REVIEW 4 major objections 4 minor 1 cited by
The paper claims that the two-dimensional Ising model deformed by its thermal operator and placed on de Sitter space is exactly solvable, and that exact late-time correlators resum the secular logarithms that wreck conformal perturbation th
Reviewed by Pith at T0; open to challenge. T0 means a machine referee read the full paper against a public rubric. the ladder, T0–T4 →
T0 review · deepseek-v4-flash
2026-08-02 02:43 UTC pith:KM77X6EM
load-bearing objection The exact dS Ising results are solid and worth refereeing; the spin/disorder exponent claim is a plausible but under-supported add-on that needs a closer look. the 4 major comments →
Ising the way into de Sitter
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
The central discovery, on the paper's own terms, is that the thermal deformation of the Ising CFT on the sphere admits an exact fermionic description as a free massive Majorana fermion, and this makes a set of de Sitter observables exactly computable. The late-time two-point function of the energy operator behaves as (1/4ℓ^2)(2πν/sinh(2πν))(uL/2)^{-1}, with a ν-independent exponent equal to the CFT dimension; the first subleading term oscillates as cos(2ν log X). The spin and disorder two-point functions, although non-local in the fermion field, are shown to satisfy a non-perturbative constraint, Δ̃σ + Δ̃μ − (Δ̃σ − Δ̃μ)² = ν² + 1/4, with perturbative expansions Δ̃σ = 1/8 + ν/2 + ν² + O(ν³) a
What carries the argument
The load-bearing object is the fermionisation map taking the strongly interacting Ising CFT deformed by ε to a free massive Majorana fermion on the Euclidean sphere. Because the sphere's Dirac spectrum is known exactly, Gaussian integration gives the renormalised partition function and the exact energy two-point function in closed hypergeometric form. For the non-local spin and disorder operators the argument switches to a system of second-order differential equations, quoted from the literature, which together with the exact antipodal ratio Gμ(2)/Gσ(2)=e^{πν} and the pure-power late-time ansatz yields the non-perturbative constraint on scaling dimensions. The late-time behaviour is organise
Load-bearing premise
The spin and disorder late-time exponents are extracted by assuming their two-point functions decay as pure power laws with no logarithmic or oscillatory corrections; if that leading form is not exact, the non-perturbative constraint on Δ̃σ and Δ̃μ does not follow.
What would settle it
Compute the spin two-point function at very large Lorentzian separations by solving the ODE system with high precision and fit the exponent over different fitting windows; if the extracted Δ̃σ shifts with the window, the pure power-law ansatz fails. Separately, the oscillatory subleading term in the thermal correlator, with frequency 2ν and phase arctan(2ν), can be checked numerically: if it is absent, the principal-series resummation claim is wrong.
If this is right
- The thermal two-point function's leading late-time exponent is ν-independent; the entire ν-dependence sits in the normalization (1/4ℓ²)(2πν/sinh 2πν).
- The subleading late-time correlator of the descendant operator εT with ε oscillates as cos(2ν log X), turning naive log²X secular growth into a finite oscillatory signal.
- The spin and disorder late-time dimensions obey Δ̃σ+Δ̃μ−(Δ̃σ−Δ̃μ)² = ν²+1/4 for all ν; at small ν the difference grows linearly and the sum grows quadratically.
- Conformal perturbation theory is generically unreliable at late times: it produces secular logarithms that the exact resummed result removes, so the ν→0 and late-time limits do not commute.
- The two-loop matching of the sphere partition function, with a ζ(3) coefficient from the Bloch–Wigner dilogarithm integral, confirms the Ising/Majorana duality on the sphere and fixes τ=m/2π.
Where Pith is reading between the lines
- The same mechanism — resummation of late-time secular logarithms into principal-series oscillations — is likely to appear in any massive or interacting QFT in dS2 whose two-point functions have a spectral representation; one testable extension is to compare the cos(2ν log X) prediction with O(N) vector models at large N.
- The exact antipodal ratio e^{πν} for spin vs disorder may extend to other Ramond-sector insertions, suggesting a simple exponential law for overlap of order/disorder states in the cylinder description; measuring it on spherical-lattice simulations at finite ν would be a direct check.
