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Domain walls, near-BPS bubbles, and probabilities in the landscape

We develop a theory of static BPS domain walls in stringy landscape and present a large family of BPS walls interpolating between different supersymmetric vacua. Examples include KKLT models, STU models, type IIB multiple flux vacua, and models with several Minkowski and AdS vacua. After the uplifti...

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Detalles Bibliográficos
Autores principales: Ceresole, Anna, Dall'Agata, Gianguido, Giryavets, Alexander, Kallosh, Renata, Linde, Andrei D.
Lenguaje:eng
Publicado: 2006
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.74.086010
http://cds.cern.ch/record/954656
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author Ceresole, Anna
Dall'Agata, Gianguido
Giryavets, Alexander
Kallosh, Renata
Linde, Andrei D.
author_facet Ceresole, Anna
Dall'Agata, Gianguido
Giryavets, Alexander
Kallosh, Renata
Linde, Andrei D.
author_sort Ceresole, Anna
collection CERN
description We develop a theory of static BPS domain walls in stringy landscape and present a large family of BPS walls interpolating between different supersymmetric vacua. Examples include KKLT models, STU models, type IIB multiple flux vacua, and models with several Minkowski and AdS vacua. After the uplifting, some of the vacua become dS, whereas some others remain AdS. The near-BPS walls separating these vacua may be seen as bubble walls in the theory of vacuum decay. As an outcome of our investigation of the BPS walls, we found that the decay rate of dS vacua to a collapsing space with a negative vacuum energy can be quite large. The parts of space that experience a decay to a collapsing space, or to a Minkowski vacuum, never return back to dS space. The channels of irreversible vacuum decay serve as sinks for the probability flow. The existence of such sinks is a distinguishing feature of the landscape. We show that it strongly affects the probability distributions in string cosmology.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2006
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spelling cern-9546562023-03-14T20:22:13Zdoi:10.1103/PhysRevD.74.086010http://cds.cern.ch/record/954656engCeresole, AnnaDall'Agata, GianguidoGiryavets, AlexanderKallosh, RenataLinde, Andrei D.Domain walls, near-BPS bubbles, and probabilities in the landscapeParticle Physics - TheoryWe develop a theory of static BPS domain walls in stringy landscape and present a large family of BPS walls interpolating between different supersymmetric vacua. Examples include KKLT models, STU models, type IIB multiple flux vacua, and models with several Minkowski and AdS vacua. After the uplifting, some of the vacua become dS, whereas some others remain AdS. The near-BPS walls separating these vacua may be seen as bubble walls in the theory of vacuum decay. As an outcome of our investigation of the BPS walls, we found that the decay rate of dS vacua to a collapsing space with a negative vacuum energy can be quite large. The parts of space that experience a decay to a collapsing space, or to a Minkowski vacuum, never return back to dS space. The channels of irreversible vacuum decay serve as sinks for the probability flow. The existence of such sinks is a distinguishing feature of the landscape. We show that it strongly affects the probability distributions in string cosmology.We develop a theory of static BPS domain walls in stringy landscape and present a large family of BPS walls interpolating between different supersymmetric vacua. Examples include KKLT models, STU models, type IIB multiple flux vacua, and models with several Minkowski and AdS vacua. After the uplifting, some of the vacua become dS, whereas some others remain AdS. The near-BPS walls separating these vacua may be seen as bubble walls in the theory of vacuum decay. As an outcome of our investigation of the BPS walls, we found that the decay rate of dS vacua to a collapsing space with a negative vacuum energy can be quite large. The parts of space that experience a decay to a collapsing space, or to a Minkowski vacuum, never return back to dS space. The channels of irreversible vacuum decay serve as sinks for the probability flow. The existence of such sinks is a distinguishing feature of the landscape. We show that it strongly affects the probability distributions in string cosmology.hep-th/0605266SLAC-PUB-11883CERN-PH-TH-2006-103SU-ITP-2006-17CERN-PH-TH-2006-103SU-ITP-2006-17oai:cds.cern.ch:9546562006-05-29
spellingShingle Particle Physics - Theory
Ceresole, Anna
Dall'Agata, Gianguido
Giryavets, Alexander
Kallosh, Renata
Linde, Andrei D.
Domain walls, near-BPS bubbles, and probabilities in the landscape
title Domain walls, near-BPS bubbles, and probabilities in the landscape
title_full Domain walls, near-BPS bubbles, and probabilities in the landscape
title_fullStr Domain walls, near-BPS bubbles, and probabilities in the landscape
title_full_unstemmed Domain walls, near-BPS bubbles, and probabilities in the landscape
title_short Domain walls, near-BPS bubbles, and probabilities in the landscape
title_sort domain walls, near-bps bubbles, and probabilities in the landscape
topic Particle Physics - Theory
url https://dx.doi.org/10.1103/PhysRevD.74.086010
http://cds.cern.ch/record/954656
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AT kalloshrenata domainwallsnearbpsbubblesandprobabilitiesinthelandscape
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