Mass production of type IIA dS vacua

Abstract A three-step procedure is proposed in type IIA string theory to stabilize multiple moduli in a dS vacuum. The first step is to construct a progenitor model with a localized stable supersymmetric Minkowski vacuum, or a discrete set of such vacua. It can be done, for example, using two non-pe...

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Main Authors: Renata Kallosh, Andrei Linde
Format: Article
Language:English
Published: SpringerOpen 2020-01-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP01(2020)169
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author Renata Kallosh
Andrei Linde
author_facet Renata Kallosh
Andrei Linde
author_sort Renata Kallosh
collection DOAJ
description Abstract A three-step procedure is proposed in type IIA string theory to stabilize multiple moduli in a dS vacuum. The first step is to construct a progenitor model with a localized stable supersymmetric Minkowski vacuum, or a discrete set of such vacua. It can be done, for example, using two non-perturbative exponents in the superpotential for each modulus, as in the KL model [1]. A large set of supersymmetric Minkowski vacua with strongly stabilized moduli is protected by a theorem on stability of these vacua in absence of flat directions [2]. The second step involves a parametrically small downshift to a supersymmetric AdS vacuum, which can be achieved by a small change of the superpotential. The third step is an uplift to a dS vacuum with a positive cosmological constant using the D 6 ¯ $$ \overline{D6} $$ -brane contribution [3, 4]. Stability of the resulting dS vacuum is inherited from the stability of the original supersymmetric Minkowski vacuum if the supersymmetry breaking in dS vacuum is parametrically small [2, 5].
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spelling doaj-art-36266a1732cb4cf3842cf24d29b7b92f2025-02-09T12:06:13ZengSpringerOpenJournal of High Energy Physics1029-84792020-01-012020112910.1007/JHEP01(2020)169Mass production of type IIA dS vacuaRenata Kallosh0Andrei Linde1Stanford Institute for Theoretical Physics and Department of Physics, Stanford UniversityStanford Institute for Theoretical Physics and Department of Physics, Stanford UniversityAbstract A three-step procedure is proposed in type IIA string theory to stabilize multiple moduli in a dS vacuum. The first step is to construct a progenitor model with a localized stable supersymmetric Minkowski vacuum, or a discrete set of such vacua. It can be done, for example, using two non-perturbative exponents in the superpotential for each modulus, as in the KL model [1]. A large set of supersymmetric Minkowski vacua with strongly stabilized moduli is protected by a theorem on stability of these vacua in absence of flat directions [2]. The second step involves a parametrically small downshift to a supersymmetric AdS vacuum, which can be achieved by a small change of the superpotential. The third step is an uplift to a dS vacuum with a positive cosmological constant using the D 6 ¯ $$ \overline{D6} $$ -brane contribution [3, 4]. Stability of the resulting dS vacuum is inherited from the stability of the original supersymmetric Minkowski vacuum if the supersymmetry breaking in dS vacuum is parametrically small [2, 5].https://doi.org/10.1007/JHEP01(2020)169Supergravity ModelsSuperstring VacuaD-branes
spellingShingle Renata Kallosh
Andrei Linde
Mass production of type IIA dS vacua
Journal of High Energy Physics
Supergravity Models
Superstring Vacua
D-branes
title Mass production of type IIA dS vacua
title_full Mass production of type IIA dS vacua
title_fullStr Mass production of type IIA dS vacua
title_full_unstemmed Mass production of type IIA dS vacua
title_short Mass production of type IIA dS vacua
title_sort mass production of type iia ds vacua
topic Supergravity Models
Superstring Vacua
D-branes
url https://doi.org/10.1007/JHEP01(2020)169
work_keys_str_mv AT renatakallosh massproductionoftypeiiadsvacua
AT andreilinde massproductionoftypeiiadsvacua