- The paper notes that an imaginary thermal deformation would access discrete-series fermions and connects to Fisher zeros on spherical lattices; a concrete follow-up is computing the renormalised partition function at imaginary ν and locating its zeros.
- The relation (6.8) looks like a dS2 bootstrap-style constraint; if the ODE system can be derived from symmetry principles alone, the exponent relations would follow without the free-fermion input, possibly generalising beyond Ising.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. This paper analyzes the two-dimensional Ising CFT deformed by the thermal operator on de Sitter space, exploiting fermionization to map the theory to a free massive Majorana fermion. The authors compute the renormalized sphere partition function, the exact two-point function of the energy operator and of descendant-like operators, and their analytic continuation to Lorentzian dS2. They compare the exact results with conformal perturbation theory, showing that secular late-time logarithms appear in perturbation theory and are resummed into oscillatory behavior in the exact correlators. For the spin and disorder operators, which are non-local in the fermionic variables, the paper imports a differential-equation system from the literature to derive a nonperturbative constraint on their late-time scaling dimensions and compares with one-loop CPT. The abstract and introduction frame the model as a solvable laboratory for late-time de Sitter dynamics and for understanding the breakdown of perturbation theory.
Significance. If the spin/disorder claims are fully established, the paper would be a valuable addition to the short list of exactly solvable interacting QFTs in de Sitter space. The exact Majorana-frame computations are presented in detail and are internally consistent: the two-loop matching of the sphere partition function, including the ζ(3) coefficient, is a strong check of the duality map τ=m/(2π). The exact energy two-point function is explicit and the demonstration that secular logs are resummed into principal-series oscillations is a concrete and instructive example of the failure of CPT at late times. The paper does not provide code, but the analytic derivations are largely self-contained and reproducible from the formulas given.
major comments (4)
- [Section 6, Eq. (6.7)] The pure power-law ansatz Gσ~A u^{-Δ̃σ}, Gμ~B u^{-Δ̃μ} is inserted into (6.3)-(6.5), but only the leading u^{-Δ̃σ-Δ̃μ} terms are matched to obtain (6.8). Subleading terms of order u^{-Δ̃σ-Δ̃μ-1} in (6.5) are not cancelled by the ansatz. Thus (6.8) is only a leading-order asymptotic condition, not a proven nonperturbative constraint on the scaling dimensions. If the true solution has logarithmic or oscillatory corrections (cf. the ν log u term in (6.16)), the exponents extracted from a pure power fit may be biased. The authors should provide an asymptotic analysis of the ODE system or state the result more modestly.
- [Section 6, Eqs. (6.3)-(6.5)] The ODE system is imported from [54] and derived on the Euclidean sphere, where u∈[0,2]. The paper integrates these equations to u>2 and uses the large-u behavior to define Δ̃σ and Δ̃μ. This assumes that the Lorentzian analytic continuation of the correlators satisfies the same differential equations. No justification for this continuation of the Ward identities is given. The authors should either prove the continuation or support it with an independent late-time calculation.
- [Section 6, Figs. 3-5] The numerical extraction of Δ̃σ and Δ̃μ is not reproducible: no code, no error bars, no stated u-range for the fits, and no comparison with a log-amended fit. Given the explicit ν log u at O(ν) in (6.16), log corrections at O(ν^2) are plausible and could shift the fitted exponents. Without these details, the comparison with (6.18) in Fig. 5 is not convincing. This is load-bearing for the individual exponent predictions, though less for (6.8) itself.
- [Section 5.1, Eq. (5.28)] The descendant operator is defined as ε_T = (1 - T∂_T)ε. From (5.21), at late times T∂_T = -2 X∂_X, so 1 - T∂_T = 1 + 2X∂_X. This does not remove the leading X^{-1} tail; the operator that implements D_X = 1 + X∂_X is 1 - (1/2)T∂_T. Consequently Eqs. (5.29) and (5.50) are not the correlators of the operator defined in (5.28). Please correct the definition or the formulas.
minor comments (4)
- [General] Numerous rendering typos 'η/∫hortrightarrow0' appear in §§1,2,5,6 and should read 'η→0'; similar arrow symbols are corrupted in a few other places.
