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  • Open Access

Holographic one-point functions and geodesics in Schwarzschild dS3

Arundhati Goldar*, Nirmalya Kajuri†, and Rhitaparna Pal‡

  • School of Physical Sciences, IIT Mandi, Himachal Pradesh 175005, India

  • *Contact author: d21086@students.iitmandi.ac.in
  • †Contact author: nirmalya@iitmandi.ac.in
  • ‡Contact author: d21089@students.iitmandi.ac.in

Phys. Rev. D 114, 066015 – Published 23 September, 2026

DOI: https://doi.org/10.1103/7hqt-b6r2

Abstract

Grinberg and Maldacena showed that heavy thermal one-point functions in AdS/CFT can encode complex geodesics reaching a black hole singularity. We study the de Sitter analog in three-dimensional Schwarzschild–de Sitter space, restricting to the finite cyclic quotients dS3/Zq. We define a one-point function through a differentiate dictionary and show that an analogous result holds for the Bunch-Davies-prepared integral. Using the exact light-field Green’s function, the bulk integral reduces exactly to a convergent one-dimensional transform, whose large-mass limit is controlled by the near-defect region and governed by a complex saddle. Its action reproduces a complex geodesic length from future infinity to the conical defect, whose real part is the renormalized boundary-to-horizon proper time and whose imaginary part is the horizon-to-defect distance. The imaginary part appears in the one-point coefficient normalized in the Lorentzian source basis; in the Euclidean basis the same saddle contributes only the real part, the two being related by a fixed connection factor.

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