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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...
Autores principales: | , , , , |
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Lenguaje: | eng |
Publicado: |
2006
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1103/PhysRevD.74.086010 http://cds.cern.ch/record/954656 |
_version_ | 1780910013234020352 |
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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. |
id | cern-954656 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2006 |
record_format | invenio |
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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