- [Figs. 3, 4] Axis labels are missing; please add them and specify the fitting interval and the fitting function used to extract the late-time exponents.
- [Eq. (6.16)] The large-u expansion of the elliptic integral K(1-u/2) is used to derive (6.16); it would be helpful to state the expansion explicitly or cite a reference.
- [References] Reference [33] is dated 2026 and appears to be a preprint; please verify the bibliographic details.
Circularity Check
No significant circularity: the exact energy sector is self-contained, and the spin/disorder constraints follow from an external ODE system plus an explicit ansatz, not from the results being derived.
full rationale
The derivation chain is not circular. The exact partition function and energy two-point function are computed in the free Majorana frame by Pfaffian integration and Wick contractions (eqs. (4.13), (5.7)); the map tau=m/(2 pi) is fixed by matching the O(nu^2) partition function and then independently checked at O(nu^4) and in the O(nu^2) epsilon-epsilon correlator. The late-time epsilon-epsilon behavior (5.25) and descendant oscillations (5.29) follow from standard hypergeometric asymptotics of the exact result, not from the CPT input. The spin/disorder section imports the Doyon–Fonseca ODE system (6.3)–(6.5) from an external paper [54], states the pure power-law ansatz (6.7) explicitly, substitutes it to obtain the constraint (6.8), and determines the exponents from the O(nu) ODE solution together with the independently derived antipodal ratio (6.9). This is a legitimate use of an external theorem and an explicit asymptotic ansatz; the constraint is a consequence of the ODE, not an input. The only self-citations ([30], [114]) appear in the outlook and are not load-bearing. Concerns about the validity of the pure-power ansatz or the accuracy of numerical exponent extraction are correctness/rigor issues, not circularity: no equation is used to predict itself, and no fitted parameter is renamed as a prediction.
Axiom & Free-Parameter Ledger
free parameters (2)
- ν = mℓ = 2πτℓ =
varied; report includes ν = 1/5 and range up to 0.14 in numerical extraction
- α =
finite scheme-dependent constant
axioms (4)
- domain assumption Fermionization: thermal Ising CFT + τ∫ε = free massive Majorana fermion; on S^2 the Z2 gauging is trivial and maps partition functions and correlators of ε to the Majorana frame.
- domain assumption Doyon–Fonseca differential equations (6.3)–(6.5) for the spin/disorder two-point functions on the sphere, derived in [54] via special Ward identities.
- standard math Analytic continuation from Euclidean sphere to Lorentzian dS2 via u → u_L gives Bunch–Davies correlators; the late-time limit is X → ∞.
- standard math Dirac spectrum on S^2: eigenvalues ± i n/ℓ with degeneracy 2n per sign (Camporesi–Higuchi).
invented entities (1)
-
ε_T descendant-like operator
independent evidence
read the original abstract
We study the two-dimensional Ising model deformed by the relevant thermal operator and placed on de Sitter (dS) spacetime. Despite being strongly interacting in its original formulation, the theory is exactly solvable on account of fermionisation. We compute exact cosmological correlators and compare them with conformal perturbation theory. In the Euclidean formulation of the model, we first compute the renormalised sphere partition function and the exact two-point functions of the thermal operator and descendant-like operators. We analytically continue the two-point functions to Lorentzian dS$_2$. Their late-time behaviour is governed by de Sitter representation theory and includes oscillations associated with principal-series scaling dimensions. We then analyse two-point functions of the spin and disorder operators, which are non-local in the fermionic variables, and derive non-perturbative constraints on their late-time scaling dimensions. In both cases, we compare the exact answers to conformal perturbation theory (CPT) and we show that divergent secular terms generically spoil the perturbative series at late times. The de Sitter Ising model shows explicitly how late-time perturbative pathologies are resummed in non-perturbative cosmological observables and provides a minimal solvable laboratory for quantum field theory dynamics in de Sitter space.
Figures
Forward citations
Cited by 1 Pith paper
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A discrete series gauge field at the late-time boundary of $dS_4$
Both Δ=1 and Δ=2 late-time Maxwell operators on planar dS4 furnish the photon unitary discrete series of SO(4,1), which splits into opposite-helicity summands via self-dual field-strength sectors.
