Complex geodesics in de Sitter space

Abstract The two-point function of a free massive scalar field on a fixed background can be evaluated in the large mass limit by using a semiclassical geodesic approximation. In de Sitter space, however, this poses a puzzle. Certain spacelike separated points are not connected by real geodesics desp...

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Main Authors: Shira Chapman, Damián A. Galante, Eleanor Harris, Sameer U. Sheorey, David Vegh
Format: Article
Language:English
Published: SpringerOpen 2023-03-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP03(2023)006
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author Shira Chapman
Damián A. Galante
Eleanor Harris
Sameer U. Sheorey
David Vegh
author_facet Shira Chapman
Damián A. Galante
Eleanor Harris
Sameer U. Sheorey
David Vegh
author_sort Shira Chapman
collection DOAJ
description Abstract The two-point function of a free massive scalar field on a fixed background can be evaluated in the large mass limit by using a semiclassical geodesic approximation. In de Sitter space, however, this poses a puzzle. Certain spacelike separated points are not connected by real geodesics despite the corresponding two-point function in the Bunch-Davies state being non-vanishing. We resolve this puzzle by considering complex geodesics after analytically continuing to the sphere. We compute one-loop corrections to the correlator and discuss the implications of our results to de Sitter holography.
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spelling doaj.art-f04b14bbc31945d5983bf909c22a73b22023-06-25T11:05:35ZengSpringerOpenJournal of High Energy Physics1029-84792023-03-012023312910.1007/JHEP03(2023)006Complex geodesics in de Sitter spaceShira Chapman0Damián A. Galante1Eleanor Harris2Sameer U. Sheorey3David Vegh4Department of Physics, Ben-Gurion University of the NegevDepartment of Mathematics, King‘s College LondonDepartment of Mathematics, King‘s College LondonDepartment of Mathematics, King‘s College LondonCentre for Theoretical Physics, Department of Physics and Astronomy, Queen Mary University of LondonAbstract The two-point function of a free massive scalar field on a fixed background can be evaluated in the large mass limit by using a semiclassical geodesic approximation. In de Sitter space, however, this poses a puzzle. Certain spacelike separated points are not connected by real geodesics despite the corresponding two-point function in the Bunch-Davies state being non-vanishing. We resolve this puzzle by considering complex geodesics after analytically continuing to the sphere. We compute one-loop corrections to the correlator and discuss the implications of our results to de Sitter holography.https://doi.org/10.1007/JHEP03(2023)006AdS-CFT Correspondencede Sitter space
spellingShingle Shira Chapman
Damián A. Galante
Eleanor Harris
Sameer U. Sheorey
David Vegh
Complex geodesics in de Sitter space
Journal of High Energy Physics
AdS-CFT Correspondence
de Sitter space
title Complex geodesics in de Sitter space
title_full Complex geodesics in de Sitter space
title_fullStr Complex geodesics in de Sitter space
title_full_unstemmed Complex geodesics in de Sitter space
title_short Complex geodesics in de Sitter space
title_sort complex geodesics in de sitter space
topic AdS-CFT Correspondence
de Sitter space
url https://doi.org/10.1007/JHEP03(2023)006
work_keys_str_mv AT shirachapman complexgeodesicsindesitterspace
AT damianagalante complexgeodesicsindesitterspace
AT eleanorharris complexgeodesicsindesitterspace
AT sameerusheorey complexgeodesicsindesitterspace
AT davidvegh complexgeodesicsindesitterspace