Complex Geodesics in the Nariai Geometry
Pith reviewed 2026-05-19 17:26 UTC · model grok-4.3
The pith
The two-point correlation function in Nariai geometry equals a sum over complex geodesics obtained by analytic continuation from a sphere product, with phases retained to eliminate spurious singularities.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
Utilizing the heat kernel formalism, the two-point correlation function is obtained from a geodesic approximation on a product of spheres. By analytically continuing one of the spheres, the correlation function in the Nariai geometry is derived as a sum over complex geodesics. The phase of each geodesic contribution must be accounted for to prevent spurious singularities.
What carries the argument
Analytic continuation of the geodesic sum (via heat kernel) from the sphere product to the Nariai geometry, keeping complex phases.
If this is right
- The correlator is expressed as an explicit sum over complex geodesics rather than real ones.
- Each term must carry its full complex phase; dropping the phase creates artificial singularities.
- The result reduces to known de Sitter expressions when the appropriate limit is taken.
- The heat-kernel route captures the heavy-mass limit without further corrections in this geometry.
Where Pith is reading between the lines
- The same continuation procedure could be applied to other near-horizon or product geometries that admit sphere-factor descriptions.
- Phase retention may be required in holographic calculations that rely on complex saddle points to obtain physically sensible correlators.
- Numerical checks in the large-mass limit could verify whether the continued sum matches direct field-theoretic computations.
Load-bearing premise
The geodesic approximation to the two-point function remains valid under analytic continuation from the product of spheres to the Nariai geometry.
What would settle it
An independent calculation of the same two-point function by direct mode expansion in Nariai coordinates that produces a different functional form or different singularity locations.
read the original abstract
We study two-point correlation functions of heavy scalar fields in the Nariai geometry. Utilizing the heat kernel formalism, we obtain this result from a geodesic approximation to the two-point function on a product of spheres. By analytically continuing one of the spheres, we obtain the correlation function in the Nariai geometry. This result involves a sum over complex geodesics, extending previous results in pure de Sitter space. We emphasize the important role of the phase of each geodesic contribution, which needs to be taken into account to avoid spurious singularities in the correlator.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper computes two-point correlation functions of heavy scalar fields in the Nariai geometry by applying the heat kernel formalism to obtain a geodesic approximation on the product of two spheres, then analytically continuing one sphere factor to reach the Nariai metric. The resulting correlator is expressed as a sum over complex geodesics, extending prior de Sitter results, with the phase of each geodesic contribution retained to eliminate spurious singularities.
Significance. If the analytic continuation is shown to preserve the geodesic saddles and phases without introducing new contributions from the altered global structure or curvature, the result would usefully generalize complex-geodesic methods from pure de Sitter to the Nariai background. This could aid calculations of heavy-field correlators in spacetimes with horizons and different topology, provided the heavy-mass limit and phase continuity are rigorously controlled.
major comments (2)
- [analytic continuation step (post-§2)] The central step of analytic continuation from S²×S² to the Nariai geometry (described in the abstract and presumably detailed after the heat-kernel setup) assumes that the complex geodesics and their phases remain valid without additional saddles or jumps in the imaginary part when the metric signature changes. No explicit path specification, demonstration of path-independence, or cross-check against the pure dS₂ limit is indicated, which is load-bearing for the claim that retaining phases cancels spurious singularities.
- [heat kernel formalism section] The heat-kernel derivation on the sphere product is used to justify the heavy-field limit, but the manuscript provides no error estimates or verification that the geodesic approximation survives the continuation without corrections arising from the changed curvature or global structure (as required for the Nariai case).
minor comments (2)
- [results section] Clarify the notation for the complex geodesic lengths and phases in the final sum; ensure they are defined consistently with the continuation parameter.
- [discussion] Add a brief comparison table or plot showing the Nariai correlator against the pure de Sitter limit in a controlled regime to illustrate the extension.
Simulated Author's Rebuttal
We are grateful to the referee for their detailed and insightful comments, which have helped us identify areas where the manuscript can be improved. We address each major comment below and commit to making the necessary revisions to clarify the analytic continuation and strengthen the justification of the approximations used.
read point-by-point responses
-
Referee: [analytic continuation step (post-§2)] The central step of analytic continuation from S²×S² to the Nariai geometry (described in the abstract and presumably detailed after the heat-kernel setup) assumes that the complex geodesics and their phases remain valid without additional saddles or jumps in the imaginary part when the metric signature changes. No explicit path specification, demonstration of path-independence, or cross-check against the pure dS₂ limit is indicated, which is load-bearing for the claim that retaining phases cancels spurious singularities.