Reference graph
Works this paper leans on
-
[1]
A. A. Starobinsky.A New Type of Isotropic Cosmological Models Without Singu- larity, Phys. Lett. B 91 (1980), 99–102
1980
-
[2]
A. H. Guth.The Inflationary Universe: A Possible Solution to the Horizon and Flatness Problems, Phys. Rev. D 23 (1981), 347–356
1981
-
[3]
A. D. Linde.A New Inflationary Universe Scenario: A Possible Solution of the Horizon, Flatness, Homogeneity, Isotropy and Primordial Monopole Problems, Phys. Lett. B 108 (1982), 389–393
1982
-
[4]
AlbrechtandP
A. AlbrechtandP. J. Steinhardt.Cosmology for Grand Unified Theories with Radiatively Induced Symmetry Breaking, Phys. Rev. Lett. 48 (1982), 1220–1223
1982
-
[5]
Planck Collaboration.Planck 2018 Results. VI. Cosmological Parameters, Astronomy & Astrophysics 641 (2020), A6
2018
-
[6]
Suzuki,D
N. Suzuki,D. Rubin,C. Lidman,G. Aldering,R. Amanullah,K. Barbary, et al.The Hubble Space Telescope Cluster Supernova Survey. V. Improving the Dark- Energy Constraints Above z > 1and Building an Early-Type-Hosted Supernova Sample, The Astrophysical Journal 746 (2012), 85
2012
-
[7]
https://www
Sloan Digital Sky Survey.Sloan Digital Sky Survey (SDSS). https://www. sdss.org. (2024)
2024
-
[8]
Anninos.De Sitter Musings, Int
D. Anninos.De Sitter Musings, Int. J. Mod. Phys. A 27 (2012), 1230013. arXiv: 1205.3855 [hep-th]
Pith/arXiv arXiv 2012
-
[9]
Witten.Quantum gravity in de Sitter space.Strings 2001: International Con- ference
E. Witten.Quantum gravity in de Sitter space.Strings 2001: International Con- ference. (2001). arXiv:hep-th/0106109
Pith/arXiv arXiv 2001
-
[10]
Nachtmann.Quantum theory in de-Sitter space, Commun
O. Nachtmann.Quantum theory in de-Sitter space, Commun. Math. Phys. 6.1 (1967), 1–16
1967
-
[11]
N. A. ChernikovandE. A. Tagirov.Quantum theory of scalar field in de Sitter space-time, Ann. Inst. H. Poincare Phys. Theor. A 9.2 (1968), 109–141
1968
-
[12]
SchomblondandP
C. SchomblondandP. Spindel.Conditions d’unicit´ e pour le propagateur∆ 1(x,y ) du champ scalaire dans l’univers de de Sitter, fr. Annales de l’institut Henri Poincar´ e. Section A, Physique Th´ eorique 25.1 (1976), 67–78
1976
-
[13]
T. S. BunchandP. C. W. Davies.Quantum Field Theory in de Sitter Space: Renormalization by Point Splitting, Proc. Roy. Soc. Lond. A 360 (1978), 117–134. [14]E. Mottola.Particle Creation in de Sitter Space, Phys. Rev. D 31 (1985), 754. [15]B. Allen.Vacuum States in de Sitter Space, Phys. Rev. D 32 (1985), 3136
1978
-
[16]
Higuchi.Symmetric Tensor Spherical Harmonics on the N Sphere and Their Application to the De Sitter Group SO( N,1), J
A. Higuchi.Symmetric Tensor Spherical Harmonics on the N Sphere and Their Application to the De Sitter Group SO( N,1), J. Math. Phys. 28 (1987). [Erratum: J. Math. Phys. 43, 6385 (2002)], 1553
1987
-
[17]
Higuchi.Linearized Gravity in de Sitter Space-Time as a Representation of SO(4,1), Class
A. Higuchi.Linearized Gravity in de Sitter Space-Time as a Representation of SO(4,1), Class. Quant. Grav. 8 (1991), 2005–2021
1991
-
[18]
