Quantum Fluctuations and Newton-Cartan Geometry for Non-Relativistic de Sitter space
Pith reviewed 2026-05-10 17:41 UTC · model grok-4.3
The pith
The one-loop partition function of the non-relativistic Schwarzian action for de Sitter gravity produces a temperature-dependent prefactor scaling as T squared.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
The central claim is that the one-loop partition function of the non-relativistic Schwarzian boundary action, computed with a path-integral measure obtained from the Ostrogradsky formalism, contains a temperature-dependent prefactor that scales as T squared, with the power agreeing with the counting of the four global symmetry generators, while the corresponding bulk description is a torsionless Newton-Cartan geometry obeying the equations of a non-relativistic JT-like action that uplifts to three-dimensional Lorentzian geometry.
What carries the argument
The Ostrogradsky formalism applied to the higher-derivative Schwarzian action, which supplies the path-integral measure used to extract the one-loop quantum fluctuations and their T squared prefactor.
Load-bearing premise
The Ostrogradsky-derived path-integral measure correctly captures the quantum fluctuations of the non-relativistic Schwarzian action without hidden gauge-fixing or measure anomalies that would alter the T squared scaling.
What would settle it
An independent computation of the same one-loop partition function by the coadjoint-orbit method that yields a temperature power different from two would falsify the central boundary result.
read the original abstract
We study a non-relativistic realisation of two-dimensional de Sitter gravity both from its boundary and bulk description with the goal of learning about de Sitter space and paving the way for extending the holographic duality into a non-relativistic direction. On the boundary side, we analyse the Schwarzian-type boundary action associated with non-relativistic de Sitter gravity and evaluate its one-loop partition function in order to compute its quantum fluctuations. Rather than relying on the coadjoint-orbit construction, we derive the path integral measure directly from the action using the Ostrogradsky formalism. We find a temperature-dependent prefactor scaling as $T^2$, of which the power agrees with the counting of the four global symmetry generators present. On the bulk side, we construct the corresponding torsionless Newton-Cartan geometry and show that it satisfies the equations of motion of a non-relativistic JT-like action and uplift the geometry to a three-dimensional Lorentzian geometry.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The manuscript studies non-relativistic two-dimensional de Sitter gravity from boundary and bulk viewpoints. On the boundary, it examines the Schwarzian-type action and computes its one-loop partition function by deriving the path-integral measure directly from the action via the Ostrogradsky formalism (rather than coadjoint orbits), obtaining a temperature-dependent prefactor scaling as T² whose power matches the four global symmetry generators. On the bulk side, it constructs the corresponding torsionless Newton-Cartan geometry, verifies that it satisfies the equations of motion of a non-relativistic JT-like action, and uplifts the geometry to three-dimensional Lorentzian space.
Significance. If the Ostrogradsky-derived measure is shown to be free of additional Jacobians or anomalies, the work supplies an independent route to the one-loop prefactor in non-relativistic Schwarzian theories and thereby strengthens the foundations for non-relativistic holographic dualities involving de Sitter space. The explicit bulk geometric construction and its consistency with the equations of motion provide a useful cross-check. The agreement between the computed power and the symmetry-generator count is a concrete, falsifiable feature that adds value if the measure derivation is fully controlled.
major comments (1)
- [Boundary analysis and one-loop partition function] The central claim that the Ostrogradsky reduction yields a measure whose functional determinant (or zero-mode factors) produces precisely a T² prefactor with no extra T-dependent contributions from auxiliary momenta, gauge redundancies, or regularization artifacts is load-bearing for the reported result. Explicit verification of the phase-space measure, including any Fadeev-Popov or Jacobian factors tied to the four global symmetries, is required before the numerical agreement with generator counting can be regarded as confirmatory.
Simulated Author's Rebuttal
We thank the referee for their careful reading and constructive feedback on our manuscript. We address the major comment on the boundary analysis below and will revise the manuscript to provide the requested explicit details on the phase-space measure.
read point-by-point responses
-
Referee: The central claim that the Ostrogradsky reduction yields a measure whose functional determinant (or zero-mode factors) produces precisely a T² prefactor with no extra T-dependent contributions from auxiliary momenta, gauge redundancies, or regularization artifacts is load-bearing for the reported result. Explicit verification of the phase-space measure, including any Fadeev-Popov or Jacobian factors tied to the four global symmetries, is required before the numerical agreement with generator counting can be regarded as confirmatory.