Authors: We thank the referee for highlighting this important point. Upon review, we recognize that the details of the analytic continuation path were not sufficiently explicit in the original manuscript. In the revised version, we will specify the analytic continuation path in the complex plane for the sphere radius parameter, demonstrate that the complex geodesics and their phases continue smoothly without introducing new saddles or jumps in the imaginary part, and provide a cross-check by recovering the known pure de Sitter results in the appropriate limit. We will also argue for path-independence by showing that the relevant geodesics lie in the same homotopy class and that the phase is determined by the continuous variation of the geodesic length. This will reinforce that retaining the phases indeed cancels the spurious singularities as claimed. revision: yes
-
Referee: [heat kernel formalism section] The heat-kernel derivation on the sphere product is used to justify the heavy-field limit, but the manuscript provides no error estimates or verification that the geodesic approximation survives the continuation without corrections arising from the changed curvature or global structure (as required for the Nariai case).
Authors: We agree that error estimates and verification of the approximation's robustness under continuation would enhance the manuscript. The heat kernel expansion on the sphere product yields the geodesic approximation with corrections that are exponentially suppressed in the heavy mass limit. In the revision, we will include explicit error bounds for this approximation and provide a discussion verifying that these bounds persist under the analytic continuation to the Nariai geometry. Since the continuation affects the metric continuously and the Nariai space has constant curvature in each factor, no new corrections from curvature changes or global topology are expected at leading order. We will add this analysis to the heat kernel section. revision: yes
Circularity Check
No circularity: derivation uses standard analytic continuation from sphere product via heat kernel
full rationale
The paper obtains the Nariai two-point function by first applying the geodesic approximation and heat kernel formalism on the product of spheres, then analytically continuing one sphere factor. This is a conventional extension of prior de Sitter results and does not reduce any claimed prediction or phase retention to a self-definition, fitted input, or self-citation chain within the paper's own equations. The derivation remains self-contained against external benchmarks such as the known sphere-product heat kernel and the analytic continuation procedure itself.
Axiom & Free-Parameter Ledger
axioms (2)
- domain assumption Geodesic approximation accurately captures the two-point function of heavy scalars via the heat kernel on the sphere product.
- domain assumption Analytic continuation from the sphere product yields the correct Nariai correlator without introducing uncontrolled errors.
Reference graph
Works this paper leans on
-
[1]
The Black Hole Singularity in AdS/CFT
L. Fidkowski, V. Hubeny, M. Kleban, and S. Shenker, “The Black hole singularity in AdS / CFT,”JHEP02(2004) 014,arXiv:hep-th/0306170
work page internal anchor Pith review Pith/arXiv arXiv 2004
-
[2]
On Charged Black Holes in Anti-de Sitter Space
D. Brecher, J. He, and M. Rozali, “On charged black holes in anti-de Sitter space,” JHEP04(2005) 004,arXiv:hep-th/0410214. – 19 –
work page internal anchor Pith review Pith/arXiv arXiv 2005
-
[3]
Excursions beyond the horizon: Black hole singularities in Yang-Mills theories (I)
G. Festuccia and H. Liu, “Excursions beyond the horizon: Black hole singularities in Yang-Mills theories. I.,”JHEP04(2006) 044,arXiv:hep-th/0506202
work page internal anchor Pith review Pith/arXiv arXiv 2006
-
[4]
N. ˇCeplak, H. Liu, A. Parnachev, and S. Valach, “Black hole singularity from OPE,” JHEP10(2024) 105,arXiv:2404.17286 [hep-th]
-
[5]
Imprint of the black hole singularity on thermal two-point functions
N. Afkhami-Jeddi, S. Caron-Huot, J. Chakravarty, and A. Maloney, “Imprint of the black hole singularity on thermal two-point functions,”arXiv:2510.21673 [hep-th]
work page internal anchor Pith review Pith/arXiv arXiv
-
[6]
Late-time correlators and complex geodesics in de Sitter space,