Higuchi.Quantum Linearization Instabilities of de Sitter Space-Time
A. Higuchi.Quantum Linearization Instabilities of de Sitter Space-Time. 1, Class. Quant. Grav. 8 (1991), 1961–1981
1991
-
[19]
Higuchi.Quantum Linearization Instabilities of de Sitter Space-Time
A. Higuchi.Quantum Linearization Instabilities of de Sitter Space-Time. 2, Class. Quant. Grav. 8 (1991), 1983–2004
1991
-
[20]
D. Anninos,T. Anous,D. Z. Freedman, andG. Konstantinidis.Late-time Structure of the Bunch-Davies De Sitter Wavefunction, JCAP 11 (2015), 048. arXiv: 1406.5490 [hep-th]. 40
Pith/arXiv arXiv 2015
-
[21]
V. GorbenkoandL. Senatore. λφ4 in dS, (2019). arXiv: 1911.00022 [hep-th]
Pith/arXiv arXiv 2019
-
[22]
SleightandM
C. SleightandM. Taronna.From AdS to dS exchanges: Spectral representation, Mellin amplitudes, and crossing, Phys. Rev. D 104.8 (2021), L081902. arXiv: 2007. 09993 [hep-th]
2021
-
[23]
M. Hogervorst,J. Penedones, andK. S. Vaziri.Towards the non-perturbative cosmological bootstrap, JHEP 02 (2023), 162. arXiv:2107.13871 [hep-th]
Pith/arXiv arXiv 2023
-
[24]
D. Anninos,F. Denef,Y. T. A. Law, andZ. Sun.Quantum de Sitter hori- zon entropy from quasicanonical bulk, edge, sphere and topological string partition functions, JHEP 01 (2022), 088. arXiv:2009.12464 [hep-th]
Pith/arXiv arXiv 2022
-
[25]
L. Di Pietro,V. Gorbenko, andS. Komatsu.Analyticity and unitarity for cosmological correlators, JHEP 03 (2022), 023. arXiv:2108.01695 [hep-th]
arXiv 2022
-
[26]
V. A. Letsios.(Non-)unitarity of strictly and partially massless fermions on de Sitter space II: an explanation based on the group-theoretic properties of the spin-3/2 and spin-5/2 eigenmodes, J. Phys. A 57.13 (2024), 135401. arXiv: 2206 . 09851 [hep-th]
2024
-
[27]
V. A. Letsios.(Non-)unitarity of strictly and partially massless fermions on de Sitter space, JHEP 05 (2023), 015. arXiv:2303.00420 [hep-th]
arXiv 2023
-
[28]
J. Penedones,K. Salehi Vaziri, andZ. Sun.Hilbert space of quantum field theory in de Sitter spacetime, Phys. Rev. D 111.4 (2025), 045001. arXiv: 2301.04146 [hep-th]
Pith/arXiv arXiv 2025
-
[29]
M. Loparco,J. Penedones,K. Salehi Vaziri, andZ. Sun.The K¨ all´ en-Lehmann representation in de Sitter spacetime, JHEP 12 (2023), 159. arXiv: 2306.00090 [hep-th]
Pith/arXiv arXiv 2023
-
[30]
V. A. LetsiosandS. Vitouladitis.Axions on de Sitter space, (2026). arXiv: 2606.28858 [hep-th]
Pith/arXiv arXiv 2026
-
[31]
D. Anninos,T. Anous, andA. Rios Fukelman.De Sitter at all loops: the story of the Schwinger model, JHEP 08 (2024), 155. arXiv:2403.16166 [hep-th]. [32]C. Jayewardena.Schwinger model onS 2, Helv. Phys. Acta 61 (1988), 636–711
Pith/arXiv arXiv 2024
-
[33]
Smith.A Note on the Perturbative Expansion of the Schwinger Model on S2, (2026)
J. Smith.A Note on the Perturbative Expansion of the Schwinger Model on S2, (2026). arXiv:2603.21938 [hep-th]
arXiv 2026
-
[34]
J. Aguilera-Damia,D. Anninos,T. Anous,J. Gleeson, andA. Rios Fukel- man.de Sitter Vacua & pUniverses, (2026). arXiv:2605.02883 [hep-th]. [35]T. Anous,J. Gleeson,P. Paul, andA. Rios Fukelman, to appear