Authors: We agree that making the verification of the phase-space measure fully explicit strengthens the result. In the manuscript we derive the path-integral measure directly from the action via the Ostrogradsky formalism; this procedure reduces the phase space while incorporating the auxiliary momenta and the second-class constraints inherent to the action. The resulting T² prefactor is generated by the four zero modes associated with the global symmetries. To address the concern about possible additional contributions, we will revise the manuscript to include a detailed computation of the full phase-space measure. This will explicitly evaluate the Jacobian arising from the Ostrogradsky coordinate transformation, compute the Fadeev-Popov determinant for the four global symmetries, and demonstrate that regularization artifacts do not introduce further T-dependent factors. We expect this addition to confirm that the prefactor remains precisely T². revision: yes
Circularity Check
No significant circularity; Ostrogradsky measure derivation is independent
full rationale
The paper derives the path-integral measure for the non-relativistic Schwarzian action directly via the Ostrogradsky formalism applied to the higher-derivative boundary action, explicitly avoiding the coadjoint-orbit construction. The resulting T² prefactor is obtained from this computation and separately noted to agree with the count of four global symmetry generators, but the derivation itself does not reduce to or presuppose that counting. No load-bearing self-citations, fitted inputs renamed as predictions, or ansatz smuggling appear in the central chain. The bulk Newton-Cartan geometry construction is a separate analysis and does not feed back into the boundary fluctuation result. The derivation is therefore self-contained against external benchmarks.
Axiom & Free-Parameter Ledger
axioms (2)
- domain assumption The non-relativistic limit of two-dimensional de Sitter gravity admits a well-defined Schwarzian-type boundary action whose higher-derivative terms can be handled by the Ostrogradsky formalism without anomalies.
- domain assumption A torsionless Newton-Cartan geometry in two dimensions can be uplifted to a three-dimensional Lorentzian geometry while preserving the equations of motion of the non-relativistic JT-like action.
Reference graph
Works this paper leans on
-
[1]
J. M. Maldacena,The LargeNlimit of superconformal field theories and supergravity,Adv. Theor. Math. Phys.2(1998) 231–252 [hep-th/9711200]
work page internal anchor Pith review Pith/arXiv arXiv 1998
-
[2]
Teitelboim,Gravitation and Hamiltonian Structure in Two Space-Time Dimensions,Phys
C. Teitelboim,Gravitation and Hamiltonian Structure in Two Space-Time Dimensions,Phys. Lett. B126(1983) 41–45
work page 1983
-
[3]
Jackiw,Lower Dimensional Gravity,Nucl
R. Jackiw,Lower Dimensional Gravity,Nucl. Phys. B252(1985) 343–356. – 26 –
work page 1985
-
[4]
Gapless Spin-Fluid Ground State in a Random Quantum Heisenberg Magnet
S. Sachdev and J. Ye,Gapless spin fluid ground state in a random, quantum Heisenberg magnet,Phys. Rev. Lett.70(1993) 3339 [cond-mat/9212030]
work page Pith review arXiv 1993
-
[5]
A simple model of quantum holography
A. Kitaev, “A simple model of quantum holography.” http://online.kitp.ucsb.edu/online/entangled15/kitaev/, http://online.kitp.ucsb.edu/online/entangled15/kitaev2/, 2015. Talks at KITP, April 7, 2015 and May 27, 2015
work page 2015
-
[6]
Holographic metals and the fractionalized Fermi liquid
S. Sachdev,Holographic metals and the fractionalized Fermi liquid,Phys. Rev. Lett.105(2010) 151602 [1006.3794]
work page Pith review arXiv 2010
-
[7]
Comments on the Sachdev-Ye-Kitaev model
J. Maldacena and D. Stanford,Remarks on the Sachdev-Ye-Kitaev model,Phys. Rev. D94 (2016), no. 10 106002 [1604.07818]
work page Pith review arXiv 2016
-
[8]
