Gravitational Wilson lines in 3D de Sitter

Abstract We construct local probes in the static patch of Euclidean dS3 gravity. These probes are Wilson line operators, designed by exploiting the Chern-Simons formulation of 3D gravity. Our prescription uses non-unitary representations of so (4) ≃ su (2) L × su(2) R , and we evaluate the Wilson li...

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Main Authors: Alejandra Castro, Philippe Sabella-Garnier, Claire Zukowski
Format: Article
Language:English
Published: SpringerOpen 2020-07-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP07(2020)202
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author Alejandra Castro
Philippe Sabella-Garnier
Claire Zukowski
author_facet Alejandra Castro
Philippe Sabella-Garnier
Claire Zukowski
author_sort Alejandra Castro
collection DOAJ
description Abstract We construct local probes in the static patch of Euclidean dS3 gravity. These probes are Wilson line operators, designed by exploiting the Chern-Simons formulation of 3D gravity. Our prescription uses non-unitary representations of so (4) ≃ su (2) L × su(2) R , and we evaluate the Wilson line for states satisfying a singlet condition. We discuss how to reproduce the Green’s functions of massive scalar fields in dS3, the construction of bulk fields, and the quasinormal mode spectrum. We also discuss the interpretation of our construction in Lorentzian signature in the inflationary patch, via SL(2, ℂ) Chern-Simons theory.
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spelling doaj.art-f4d3d2b2c8964ce18bd874cce79684b12022-12-22T00:09:09ZengSpringerOpenJournal of High Energy Physics1029-84792020-07-012020714010.1007/JHEP07(2020)202Gravitational Wilson lines in 3D de SitterAlejandra Castro0Philippe Sabella-Garnier1Claire Zukowski2Institute for Theoretical Physics, University of AmsterdamLorentz Institute, Leiden UniversityInstitute for Theoretical Physics, University of AmsterdamAbstract We construct local probes in the static patch of Euclidean dS3 gravity. These probes are Wilson line operators, designed by exploiting the Chern-Simons formulation of 3D gravity. Our prescription uses non-unitary representations of so (4) ≃ su (2) L × su(2) R , and we evaluate the Wilson line for states satisfying a singlet condition. We discuss how to reproduce the Green’s functions of massive scalar fields in dS3, the construction of bulk fields, and the quasinormal mode spectrum. We also discuss the interpretation of our construction in Lorentzian signature in the inflationary patch, via SL(2, ℂ) Chern-Simons theory.http://link.springer.com/article/10.1007/JHEP07(2020)202Chern-Simons TheoriesClassical Theories of GravityWilson’t Hooft and Polyakov loops
spellingShingle Alejandra Castro
Philippe Sabella-Garnier
Claire Zukowski
Gravitational Wilson lines in 3D de Sitter
Journal of High Energy Physics
Chern-Simons Theories
Classical Theories of Gravity
Wilson
’t Hooft and Polyakov loops
title Gravitational Wilson lines in 3D de Sitter
title_full Gravitational Wilson lines in 3D de Sitter
title_fullStr Gravitational Wilson lines in 3D de Sitter
title_full_unstemmed Gravitational Wilson lines in 3D de Sitter
title_short Gravitational Wilson lines in 3D de Sitter
title_sort gravitational wilson lines in 3d de sitter
topic Chern-Simons Theories
Classical Theories of Gravity
Wilson
’t Hooft and Polyakov loops
url http://link.springer.com/article/10.1007/JHEP07(2020)202
work_keys_str_mv AT alejandracastro gravitationalwilsonlinesin3ddesitter
AT philippesabellagarnier gravitationalwilsonlinesin3ddesitter
AT clairezukowski gravitationalwilsonlinesin3ddesitter