Recognition: 4 theorem links
· Lean TheoremGravitational electric-magnetic duality at the light ring and quasinormal mode isospectrality in effective field theories
Pith reviewed 2026-05-08 17:44 UTC · model grok-4.3
The pith
Gravitational electric-magnetic duality at the light ring enforces isospectrality of quasinormal modes even after certain higher-derivative corrections to general relativity.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
In general relativity, dynamical metric fluctuations on the plane-wave backgrounds that arise from the light-ring Penrose limit admit a gravitational analog of electric-magnetic duality. This duality interchanges the even- and odd-parity sectors and thereby forces their quasinormal spectra to coincide. When higher-derivative operators are added, the requirement that the same duality remain a symmetry of the linearized equations constrains the allowed couplings; the constrained theories are precisely those that preserve isospectrality in the eikonal limit. The authors conclude that light-ring duality is the organizing principle behind eikonal isospectrality and conjecture that the same holds,
What carries the argument
The gravitational electric-magnetic duality acting on metric fluctuations in the plane-wave spacetimes obtained from the light-ring Penrose limit.
If this is right
- Isospectrality survives in the eikonal limit precisely when the higher-derivative corrections are invariant under the light-ring duality.
- The allowed operators are linearly constrained; the surviving combinations automatically keep even- and odd-parity frequencies identical.
- The same organizing principle is conjectured to apply to any other duality-invariant correction beyond the class explicitly studied.
- The duality provides a direct diagnostic for whether a given effective-field-theory term will preserve or break isospectrality without solving the full perturbation equations.
Where Pith is reading between the lines
- The result offers a symmetry-based classification of which beyond-GR operators are safe for isospectrality, potentially simplifying model-building in modified gravity.
- One could test the conjecture by checking whether known duality-invariant terms in Einstein-scalar-Gauss-Bonnet or dynamical Chern-Simons gravity preserve the degeneracy in the eikonal limit.
- If the duality continues to protect isospectrality at higher orders, it may also constrain the form of non-perturbative corrections that could appear in string-inspired models.
Load-bearing premise
The plane-wave spacetimes extracted from the light-ring Penrose limit faithfully encode the essential dynamics of eikonal quasinormal modes, and the duality can be imposed on the higher-derivative operators without further restrictions that would invalidate the coupling constraints.
What would settle it
An explicit computation of eikonal quasinormal modes for a higher-derivative correction that preserves the light-ring duality yet produces non-degenerate even- and odd-parity spectra.
Figures
read the original abstract
Black hole perturbations are characterized by a superposition of damped exponentials known as quasinormal modes. In general relativity, the spectra of parity-even and parity-odd quasinormal modes coincide -- a property known as isospectrality, which is typically broken by corrections beyond general relativity. Recently, certain higher-derivative operators were shown to preserve isospectrality in the high-frequency (eikonal) regime. Motivated by the relation between the light ring Penrose limit and the eikonal limit, we study isospectrality in a class of plane-wave spacetimes. In general relativity, we show that dynamical metric fluctuations on these backgrounds admit a gravitational analog of electric-magnetic duality, which enforces isospectrality. Requiring this duality to persist in the presence of higher-derivative corrections constrains the couplings so that isospectrality is preserved. We conclude that gravitational electric-magnetic duality at the light ring is the organizing principle behind isospectrality in the eikonal limit, and we conjecture that this remains true for other duality-invariant corrections to general relativity.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper claims that gravitational electric-magnetic duality holds for dynamical metric fluctuations on plane-wave spacetimes obtained from the light-ring Penrose limit in general relativity, thereby enforcing isospectrality between parity-even and parity-odd quasinormal modes in the eikonal limit. Requiring the duality to persist under higher-derivative corrections then constrains the allowed EFT couplings so that isospectrality is preserved. The authors conclude that this duality at the light ring is the organizing principle for eikonal isospectrality and conjecture that the result extends to other duality-invariant corrections to GR.
Significance. If the central derivations hold, the work supplies a symmetry-based explanation for the preservation of eikonal isospectrality under selected higher-derivative operators, offering a practical criterion for constructing EFTs compatible with GR-like spectral properties. The use of the Penrose limit to isolate the relevant dynamics is a technically interesting link between local plane-wave geometry and global black-hole perturbation spectra.
major comments (2)
- [The discussion of the Penrose limit and its relation to the eikonal regime] The reduction step from the light-ring Penrose limit to eikonal QNM isospectrality assumes that local duality on the resulting plane-wave backgrounds captures all relevant dynamics without residual curvature or horizon contributions that could split the spectra. This assumption is load-bearing for the claim that duality enforces isospectrality in the original geometry, yet the manuscript provides no explicit matching or global consistency argument showing that the local plane-wave equations suffice.