AdS$_2$ holography and the SYK model
G. Sárosi,AdS 2 holography and the SYK model,PoSModave2017(2018) 001 [1711.08482]
work page Pith review arXiv 2018
- [9]
-
[10]
T. G. Mertens,The Schwarzian theory — origins,JHEP05(2018) 036 [1801.09605]
work page Pith review arXiv 2018
-
[11]
Dilaton Gravity in Two Dimensions
D. Grumiller, W. Kummer and D. V. Vassilevich,Dilaton gravity in two-dimensions,Phys. Rept.369327–430 [hep-th/0204253]
-
[12]
M. H. Christensen, J. Hartong, N. A. Obers and B. Rollier,Torsional Newton-Cartan Geometry and Lifshitz Holography,Phys. Rev. D89(2014) 061901 [1311.4794]
work page Pith review arXiv 2014
-
[13]
Gauging the Carroll Algebra and Ultra-Relativistic Gravity
J. Hartong,Gauging the Carroll Algebra and Ultra-Relativistic Gravity,JHEP08(2015) 069 [1505.05011]
work page Pith review arXiv 2015
-
[14]
Non-Relativistic Gravity and its Coupling to Matter,
D. Hansen, J. Hartong and N. A. Obers,Non-Relativistic Gravity and its Coupling to Matter, JHEP06(2020) 145 [2001.10277]
-
[15]
D. Hansen, N. A. Obers, G. Oling and B. T. Søgaard,Carroll Expansion of General Relativity, SciPost Phys.13(2022), no. 3 055 [2112.12684]
-
[16]
E. Bergshoeff, J. Figueroa-O’Farrill and J. Gomis,A non-lorentzian primer,SciPost Phys. Lect. Notes69(2023) 1 [2206.12177]
-
[17]
Non-Relativistic Closed String Theory
J. Gomis and H. Ooguri,Nonrelativistic closed string theory,J. Math. Phys.42(2001) 3127–3151 [hep-th/0009181]
work page Pith review arXiv 2001
-
[18]
U. H. Danielsson, A. Guijosa and M. Kruczenski,IIA/B, wound and wrapped,JHEP10(2000) 020 [hep-th/0009182]
work page Pith review arXiv 2000
-
[19]
B. Cardona, J. Gomis and J. M. Pons,Dynamics of Carroll Strings,JHEP07(2016) 050 [1605.05483]
work page Pith review arXiv 2016
-
[20]
L. Bidussi, T. Harmark, J. Hartong, N. A. Obers and G. Oling,Torsional string Newton-Cartan geometry for non-relativistic strings,JHEP02(2022) 116 [2107.00642]
-
[21]
G. Oling and Z. Yan,Aspects of Nonrelativistic Strings,Front. in Phys.10(2022) 832271 [2202.12698]
-
[22]
M. Harksen, D. Hidalgo, W. Sybesma and L. Thorlacius,Carroll strings with an extended symmetry algebra,JHEP05(2024) 206 [2403.01984]
-
[23]
M. Taylor,Lifshitz holography,Class. Quant. Grav.33(2016), no. 3 033001 [1512.03554]
work page Pith review arXiv 2016
-
[24]
J.-M. Lévy-Leblond,Une nouvelle limite non-relativiste du groupe de poincaré,Annales De L Institut Henri Poincare-physique Theorique3(1965) 1–12. – 27 –
work page 1965
-
[25]
Newton-Hooke Algebras, Non-relativistic Branes and Generalized pp-wave Metrics
J. Brugues, J. Gomis and K. Kamimura,Newton-Hooke algebras, non-relativistic branes and generalized pp-wave metrics,Phys. Rev. D73(2006) 085011 [hep-th/0603023]
work page Pith review arXiv 2006
-
[26]
J. G. D. J. R. Derome,Hooke’s symmetries and nonrelativistic cosmological kinematics. — I, Il Nuovo Cimento B (1971-1996)9(1972) 351–376 [10.1007/BF02734453]
-
[27]
R. Aldrovandi, A. L. Barbosa, L. C. B. Crispino and J. G. Pereira,Non-Relativistic spacetimes with cosmological constant,Class. Quant. Grav.16(1999) 495–506 [gr-qc/9801100]
work page internal anchor Pith review arXiv 1999
-
[28]
Gao,Symmetries, matrices, and de Sitter gravity,Conf
Y.-h. Gao,Symmetries, matrices, and de Sitter gravity,Conf. Proc. C0208124(2002) 271–310 [hep-th/0107067]
work page internal anchor Pith review arXiv 2002
-
[29]
D. Grumiller, J. Hartong, S. Prohazka and J. Salzer,Limits of JT gravity,JHEP02(2021) 134 [2011.13870]
- [30]
- [31]
-
[32]
H. Bacry and J. Levy-Leblond,Possible kinematics,J. Math. Phys.9(1968) 1605–1614
work page 1968
-
[33]
G. W. Gibbons and C. E. Patricot,Newton-Hooke space-times, Hpp waves and the cosmological constant,Class. Quant. Grav.20(2003) 5225 [hep-th/0308200]
work page internal anchor Pith review arXiv 2003
-
[34]
The asymptotic dynamics of three-dimensional Einstein gravity with a negative cosmological constant