Pith/arXiv arXiv 2026
-
[36]
D. L´opez Nacir,F. D. Mazzitelli, andL. G. Trombetta. O(N)model in Euclidean de Sitter space: beyond the leading infrared approximation, JHEP 09 (2016), 117. arXiv:1606.03481 [hep-th]
Pith/arXiv arXiv 2016
-
[37]
L. Di Pietro,V. Gorbenko, andS. Komatsu.Cosmological Correlators at Finite Coupling, (2023). arXiv:2312.17195 [hep-th]
Pith/arXiv arXiv 2023
-
[38]
O. Diego,J. Gonzalez, andJ. Salas.The Ising model on spherical lattices: Dimer versus Monte Carlo approach, J. Phys. A 27 (1994), 2965–2983. arXiv: hep-lat/9307018
Pith/arXiv arXiv 1994
-
[39]
C. Hoelbling,A. Jakovac,J. Jersak,C. B. Lang, andT. Neuhaus.Spin and gauge systems on spherical lattices, Nucl. Phys. B Proc. Suppl. 47 (1996). Ed. byT. D. Kieu,B. H. J. McKellar, andA. J. Guttmann, 815–818. arXiv: hep-lat/9509009. 41
Pith/arXiv arXiv 1996
-
[40]
C. HolmandW. Janke.Ising spins on a gravitating sphere, Phys. Lett. B 375 (1996), 69–74. arXiv:hep-lat/9512002
Pith/arXiv arXiv 1996
-
[41]
C. HoelblingandC. B. Lang.Universality of the Ising model on sphere-like lattices, Phys. Rev. B 54 (1996), 3434. arXiv:hep-lat/9602025
Pith/arXiv arXiv 1996
-
[42]
R. C. BrowerandE. K. Owen.The Ising Model on S2, (2024). arXiv: 2407.00459 [hep-lat]
Pith/arXiv arXiv 2024
-
[43]
J. B. HartleandS. W. Hawking.Wave function of the Universe, Phys. Rev. D 28 12 (1983), 2960–2975
1983
-
[44]
Miller.Path integral games with de Sitter α-vacua, JHEP 10 (2025), 097
N. Miller.Path integral games with de Sitter α-vacua, JHEP 10 (2025), 097. arXiv: 2503.13701 [hep-th]
arXiv 2025
-
[45]
K. KirstenandJ. Garriga.Massless minimally coupled fields in de Sitter space: O(4) symmetric states versus de Sitter invariant vacuum, Phys. Rev. D 48 (1993), 567–577. arXiv:gr-qc/9305013
Pith/arXiv arXiv 1993
-
[46]
D. Baumann,D. Green,A. Joyce,E. Pajer,G. L. Pimentel,C. Sleight, andM. Taronna.Snowmass White Paper: The Cosmological Bootstrap, SciPost Phys. Comm. Rep. 2024 (2024), 1. arXiv:2203.08121 [hep-th]
Pith/arXiv arXiv 2024
-
[47]
L. H. Ford.Quantum instability of de Sitter spacetime, Phys. Rev. D 31 4 (1985), 710–717
1985
-
[48]
Antoniadis,J
I. Antoniadis,J. Iliopoulos, andT. N. Tomaras.Quantum Instability of de Sitter Space, Phys. Rev. Lett. 56 13 (1986), 1319–1322
1986
-
[49]
TsamisandR
N. TsamisandR. Woodard.Strong Infrared Effects in Quantum Gravity, Annals of Physics 238.1 (1995), 1–82
1995
-
[50]
L. SenatoreandM. Zaldarriaga.On Loops in Inflation, JHEP 12 (2010), 008. arXiv:0912.2734 [hep-th]
Pith/arXiv arXiv 2010
-
[51]
A. M. Polyakov.Infrared instability of the de Sitter space, (2012). arXiv: 1209. 4135 [hep-th]
2012
-
[52]
E. T. Akhmedov,U. Moschella, andF. K. Popov.Characters of different secular effects in various patches of de Sitter space, (2019). arXiv: 1901.07293 [hep-th]
Pith/arXiv arXiv 2019
-
[53]
D. GreenandA. Premkumar.Dynamical RG and Critical Phenomena in de Sitter Space, JHEP 04 (2020), 064. arXiv:2001.05974 [hep-th]
Pith/arXiv arXiv 2020
-
[54]
B. DoyonandP. Fonseca.Ising field theory on a Pseudosphere, J. Stat. Mech. 0407 (2004), P07002. arXiv:hep-th/0404136