- [The section deriving EFT constraints from persistence of duality] When extending the duality to higher-derivative operators, the paper imposes the duality condition directly on the plane-wave fluctuations to constrain couplings. It is not shown that this procedure is equivalent to imposing duality on the full linearized perturbation equations around the black-hole background; additional terms generated by the reduction could relax or invalidate the reported constraints on the EFT coefficients.
minor comments (2)
- Notation for the electric and magnetic parts of the Weyl tensor (or their plane-wave analogs) should be introduced with an explicit definition before being used in the duality transformation.
- The abstract states that certain operators 'preserve isospectrality' but does not list the specific operators or the dimension at which they appear; adding this information would improve readability.
Simulated Author's Rebuttal
We thank the referee for their careful reading of the manuscript and for the positive assessment of its significance. We address the two major comments point by point below, providing clarifications on the assumptions and indicating the revisions we will make to strengthen the presentation.
read point-by-point responses
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Referee: [The discussion of the Penrose limit and its relation to the eikonal regime] The reduction step from the light-ring Penrose limit to eikonal QNM isospectrality assumes that local duality on the resulting plane-wave backgrounds captures all relevant dynamics without residual curvature or horizon contributions that could split the spectra. This assumption is load-bearing for the claim that duality enforces isospectrality in the original geometry, yet the manuscript provides no explicit matching or global consistency argument showing that the local plane-wave equations suffice.
Authors: We agree that an explicit discussion of this connection would strengthen the manuscript. The Penrose limit is a standard tool to extract the eikonal limit of quasinormal modes, as it focuses on the high-frequency, short-wavelength regime near the unstable photon orbit (light ring). In this limit, the wave equations reduce to those on a plane-wave spacetime, and the duality symmetry we identify acts on these reduced equations to enforce the degeneracy between even and odd modes. Residual curvature effects from the global geometry are subleading in the eikonal expansion and do not affect the leading-order isospectrality. To address the referee's concern, we will add a dedicated paragraph in the introduction or a new subsection in Section 2 explaining this reduction and citing relevant literature on the validity of the Penrose limit for eikonal QNMs. This will include a brief argument why horizon contributions are irrelevant in the eikonal limit. We believe this clarification will resolve the issue without requiring major changes to the derivations. revision: partial
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Referee: [The section deriving EFT constraints from persistence of duality] When extending the duality to higher-derivative operators, the paper imposes the duality condition directly on the plane-wave fluctuations to constrain couplings. It is not shown that this procedure is equivalent to imposing duality on the full linearized perturbation equations around the black-hole background; additional terms generated by the reduction could relax or invalidate the reported constraints on the EFT coefficients.
Authors: This is a valid point regarding the order of limits and reductions. Our approach is motivated by the fact that the eikonal limit corresponds precisely to the dynamics on the Penrose-limit plane waves, so requiring duality invariance there directly ensures that the higher-derivative terms do not break isospectrality at leading eikonal order. Since the higher-derivative operators are local, their contribution in the reduced geometry captures the leading effect. However, we concede that a rigorous demonstration that no additional terms arise from commuting the duality condition with the Penrose limit would be desirable. We will revise the relevant section (likely Section 4) to include a discussion of this point, arguing that because the Penrose limit is a local coordinate transformation near the light ring, and the EFT corrections are diffeomorphism-invariant, the constraints remain valid for the eikonal spectra. We will also note that this is consistent with numerical checks in the literature for specific EFTs. If further verification is needed, we can consider expanding the full equations in future work, but for the current scope, this provides the organizing principle as claimed. revision: partial
Circularity Check
No circularity: derivation derives duality explicitly in GR then applies it to constrain EFT terms
full rationale
The paper first constructs gravitational electric-magnetic duality on the plane-wave backgrounds obtained from the light-ring Penrose limit within general relativity and shows that this duality enforces isospectrality of the metric fluctuations. It then requires the same duality to hold after adding higher-derivative operators, thereby obtaining constraints on the EFT couplings that preserve isospectrality. This chain does not reduce any claimed prediction to a fitted input by construction, does not rely on self-citations for its central steps, and does not smuggle an ansatz or rename a known result. The Penrose-limit assumption is an explicit modeling choice whose validity is independent of the duality derivation itself. No load-bearing step collapses to a tautology or to prior work by the same authors.
Axiom & Free-Parameter Ledger
axioms (2)
- domain assumption General relativity governs the background geometry and linear perturbations on the plane-wave spacetimes
- domain assumption Higher-derivative operators appear in the effective field theory expansion around GR
Lean theorems connected to this paper
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Cost / FunctionalEquation (J(x)=½(x+x⁻¹)−1)washburn_uniqueness_aczel unclear?
unclearRelation between the paper passage and the cited Recognition theorem.
we show that dynamical metric fluctuations on these backgrounds admit a gravitational analog of electric-magnetic duality, which enforces isospectrality
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Foundation/BranchSelection (RCL bilinear vs additive branch)branch_selection unclear?
unclearRelation between the paper passage and the cited Recognition theorem.
