A new class of de Sitter vacua in type IIB large volume compactifications

Abstract We construct a new class of metastable de Sitter vacua of flux compactifications of type IIB string theory. These solutions provide a natural extension of the ‘Large Volume Scenario’ anti-de Sitter vacua, and can analogously be realised at parametrically large volume and weak string couplin...

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Main Authors: Diego Gallego, M. C. David Marsh, Bert Vercnocke, Timm Wrase
Format: Article
Language:English
Published: SpringerOpen 2017-10-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP10(2017)193
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author Diego Gallego
M. C. David Marsh
Bert Vercnocke
Timm Wrase
author_facet Diego Gallego
M. C. David Marsh
Bert Vercnocke
Timm Wrase
author_sort Diego Gallego
collection DOAJ
description Abstract We construct a new class of metastable de Sitter vacua of flux compactifications of type IIB string theory. These solutions provide a natural extension of the ‘Large Volume Scenario’ anti-de Sitter vacua, and can analogously be realised at parametrically large volume and weak string coupling, using standard N $$ \mathcal{N} $$ = 1 supergravity. For these new vacua, a positive vacuum energy is achieved from the inclusion of a small amount of flux-induced supersymmetry breaking in the complex structure and axio-dilaton sector, and no additional ‘uplift’ contribution (e.g. from anti-branes) is required. We show that the approximate no-scale structure of the effective theory strongly influences the spectrum of the stabilised moduli: one complex structure modulus remains significantly lighter than the supersymmetry breaking scale, and metastability requires only modest amounts of tuning. After discussing these general results, we provide a recipe for constructing de Sitter vacua on a given compactification manifold, and give an explicit example of a de Sitter vacuum for the compactification on the Calabi-Yau orientifold realised in ℂ ℙ 11169 4 $$ \mathbb{C}{\mathrm{\mathbb{P}}}_{11169}^4 $$ . Finally, we note that these solutions have intriguing implications for phenomenology, predicting no csuperpartners in the spectrum below ∼50 TeV, and no WIMP dark matter.
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spelling doaj.art-869b5d7310ba4cd69124ba520a747aa12022-12-22T00:04:04ZengSpringerOpenJournal of High Energy Physics1029-84792017-10-0120171013410.1007/JHEP10(2017)193A new class of de Sitter vacua in type IIB large volume compactificationsDiego Gallego0M. C. David Marsh1Bert Vercnocke2Timm Wrase3Escuela de Física, Universidad Pedagógica y Tecnológica de Colombia (UPTC)Department of Applied Mathematics and Theoretical Physics, University of CambridgeInstitute for Theoretical Physics, KU LeuvenInstitute for Theoretical Physics, TU WienAbstract We construct a new class of metastable de Sitter vacua of flux compactifications of type IIB string theory. These solutions provide a natural extension of the ‘Large Volume Scenario’ anti-de Sitter vacua, and can analogously be realised at parametrically large volume and weak string coupling, using standard N $$ \mathcal{N} $$ = 1 supergravity. For these new vacua, a positive vacuum energy is achieved from the inclusion of a small amount of flux-induced supersymmetry breaking in the complex structure and axio-dilaton sector, and no additional ‘uplift’ contribution (e.g. from anti-branes) is required. We show that the approximate no-scale structure of the effective theory strongly influences the spectrum of the stabilised moduli: one complex structure modulus remains significantly lighter than the supersymmetry breaking scale, and metastability requires only modest amounts of tuning. After discussing these general results, we provide a recipe for constructing de Sitter vacua on a given compactification manifold, and give an explicit example of a de Sitter vacuum for the compactification on the Calabi-Yau orientifold realised in ℂ ℙ 11169 4 $$ \mathbb{C}{\mathrm{\mathbb{P}}}_{11169}^4 $$ . Finally, we note that these solutions have intriguing implications for phenomenology, predicting no csuperpartners in the spectrum below ∼50 TeV, and no WIMP dark matter.http://link.springer.com/article/10.1007/JHEP10(2017)193Flux compactificationsSupergravity ModelsSuperstring Vacua
spellingShingle Diego Gallego
M. C. David Marsh
Bert Vercnocke
Timm Wrase
A new class of de Sitter vacua in type IIB large volume compactifications
Journal of High Energy Physics
Flux compactifications
Supergravity Models
Superstring Vacua
title A new class of de Sitter vacua in type IIB large volume compactifications
title_full A new class of de Sitter vacua in type IIB large volume compactifications
title_fullStr A new class of de Sitter vacua in type IIB large volume compactifications
title_full_unstemmed A new class of de Sitter vacua in type IIB large volume compactifications
title_short A new class of de Sitter vacua in type IIB large volume compactifications
title_sort new class of de sitter vacua in type iib large volume compactifications
topic Flux compactifications
Supergravity Models
Superstring Vacua
url http://link.springer.com/article/10.1007/JHEP10(2017)193
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