Pith/arXiv arXiv 2004
-
[55]
M. Spradlin,A. Strominger, andA. Volovich.Les Houches lectures on de Sitter space.Les Houches Summer School: Session 76: Euro Summer School on Unity of Fundamental Physics: Gravity, Gauge Theory and Strings. (2001), 423–453. arXiv:hep-th/0110007
Pith/arXiv arXiv 2001
-
[56]
D. A. Galante.Modave lectures on de Sitter space & holography, PoS Modave2022 (2023), 003. arXiv:2306.10141 [hep-th]
Pith/arXiv arXiv 2023
-
[57]
Hirai.On irreducible representations of the Lorentz group of n-th order, Pro- ceedings of the Japan Academy 38.6 (1962), 258–262
T. Hirai.On irreducible representations of the Lorentz group of n-th order, Pro- ceedings of the Japan Academy 38.6 (1962), 258–262
1962
-
[58]
Ottoson.A Classification of the Unitary Irreducible Representations ofSO0(N, 1), Communications in Mathematical Physics 8.3 (1968), 228–244
U. Ottoson.A Classification of the Unitary Irreducible Representations ofSO0(N, 1), Communications in Mathematical Physics 8.3 (1968), 228–244
1968
-
[59]
Schwarz.Unitary irreducible representations of the groups SO(n, 1), Journal of Mathematical Physics 12.1 (1971), 131–139
F. Schwarz.Unitary irreducible representations of the groups SO(n, 1), Journal of Mathematical Physics 12.1 (1971), 131–139. 42
1971
-
[60]
T. Basile,X. Bekaert, andN. Boulanger.Mixed-symmetry fields in de Sitter space: a group theoretical glance, JHEP 05 (2017), 081. arXiv:1612.08166 [hep-th]
Pith/arXiv arXiv 2017
-
[61]
Sun.A note on the representations of SO(1,d + 1), Rev
Z. Sun.A note on the representations of SO(1,d + 1), Rev. Math. Phys. 37.01 (2025), 2430007. arXiv:2111.04591 [hep-th]
Pith/arXiv arXiv 2025
-
[62]
S ¸eng¨or.Particles of a de Sitter Universe, Universe 9.2 (2023), 59
G. S ¸eng¨or.Particles of a de Sitter Universe, Universe 9.2 (2023), 59. arXiv: 2212.10626 [hep-th]
Pith/arXiv arXiv 2023
-
[63]
M. Enayati,J.-P. Gazeau,H. Pejhan, andA. Wang.The de Sitter (dS) Group and its Representations. An Introduction to Elementary Systems and Modeling the Dark Energy Universe. Synthesis Lectures on Mathematics & Statistics. Springer (2023). arXiv:2201.11457 [math-ph]
Pith/arXiv arXiv 2023
-
[64]
Schaub.A Walk Through Spin(1,d + 1), (2024)
V. Schaub.A Walk Through Spin(1,d + 1), (2024). arXiv: 2405.01659 [hep-th]
Pith/arXiv arXiv 2024
-
[65]
Hinterbichler.De Sitter Representations, (2026)
K. Hinterbichler.De Sitter Representations, (2026). arXiv: 2606.26221 [hep-th]
Pith/arXiv arXiv 2026
-
[66]
Kitaev.Notes on ˜SL(2,R )representations, (2017)
A. Kitaev.Notes on ˜SL(2,R )representations, (2017). arXiv: 1711.08169 [hep-th]
Pith/arXiv arXiv 2017
-
[67]
A. Higuchi,D. Marolf, andI. A. Morrison.On the Equivalence between Euclidean and In-In Formalisms in de Sitter QFT, Phys. Rev. D 83 (2011), 084029. arXiv:1012.3415 [gr-qc]
Pith/arXiv arXiv 2011
-
[68]
AllenandT
B. AllenandT. Jacobson.Vector Two Point Functions in Maximally Symmetric Spaces, Commun. Math. Phys. 103 (1986), 669
1986
-
[69]
