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A natural solution to the $\mu$ problem
We propose a simple mechanism for solving the $\mu$ problem in the context of minimal low--energy supergravity models. This is based on the appearance of non--renormalizable couplings in the superpotential. In particular, if $H_1H_2$ is an allowed operator by all the symmetries of the theory, it is...
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Lenguaje: | eng |
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1993
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Acceso en línea: | https://dx.doi.org/10.1016/0370-2693(93)90081-R http://cds.cern.ch/record/245793 |
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author | Casas, J.A. Munoz, C. |
author_facet | Casas, J.A. Munoz, C. |
author_sort | Casas, J.A. |
collection | CERN |
description | We propose a simple mechanism for solving the $\mu$ problem in the context of minimal low--energy supergravity models. This is based on the appearance of non--renormalizable couplings in the superpotential. In particular, if $H_1H_2$ is an allowed operator by all the symmetries of the theory, it is natural to promote the usual renormalizable superpotential $W_o$ to $W_o+\lambda W_o H_1H_2$, yielding an effective $\mu$ parameter whose size is directly related to the gravitino mass once supersymmetry is broken (this result is maintained if $H_1H_2$ couples with different strengths to the various terms present in $W_o$). On the other hand, the $\mu$ term must be absent from $W_o$, otherwise the natural scale for $\mu$ would be $M_P$. Remarkably enough, this is entirely justified in the supergravity theories coming from superstrings, where mass terms for light fields are forbidden in the superpotential. We also analyse the $SU(2)\times U(1)$ breaking, finding that it takes place satisfactorily. Finally, we give a realistic example in which supersymmetry is broken by gaugino condensation, where the mechanism proposed for solving the $\mu$ problem can be gracefully implemented. |
id | cern-245793 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 1993 |
record_format | invenio |
spelling | cern-2457932023-03-14T18:53:09Zdoi:10.1016/0370-2693(93)90081-Rhttp://cds.cern.ch/record/245793engCasas, J.A.Munoz, C.A natural solution to the $\mu$ problemGeneral Theoretical PhysicsParticle Physics - PhenomenologyWe propose a simple mechanism for solving the $\mu$ problem in the context of minimal low--energy supergravity models. This is based on the appearance of non--renormalizable couplings in the superpotential. In particular, if $H_1H_2$ is an allowed operator by all the symmetries of the theory, it is natural to promote the usual renormalizable superpotential $W_o$ to $W_o+\lambda W_o H_1H_2$, yielding an effective $\mu$ parameter whose size is directly related to the gravitino mass once supersymmetry is broken (this result is maintained if $H_1H_2$ couples with different strengths to the various terms present in $W_o$). On the other hand, the $\mu$ term must be absent from $W_o$, otherwise the natural scale for $\mu$ would be $M_P$. Remarkably enough, this is entirely justified in the supergravity theories coming from superstrings, where mass terms for light fields are forbidden in the superpotential. We also analyse the $SU(2)\times U(1)$ breaking, finding that it takes place satisfactorily. Finally, we give a realistic example in which supersymmetry is broken by gaugino condensation, where the mechanism proposed for solving the $\mu$ problem can be gracefully implemented.We propose a simple mechanism for solving the μ-problem in the context of minimal low-energy supergravity models. This is based on the appearance of non-renormalizable couplings in the superpotential. In particular, if H 1 H 2 is an allowed operator by all the symmetries of the theory, it is natural to promote the usual renormalizable superpotential W 0 to W 0 + λW 0 H 1 H 2 , yielding an effective μ parameter whose size is directly related to the gravitino mass once supersymmetry is broken (this result is maintained if H 1 H 2 couples with different strengths to the various terms present in W 0 ). On the other hand, the μ-term must be absent in W 0 , otherwise the natural scale for μ would be M > Pl . Remarkably enough, this is entirely justified in the SUGRA theories coming from superstrings, where mass terms for light fields are forbidden in the superpotential. We also analyze the SU(2)×U(1) breaking, finding that it takes place satisfactorily. Finally, we give a realistic example in which SUSY is broken by gaugino condensation where the mechanism proposed for solving the μ-problem can be gracefully implemented.We propose a simple mechanism for solving the $\mu$ problem in the context of minimal low--energy supergravity models. This is based on the appearance of non--renormalizable couplings in the superpotential. In particular, if $H_1H_2$ is an allowed operator by all the symmetries of the theory, it is natural to promote the usual renormalizable superpotential $W_o$ to $W_o+\lambda W_o H_1H_2$, yielding an effective $\mu$ parameter whose size is directly related to the gravitino mass once supersymmetry is broken (this result is maintained if $H_1H_2$ couples with different strengths to the various terms present in $W_o$). On the other hand, the $\mu$ term must be absent from $W_o$, otherwise the natural scale for $\mu$ would be $M_P$. Remarkably enough, this is entirely justified in the supergravity theories coming from superstrings, where mass terms for light fields are forbidden in the superpotential. We also analyse the $SU(2)\times U(1)$ breaking, finding that it takes place satisfactorily. Finally, we give a realistic example in which supersymmetry is broken by gaugino condensation, where the mechanism proposed for solving the $\mu$ problem can be gracefully implemented.hep-ph/9302227FTUAM-92-45CERN-TH-6764-92IEM-FT-66-92CERN-TH-6764-92FTUAM-92-45IEM-FT-66oai:cds.cern.ch:2457931993 |
spellingShingle | General Theoretical Physics Particle Physics - Phenomenology Casas, J.A. Munoz, C. A natural solution to the $\mu$ problem |
title | A natural solution to the $\mu$ problem |
title_full | A natural solution to the $\mu$ problem |
title_fullStr | A natural solution to the $\mu$ problem |
title_full_unstemmed | A natural solution to the $\mu$ problem |
title_short | A natural solution to the $\mu$ problem |
title_sort | natural solution to the $\mu$ problem |
topic | General Theoretical Physics Particle Physics - Phenomenology |
url | https://dx.doi.org/10.1016/0370-2693(93)90081-R http://cds.cern.ch/record/245793 |
work_keys_str_mv | AT casasja anaturalsolutiontothemuproblem AT munozc anaturalsolutiontothemuproblem AT casasja naturalsolutiontothemuproblem AT munozc naturalsolutiontothemuproblem |