Cargando…
The Swampland, Moduli and Holography
<!--HTML-->String compactifications are essential for connecting string theory to low energy particle physics and cosmology. Moduli stabilisation gives rise to effective Lagrangians that capture the low-energy degrees of freedom. Much recent interest has been on swampland consistency condition...
Autor principal: | |
---|---|
Lenguaje: | eng |
Publicado: |
2019
|
Materias: | |
Acceso en línea: | http://cds.cern.ch/record/2679353 |
_version_ | 1780962886935379968 |
---|---|
author | Conlon, Joe |
author_facet | Conlon, Joe |
author_sort | Conlon, Joe |
collection | CERN |
description | <!--HTML-->String compactifications are essential for connecting string theory to low energy particle physics and cosmology. Moduli stabilisation gives rise to effective Lagrangians that capture the low-energy degrees of freedom. Much recent interest has been on swampland consistency conditions on such effective field theories - which low energy Lagrangians can arise from quantum gravity? How are moduli Lagrangians constrained by consistency with quantum gravity? As moduli stabilisation scenarios often exist in AdS space, we can also ask: what do swampland conditions mean in the context of AdS/CFT? Focussing in particular on the Large Volume Scenario, I describe work towards developing a holographic understanding of moduli stabilisation and swampland consistency conditions. |
id | cern-2679353 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2019 |
record_format | invenio |
spelling | cern-26793532022-11-02T22:34:59Zhttp://cds.cern.ch/record/2679353engConlon, JoeThe Swampland, Moduli and HolographyString Geometry and String Phenomenology InstituteTH institutes<!--HTML-->String compactifications are essential for connecting string theory to low energy particle physics and cosmology. Moduli stabilisation gives rise to effective Lagrangians that capture the low-energy degrees of freedom. Much recent interest has been on swampland consistency conditions on such effective field theories - which low energy Lagrangians can arise from quantum gravity? How are moduli Lagrangians constrained by consistency with quantum gravity? As moduli stabilisation scenarios often exist in AdS space, we can also ask: what do swampland conditions mean in the context of AdS/CFT? Focussing in particular on the Large Volume Scenario, I describe work towards developing a holographic understanding of moduli stabilisation and swampland consistency conditions.oai:cds.cern.ch:26793532019 |
spellingShingle | TH institutes Conlon, Joe The Swampland, Moduli and Holography |
title | The Swampland, Moduli and Holography |
title_full | The Swampland, Moduli and Holography |
title_fullStr | The Swampland, Moduli and Holography |
title_full_unstemmed | The Swampland, Moduli and Holography |
title_short | The Swampland, Moduli and Holography |
title_sort | swampland, moduli and holography |
topic | TH institutes |
url | http://cds.cern.ch/record/2679353 |
work_keys_str_mv | AT conlonjoe theswamplandmoduliandholography AT conlonjoe stringgeometryandstringphenomenologyinstitute AT conlonjoe swamplandmoduliandholography |