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Moduli Stabilisation on the Worldsheet

We consider compactifications of type II string theory using exact internal CFT's with central charge $c=9+\epsilon$, $|\epsilon| \ll 1$, leading to an effective potential for the dilaton. For $\epsilon>0$ the potential is positive and the dilaton is ultimately driven to weak coupling. For $...

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Detalles Bibliográficos
Autores principales: Deo, Jawad Arshad, Lambert, Neil, Recknagel, Andreas
Lenguaje:eng
Publicado: 2010
Materias:
Acceso en línea:https://dx.doi.org/10.1007/JHEP02(2011)111
http://cds.cern.ch/record/1316418
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author Deo, Jawad Arshad
Lambert, Neil
Recknagel, Andreas
author_facet Deo, Jawad Arshad
Lambert, Neil
Recknagel, Andreas
author_sort Deo, Jawad Arshad
collection CERN
description We consider compactifications of type II string theory using exact internal CFT's with central charge $c=9+\epsilon$, $|\epsilon| \ll 1$, leading to an effective potential for the dilaton. For $\epsilon>0$ the potential is positive and the dilaton is ultimately driven to weak coupling. For $\epsilon<0$ the dilaton is driven to strong coupling, but we can stabilise the background by including D-branes. The resulting minimum admits an $AdS_4$ solution where the cosmological constant is of the order $\epsilon^3$ and the string coupling constant is of order $\epsilon$. Furthermore these CFT's typically do not possess any massless or tachyonic modes. Thus these vacua provide exact CFT descriptions of moduli stabilisation in weakly coupled string theory.
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institution Organización Europea para la Investigación Nuclear
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publishDate 2010
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spelling cern-13164182023-03-14T20:30:55Zdoi:10.1007/JHEP02(2011)111http://cds.cern.ch/record/1316418engDeo, Jawad ArshadLambert, NeilRecknagel, AndreasModuli Stabilisation on the WorldsheetParticle Physics - TheoryWe consider compactifications of type II string theory using exact internal CFT's with central charge $c=9+\epsilon$, $|\epsilon| \ll 1$, leading to an effective potential for the dilaton. For $\epsilon>0$ the potential is positive and the dilaton is ultimately driven to weak coupling. For $\epsilon<0$ the dilaton is driven to strong coupling, but we can stabilise the background by including D-branes. The resulting minimum admits an $AdS_4$ solution where the cosmological constant is of the order $\epsilon^3$ and the string coupling constant is of order $\epsilon$. Furthermore these CFT's typically do not possess any massless or tachyonic modes. Thus these vacua provide exact CFT descriptions of moduli stabilisation in weakly coupled string theory.We consider compactifications of type II string theory using exact internal CFT's with central charge $c=9+\epsilon$, $|\epsilon| \ll 1$, leading to an effective potential for the dilaton. For $\epsilon>0$ the potential is positive and the dilaton is ultimately driven to weak coupling. For $\epsilon<0$ the dilaton is driven to strong coupling, but we can stabilise the background by including D-branes. The resulting minimum admits an $AdS_4$ solution where the cosmological constant is of the order $\epsilon^3$ and the string coupling constant is of order $\epsilon$. Furthermore these CFT's typically do not possess any massless or tachyonic modes. Thus these vacua provide exact CFT descriptions of moduli stabilisation in weakly coupled string theory.arXiv:1012.3972oai:cds.cern.ch:13164182010-12-20
spellingShingle Particle Physics - Theory
Deo, Jawad Arshad
Lambert, Neil
Recknagel, Andreas
Moduli Stabilisation on the Worldsheet
title Moduli Stabilisation on the Worldsheet
title_full Moduli Stabilisation on the Worldsheet
title_fullStr Moduli Stabilisation on the Worldsheet
title_full_unstemmed Moduli Stabilisation on the Worldsheet
title_short Moduli Stabilisation on the Worldsheet
title_sort moduli stabilisation on the worldsheet
topic Particle Physics - Theory
url https://dx.doi.org/10.1007/JHEP02(2011)111
http://cds.cern.ch/record/1316418
work_keys_str_mv AT deojawadarshad modulistabilisationontheworldsheet
AT lambertneil modulistabilisationontheworldsheet
AT recknagelandreas modulistabilisationontheworldsheet