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A string no-scale supergravity model and its experimental consequences
We propose a string-derived model based on the gauge group SU(5)\times U(1) which satisfies the stringent constraints from no-scale supergravity, allows gauge coupling unification at the string scale, and entails previously unexplored correlations among various sectors of the model. All supersymmetr...
Autores principales: | , , |
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Lenguaje: | eng |
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1995
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Acceso en línea: | https://dx.doi.org/10.1103/PhysRevD.52.4178 http://cds.cern.ch/record/277693 |
_version_ | 1780887666992087040 |
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author | Lopez, Jorge L. Nanopoulos, Dimitri V. Zichichi, A. |
author_facet | Lopez, Jorge L. Nanopoulos, Dimitri V. Zichichi, A. |
author_sort | Lopez, Jorge L. |
collection | CERN |
description | We propose a string-derived model based on the gauge group SU(5)\times U(1) which satisfies the stringent constraints from no-scale supergravity, allows gauge coupling unification at the string scale, and entails previously unexplored correlations among various sectors of the model. All supersymmetric observables are given in terms of a single mass parameter with self-consistency of the model determining the rest, including \tan\beta=2.2-2.3 and m_t\approx175\GeV. A small non-universality of the scalar masses at the string scale produces a downward shift in the right-handed slepton masses at the electroweak scale, such that for m_{1/2}\gsim180\GeV these particles become lighter than the lightest neutralino. This cutoff in the parameter space entails the imminent discovery of charginos at the Tevatron via trilepton events (m_{\chi^\pm_1}<90\GeV). Also, the lightest Higgs boson (m_h<90\GeV), the lightest chargino, and the right-handed sleptons (m_{\tilde\ell_R}<50\GeV) should be readily observable at LEPII. We also discuss the model predictions for B(b\to s\gamma) (g-2)_\mu, R_b, and the prospects for direct neutralino dark matter detection. |
id | cern-277693 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 1995 |
record_format | invenio |
spelling | cern-2776932023-03-14T20:43:47Zdoi:10.1103/PhysRevD.52.4178http://cds.cern.ch/record/277693engLopez, Jorge L.Nanopoulos, Dimitri V.Zichichi, A.A string no-scale supergravity model and its experimental consequencesParticle Physics - PhenomenologyWe propose a string-derived model based on the gauge group SU(5)\times U(1) which satisfies the stringent constraints from no-scale supergravity, allows gauge coupling unification at the string scale, and entails previously unexplored correlations among various sectors of the model. All supersymmetric observables are given in terms of a single mass parameter with self-consistency of the model determining the rest, including \tan\beta=2.2-2.3 and m_t\approx175\GeV. A small non-universality of the scalar masses at the string scale produces a downward shift in the right-handed slepton masses at the electroweak scale, such that for m_{1/2}\gsim180\GeV these particles become lighter than the lightest neutralino. This cutoff in the parameter space entails the imminent discovery of charginos at the Tevatron via trilepton events (m_{\chi^\pm_1}<90\GeV). Also, the lightest Higgs boson (m_h<90\GeV), the lightest chargino, and the right-handed sleptons (m_{\tilde\ell_R}<50\GeV) should be readily observable at LEPII. We also discuss the model predictions for B(b\to s\gamma) (g-2)_\mu, R_b, and the prospects for direct neutralino dark matter detection.We propose a string-derived model based on the gauge group $SU(5)\times U(1)$ which satisfies the stringent constraints from no-scale supergravity, allows gauge coupling unification at the string scale, and entails previously unexplored correlations among various sectors of the model. All supersymmetric observables are given in terms of a single mass parameter with self-consistency of the model determining the rest, including $\tan\beta=2.2-2.3$ and $m_t\approx175\GeV$. A small non-universality of the scalar masses at the string scale produces a downward shift in the right-handed slepton masses at the electroweak scale, such that for $m_{1/2}\gsim180\GeV$ these particles become lighter than the lightest neutralino. This cutoff in the parameter space entails the imminent discovery of charginos at the Tevatron via trilepton events ($m_{\chi~\pm_1}<90\GeV$). Also, the lightest Higgs boson ($m_h<90\GeV$), the lightest chargino, and the right-handed sleptons ($m_{\tilde\ell_R}<50\GeV$) should be readily observable at LEPII. We also discuss the model predictions for $B(b\to s\gamma)$, $(g-2)_\mu$, $R_b$, and the prospects for direct neutralino dark matter detection.We propose a string-derived model based on the gauge group $SU(5)\times U(1)$ which satisfies the stringent constraints from no-scale supergravity, allows gauge coupling unification at the string scale, and entails previously unexplored correlations among various sectors of the model. All supersymmetric observables are given in terms of a single mass parameter with self-consistency of the model determining the rest, including $\tan\beta=2.2-2.3$ and $m_t\approx175\GeV$. A small non-universality of the scalar masses at the string scale produces a downward shift in the right-handed slepton masses at the electroweak scale, such that for $m_{1/2}\gsim180\GeV$ these particles become lighter than the lightest neutralino. This cutoff in the parameter space entails the imminent discovery of charginos at the Tevatron via trilepton events ($m_{\chi^\pm_1}<90\GeV$). Also, the lightest Higgs boson ($m_h<90\GeV$), the lightest chargino, and the right-handed sleptons ($m_{\tilde\ell_R}<50\GeV$) should be readily observable at LEPII. We also discuss the model predictions for $B(b\to s\gamma)$, $(g-2)_\mu$, $R_b$, and the prospects for direct neutralino dark matter detection.hep-ph/9502414CTP-TAMU-06-95ACT-02-95CTP-TAMU-95-6oai:cds.cern.ch:2776931995-02-28 |
spellingShingle | Particle Physics - Phenomenology Lopez, Jorge L. Nanopoulos, Dimitri V. Zichichi, A. A string no-scale supergravity model and its experimental consequences |
title | A string no-scale supergravity model and its experimental consequences |
title_full | A string no-scale supergravity model and its experimental consequences |
title_fullStr | A string no-scale supergravity model and its experimental consequences |
title_full_unstemmed | A string no-scale supergravity model and its experimental consequences |
title_short | A string no-scale supergravity model and its experimental consequences |
title_sort | string no-scale supergravity model and its experimental consequences |
topic | Particle Physics - Phenomenology |
url | https://dx.doi.org/10.1103/PhysRevD.52.4178 http://cds.cern.ch/record/277693 |
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