SU(5) x U(1) supergravity models |
title_full_unstemmed | The strongest experimental constraints on SU(5) x U(1) supergravity models |
title_short | The strongest experimental constraints on SU(5) x U(1) supergravity models |
title_sort | strongest experimental constraints on su(5) x u(1) supergravity models |
topic | Particle Physics - Phenomenology |
url | https://dx.doi.org/10.1103/PhysRevD.49.355 http://cds.cern.ch/record/252811 |
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