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No-Scale SU(5) Super-GUTs
We reconsider the minimal SU(5) grand unified theory (GUT) in the context of no-scale supergravity inspired by string compactification scenarios, assuming that the soft supersymmetry-breaking parameters satisfy universality conditions at some input scale $M_\mathrm{in}$ above the GUT scale $M_{\math...
Autores principales: | , , , , |
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Lenguaje: | eng |
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2017
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1140/epjc/s10052-017-4805-x http://cds.cern.ch/record/2244880 |
_version_ | 1780953449479798784 |
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author | Ellis, John Evans, Jason L. Nagata, Natsumi Nanopoulos, Dimitri V. Olive, Keith A. |
author_facet | Ellis, John Evans, Jason L. Nagata, Natsumi Nanopoulos, Dimitri V. Olive, Keith A. |
author_sort | Ellis, John |
collection | CERN |
description | We reconsider the minimal SU(5) grand unified theory (GUT) in the context of no-scale supergravity inspired by string compactification scenarios, assuming that the soft supersymmetry-breaking parameters satisfy universality conditions at some input scale $M_\mathrm{in}$ above the GUT scale $M_{\mathrm{GUT}}$ . When setting up such a no-scale super-GUT model, special attention must be paid to avoiding the Scylla of rapid proton decay and the Charybdis of an excessive density of cold dark matter, while also having an acceptable mass for the Higgs boson. We do not find consistent solutions if none of the matter and Higgs fields are assigned to twisted chiral supermultiplets, even in the presence of Giudice–Masiero terms. However, consistent solutions may be found if at least one fiveplet of GUT Higgs fields is assigned to a twisted chiral supermultiplet, with a suitable choice of modular weights. Spin-independent dark matter scattering may be detectable in some of these consistent solutions. |
id | cern-2244880 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2017 |
record_format | invenio |
spelling | cern-22448802023-09-12T03:29:36Zdoi:10.1140/epjc/s10052-017-4805-xhttp://cds.cern.ch/record/2244880engEllis, JohnEvans, Jason L.Nagata, NatsumiNanopoulos, Dimitri V.Olive, Keith A.No-Scale SU(5) Super-GUTsastro-ph.COAstrophysics and Astronomyhep-phParticle Physics - PhenomenologyWe reconsider the minimal SU(5) grand unified theory (GUT) in the context of no-scale supergravity inspired by string compactification scenarios, assuming that the soft supersymmetry-breaking parameters satisfy universality conditions at some input scale $M_\mathrm{in}$ above the GUT scale $M_{\mathrm{GUT}}$ . When setting up such a no-scale super-GUT model, special attention must be paid to avoiding the Scylla of rapid proton decay and the Charybdis of an excessive density of cold dark matter, while also having an acceptable mass for the Higgs boson. We do not find consistent solutions if none of the matter and Higgs fields are assigned to twisted chiral supermultiplets, even in the presence of Giudice–Masiero terms. However, consistent solutions may be found if at least one fiveplet of GUT Higgs fields is assigned to a twisted chiral supermultiplet, with a suitable choice of modular weights. Spin-independent dark matter scattering may be detectable in some of these consistent solutions.We reconsider the minimal SU(5) Grand Unified Theory (GUT) in the context of no-scale supergravity, assuming that the soft supersymmetry-breaking parameters satisfy universality conditions at some input scale M_in above the GUT scale M_GUT. When setting up such a no-scale super-GUT model, special attention must be paid to avoiding the Scylla of rapid proton decay and the Charybdis of an excessive density of cold dark matter, while also having an acceptable mass for the Higgs boson. We do not find consistent solutions if none of the matter and Higgs fields are assigned to twisted chiral supermultiplets, even in the presence of Giudice-Masiero terms. However, consistent solutions may be found if at least one fiveplet of GUT Higgs fields is assigned to a twisted chiral supermultiplet, with a suitable choice of modular weights. Spin-independent dark matter scattering may be detectable in some of these consistent solutions.arXiv:1702.00379KCL-PH-TH-2017-05CERN-TH-2017-010KIAS-P17008UT-17-03MI-TH-1738UMN-TH-3618-17FTPI-MINN-17-02ACT-01-17oai:cds.cern.ch:22448802017-02-01 |
spellingShingle | astro-ph.CO Astrophysics and Astronomy hep-ph Particle Physics - Phenomenology Ellis, John Evans, Jason L. Nagata, Natsumi Nanopoulos, Dimitri V. Olive, Keith A. No-Scale SU(5) Super-GUTs |
title | No-Scale SU(5) Super-GUTs |
title_full | No-Scale SU(5) Super-GUTs |
title_fullStr | No-Scale SU(5) Super-GUTs |
title_full_unstemmed | No-Scale SU(5) Super-GUTs |
title_short | No-Scale SU(5) Super-GUTs |
title_sort | no-scale su(5) super-guts |
topic | astro-ph.CO Astrophysics and Astronomy hep-ph Particle Physics - Phenomenology |
url | https://dx.doi.org/10.1140/epjc/s10052-017-4805-x http://cds.cern.ch/record/2244880 |
work_keys_str_mv | AT ellisjohn noscalesu5superguts AT evansjasonl noscalesu5superguts AT nagatanatsumi noscalesu5superguts AT nanopoulosdimitriv noscalesu5superguts AT olivekeitha noscalesu5superguts |