L. Aalsma, M. M. Faruk, J. P. van der Schaar, M. R. Visser, and J. de Witte, “Late-time correlators and complex geodesics in de Sitter space,”SciPost Phys.15 no. 1, (2023) 031,arXiv:2212.01394 [hep-th]
-
[7]
Complex geodesics in de Sitter space,
S. Chapman, D. A. Galante, E. Harris, S. U. Sheorey, and D. Vegh, “Complex geodesics in de Sitter space,”JHEP03(2023) 006,arXiv:2212.01398 [hep-th]
-
[8]
A paucity of bulk entangling surfaces: AdS wormholes with de Sitter interiors
S. Fischetti, D. Marolf, and A. C. Wall, “A paucity of bulk entangling surfaces: AdS wormholes with de Sitter interiors,”Class. Quant. Grav.32(2015) 065011, arXiv:1409.6754 [hep-th]
work page internal anchor Pith review Pith/arXiv arXiv 2015
-
[9]
Timelike entanglement entropy,
K. Doi, J. Harper, A. Mollabashi, T. Takayanagi, and Y. Taki, “Timelike entanglement entropy,”JHEP05(2023) 052,arXiv:2302.11695 [hep-th]
-
[10]
An observer’s measure of de Sitter entropy,
M. Mirbabayi, “An observer’s measure of de Sitter entropy,”JHEP10(2024) 077, arXiv:2311.07724 [hep-th]
-
[11]
Heat kernel expansion: user's manual
D. V. Vassilevich, “Heat kernel expansion: User’s manual,”Phys. Rept.388(2003) 279–360,arXiv:hep-th/0306138
work page internal anchor Pith review Pith/arXiv arXiv 2003
-
[12]
Harmonic analysis and propagators on homogeneous spaces,
R. Camporesi, “Harmonic analysis and propagators on homogeneous spaces,”Phys. Rept.196(1990) 1–134
work page 1990
-
[13]
Schulman,Techniques and Applications of Path Integration
L. Schulman,Techniques and Applications of Path Integration. Dover Books on Physics. Dover Publications, 2012
work page 2012
-
[14]
Gravitational dynamics of near-extreme Kerr (Anti-)de Sitter black holes,
F. Mariani and C. Toldo, “Gravitational dynamics of near-extreme Kerr (Anti-)de Sitter black holes,”JHEP02(2026) 052,arXiv:2505.02674 [hep-th]
-
[15]
Supersymmetric, cold and lukewarm black holes in cosmological Einstein-Maxwell theory
L. J. Romans, “Supersymmetric, cold and lukewarm black holes in cosmological Einstein-Maxwell theory,”Nucl. Phys. B383(1992) 395–415,arXiv:hep-th/9203018
work page internal anchor Pith review Pith/arXiv arXiv 1992
-
[16]
Limits on the Statistical Description of Charged de Sitter Black Holes
L. Aalsma, P. Lin, J. P. van der Schaar, G. Shiu, and W. Sybesma, “Limits on the Statistical Description of Charged de Sitter Black Holes,”arXiv:2511.03867 [hep-th]
work page internal anchor Pith review Pith/arXiv arXiv
-
[17]
Static sphere observers and geodesics in Schwarzschild-de Sitter spacetime,
M. M. Faruk, E. Morvan, and J. P. van der Schaar, “Static sphere observers and geodesics in Schwarzschild-de Sitter spacetime,”JCAP05(2024) 118, arXiv:2312.06878 [gr-qc]. – 20 –
-
[18]
De Sitter Holography: Fluctuations, Anomalous Symmetry, and Wormholes,
L. Susskind, “De Sitter Holography: Fluctuations, Anomalous Symmetry, and Wormholes,”Universe7no. 12, (2021) 464,arXiv:2106.03964 [hep-th]
-
[19]
Quasinormal modes and the switchback effect in Schwarzschild-de Sitter,
M. M. Faruk, F. Rost, and J. P. van der Schaar, “Quasinormal modes and the switchback effect in Schwarzschild-de Sitter,”JHEP07(2025) 050,arXiv:2501.01388 [hep-th]
-
[20]
Logarithmic corrections to near-extremal entropy of charged de Sitter black holes,
S. Maulik, A. Mitra, D. Mukherjee, and A. Ray, “Logarithmic corrections to near-extremal entropy of charged de Sitter black holes,”JHEP01(2026) 156, arXiv:2503.08617 [hep-th]
-
[21]
The wavefunction of a quantum S 1 ×S 2 universe,
G. J. Turiaci and C.-H. Wu, “The wavefunction of a quantum S 1 ×S 2 universe,” JHEP07(2025) 158,arXiv:2503.14639 [hep-th]
-
[22]
Quantum corrections to the path integral of near extremal de Sitter black holes,
M. J. Blacker, A. Castro, W. Sybesma, and C. Toldo, “Quantum corrections to the path integral of near extremal de Sitter black holes,”JHEP08(2025) 120, arXiv:2503.14623 [hep-th]
-
[23]
P. Arnaudo, G. Bonelli, and A. Tanzini, “One loop corrections to the thermodynamics of near-extremal Kerr-(A)dS black holes from Heun equation,”JHEP12(2025) 018, arXiv:2506.08959 [hep-th]
- [24]
-
[25]
NIST Digital Library of Mathematical Functions.HTTPS://DLMF.NIST.GOV/. Accessed: 2026-04-23
work page 2026
-
[26]
Hypergeometric function — Wikipedia
“Hypergeometric function — Wikipedia.” https://en.wikipedia.org/wiki/Hypergeometric_function. Accessed: 2026-01-27. – 21 –
work page 2026
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.