O. Coussaert, M. Henneaux and P. van Driel,The Asymptotic dynamics of three-dimensional Einstein gravity with a negative cosmological constant,Class. Quant. Grav.12(1995) 2961–2966 [gr-qc/9506019]
work page Pith review arXiv 1995
-
[35]
E. A. Ivanov and V. I. Ogievetsky,The Inverse Higgs Phenomenon in Nonlinear Realizations, Teor. Mat. Fiz.25(1975) 164–177
work page 1975
-
[36]
Flat space holography and the complex Sachdev-Ye-Kitaev model,
H. Afshar, H. A. González, D. Grumiller and D. Vassilevich,Flat space holography and the complex Sachdev-Ye-Kitaev model,Phys. Rev. D101(2020), no. 8 086024 [1911.05739]
- [37]
-
[38]
A. A. Kirillov,Elements of the Theory of Representations, vol. 220 ofGrundlehren der mathematischen Wissenschaften. Springer Berlin, Heidelberg, 1 ed., 1976
work page 1976
-
[39]
Kostant,Quantization and unitary representations
B. Kostant,Quantization and unitary representations. Springer, Berlin, Heidelberg, 1970
work page 1970
-
[40]
Souriau,Structure des systèmes dynamiques
J.-M. Souriau,Structure des systèmes dynamiques. Dunod, Paris, 1970. Réimprimé par les éditions Jacques Gabay, 2008
work page 1970
-
[41]
R. P. Woodard,Ostrogradsky’s theorem on Hamiltonian instability,Scholarpedia10(2015), no. 8 32243 [1506.02210]
work page Pith review arXiv 2015
-
[42]
J. Maldacena, G. J. Turiaci and Z. Yang,Two dimensional Nearly de Sitter gravity,JHEP01 (2021) 139 [1904.01911]
-
[43]
Low-dimensional de Sitter quantum gravity,
J. Cotler, K. Jensen and A. Maloney,Low-dimensional de Sitter quantum gravity,JHEP06 (2020) 048 [1905.03780]
-
[44]
Fermionic Localization of the Schwarzian Theory
D. Stanford and E. Witten,Fermionic Localization of the Schwarzian Theory,JHEP10(2017) 008 [1703.04612]
work page Pith review arXiv 2017
-
[45]
E. Cartan,Sur les variétés à connexion affine et la théorie de la relativité généralisée (première partie),Ann. Éc. Norm. Supér.40(1923) 325–412. – 28 –
work page 1923
-
[46]
Cartan,Sur les variétés à connexion affine et la théorie de la relativité généralisée (suite), Ann
E. Cartan,Sur les variétés à connexion affine et la théorie de la relativité généralisée (suite), Ann. Éc. Norm. Supér.41(1924) 1–25
work page 1924
-
[47]
J. Hartong, N. A. Obers and G. Oling,Review on Non-Relativistic Gravity,Front. in Phys.11 (2023) 1116888 [2212.11309]
- [48]
-
[49]
E. A. Bergshoeff, J. Hartong and J. Rosseel,Torsional Newton–Cartan geometry and the Schrödinger algebra,Class. Quant. Grav.32(2015), no. 13 135017 [1409.5555]
work page Pith review arXiv 2015
-
[50]
Lifshitz space–times for Schr¨ odinger holography,
J. Hartong, E. Kiritsis and N. A. Obers,Lifshitz space–times for Schrödinger holography,Phys. Lett. B746(2015) 318–324 [1409.1519]
work page internal anchor Pith review arXiv 2015
-
[51]
J. Hartong, A. Mehra and J. Musaeus,Galilean fluids from non-relativistic gravity,JHEP10 (2024) 156 [2408.16734]
- [52]
-
[53]
Andringa,Newton-Cartan gravity revisited
R. Andringa,Newton-Cartan gravity revisited. PhD thesis, High-Energy Frontier, Groningen U., Groningen U., 2016
work page 2016
- [54]
-
[55]
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 [2503.08617]
-
[56]
S. Maulik, L. A. Pando Zayas, A. Ray and J. Zhang,Universality in logarithmic temperature corrections to near-extremal rotating black hole thermodynamics in various dimensions,JHEP 06(2024) 034 [2401.16507]
- [57]
-
[58]
Witten,Coadjoint Orbits of the Virasoro Group,Commun
E. Witten,Coadjoint Orbits of the Virasoro Group,Commun. Math. Phys.114(1988) 1
work page 1988
-
[59]
A. Alekseev and S. L. Shatashvili,Path Integral Quantization of the Coadjoint Orbits of the Virasoro Group and 2D Gravity,Nucl. Phys. B323(1989) 719–733
work page 1989
-
[60]
P. Saad, S. H. Shenker and D. Stanford,JT gravity as a matrix integral,1903.11115. – 29 –
work page Pith review arXiv 1903
discussion (0)
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