R. CamporesiandA. Higuchi.On the eigenfunctions of the Dirac operator on spheres and real hyperbolic spaces, J. Geom. Phys. 20 (1996), 1–18. arXiv: gr-qc/9505009
Pith/arXiv arXiv 1996
-
[70]
V. A. Letsios.The eigenmodes for spinor quantum field theory in global de Sitter space–time, J. Math. Phys. 62.3 (2021), 032303. arXiv:2011.07875 [gr-qc]
Pith/arXiv arXiv 2021
-
[71]
Schaub.Spinors in (Anti-)de Sitter Space
V. Schaub.Spinors in (Anti-)de Sitter Space. (2023). arXiv: 2302.08535 [hep-th]
Pith/arXiv arXiv 2023
-
[72]
Salehi Vaziri.A non-perturbative construction of the de Sitter late-time boundary, (2024)
K. Salehi Vaziri.A non-perturbative construction of the de Sitter late-time boundary, (2024). arXiv:2412.00183 [hep-th]
Pith/arXiv arXiv 2024
-
[73]
G. Seng¨orandC. Skordis.Unitarity at the Late time Boundary of de Sitter, JHEP 06 (2020), 041. arXiv:1912.09885 [hep-th]
Pith/arXiv arXiv 2020
-
[74]
T. Cohen,D. Green, andY. Huang.Operator origin of anomalous dimensions in de Sitter space, Phys. Rev. D 111.10 (2025), 103513. arXiv: 2407.08581 [hep-th]
Pith/arXiv arXiv 2025
-
[75]
Botshekananfard,E
M. Botshekananfard,E. B ¨us ¸ra G¨uraksın,V. A. Letsios, andG. S ¸eng¨or. A discrete series gauge field at the late-time boundary ofdS 4, to appear (2026)
2026
-
[76]
A. GuijosaandD. A. Lowe.A New twist on dS / CFT, Phys. Rev. D 69 (2004), 106008. arXiv:hep-th/0312282. [77]T. AnousandJ. Skulte.An invitation to the principal series, SciPost Phys. 9.3 (2020), 028
Pith/arXiv arXiv 2004
-
[78]
J. Frohlich,J. Fuchs,I. Runkel, andC. Schweigert.Kramers-Wannier duality from conformal defects, Phys. Rev. Lett. 93 (2004), 070601. arXiv: cond- mat/0404051
arXiv 2004
-
[79]
C.-M. Chang,Y. -H. Lin,S. -H. Shao,Y. Wang, andX. Yin.Topological Defect Lines and Renormalization Group Flows in Two Dimensions, JHEP 01 (2019), 026. arXiv:1802.04445 [hep-th]
Pith/arXiv arXiv 2019
-
[80]
A. Karch,D. Tong, andC. Turner.A Web of 2d Dualities:Z 2 Gauge Fields and Arf Invariants, SciPost Phys. 7 (2019), 007. arXiv:1902.05550 [hep-th]. 43
Pith/arXiv arXiv 2019
-
[81]
L. BhardwajandY. Tachikawa.On finite symmetries and their gauging in two dimensions, JHEP 03 (2018), 189. arXiv:1704.02330 [hep-th]
Pith/arXiv arXiv 2018
-
[82]
I. RunkelandG. M. T. Watts.Fermionic CFTs and classifying algebras, JHEP 06 (2020), 025. arXiv:2001.05055 [hep-th]
Pith/arXiv arXiv 2020
-
[83]
A. B. Zamolodchikov.Integrals of motion and S-matrix of the (scaled) T =Tc Ising model with magnetic field, Int. J. Mod. Phys. A 4 (1989), 4235–4248
1989
-
[84]
Delfino.Integrable field theory and critical phenomena: The Ising model in a magnetic field, J
G. Delfino.Integrable field theory and critical phenomena: The Ising model in a magnetic field, J. Phys. A 37 (2004), R45–R78. arXiv:hep-th/0312119 [hep-th]
Pith/arXiv arXiv 2004
-
[85]
F. Ambrosino,I. Runkel, andG. M. T. Watts.Translation invariant defects as an extension of topological symmetries, Int. J. Mod. Phys. A 41.07 (2026), 2648001. arXiv:2511.02007 [hep-th]
arXiv 2026
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