Ψ_H ↦ e^{±iθ} Ψ_H ... ˙C^{±}_{abcd} ↦ e^{±iθ} ˙C^{±}_{abcd}
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Foundation/DimensionForcing / 8-tick period(no parallel; 'eight-derivative' here is curvature order, unrelated to RS 8-tick clock) unclear?
unclearRelation between the paper passage and the cited Recognition theorem.
Up to eight-derivative corrections, the most general EFT extension of GR ... ε₁ = ε₂ ≡ ε
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Constants (c=1, ℏ, G as φ-powers)RealityCertificate unclear?
unclearRelation between the paper passage and the cited Recognition theorem.
the Penrose limit ... yields the pp-wave ds² = -A_{ij}(u) x^i x^j du² + 2 du dv - dx² - dy²
What do these tags mean?
- matches
- The paper's claim is directly supported by a theorem in the formal canon.
- supports
- The theorem supports part of the paper's argument, but the paper may add assumptions or extra steps.
- extends
- The paper goes beyond the formal theorem; the theorem is a base layer rather than the whole result.
- uses
- The paper appears to rely on the theorem as machinery.
- contradicts
- The paper's claim conflicts with a theorem or certificate in the canon.
- unclear
- Pith found a possible connection, but the passage is too broad, indirect, or ambiguous to say the theorem truly supports the claim.
Reference graph
Works this paper leans on
-
[1]
Black hole spectroscopy: from theory to experiment
E. Berti, V. Cardoso, G. Carullo,et al., Black hole spectroscopy: from theory to experiment, (2025), arXiv:2505.23895 [gr-qc]
work page internal anchor Pith review arXiv 2025
-
[2]
C. V. Vishveshwara, Scattering of Gravitational Radiation by a Schwarzschild Black-hole, Nature227, 936 (1970)
1970
-
[3]
W. H. Press, Long Wave Trains of Gravitational Waves from a Vibrating Black Hole, Astrophys. J. Lett.170, L105 (1971)
1971
-
[4]
S. A. Teukolsky, Perturbations of a rotating black hole. 1. Fundamental equations for gravitational electromagnetic and neutrino field perturbations, Astrophys. J.185, 635 (1973)
1973
-
[5]
Chandrasekhar and S
S. Chandrasekhar and S. L. Detweiler, The quasi-normal modes of the Schwarzschild black hole, Proc. Roy. Soc. Lond. A344, 441 (1975)
1975
-
[6]
K. D. Kokkotas and B. G. Schmidt, Quasinormal modes of stars and black holes, Living Rev. Rel.2, 2 (1999), arXiv:gr-qc/9909058
work page internal anchor Pith review arXiv 1999
-
[7]
Quasinormal modes of black holes and black branes
E. Berti, V. Cardoso, and A. O. Starinets, Quasinormal modes of black holes and black branes, Class. Quant. Grav. 26, 163001 (2009), arXiv:0905.2975 [gr-qc]
work page internal anchor Pith review arXiv 2009
- [8]
-
[9]
On gravitational-wave spectroscopy of massive black holes with the space interferometer LISA
E. Berti, V. Cardoso, and C. M. Will, On gravitational- wave spectroscopy of massive black holes with the space interferometer LISA, Phys. Rev. D73, 064030 (2006), arXiv:gr-qc/0512160
work page Pith review arXiv 2006
-
[10]
Bayesian model selection for testing the no-hair theorem with black hole ringdowns
S. Gossan, J. Veitch, and B. S. Sathyaprakash, Bayesian model selection for testing the no-hair theorem with black hole ringdowns, Phys. Rev. D85, 124056 (2012), arXiv:1111.5819 [gr-qc]
work page Pith review arXiv 2012
-
[11]
Testing General Relativity with Present and Future Astrophysical Observations
E. Bertiet al., Testing General Relativity with Present and Future Astrophysical Observations, Class. Quant. Grav.32, 243001 (2015), arXiv:1501.07274 [gr-qc]
work page internal anchor Pith review arXiv 2015
- [12]
-
[13]
N. Franchini and S. H. Völkel, Testing General Rel- ativity with Black Hole Quasi-normal Modes (2024) arXiv:2305.01696 [gr-qc]
- [14]
- [15]
-
[16]
Regge and J
T. Regge and J. A. Wheeler, Stability of a Schwarzschild singularity, Phys. Rev.108, 1063 (1957)
1957
-
[17]
F. J. Zerilli, Effective potential for even parity Regge- Wheeler gravitational perturbation equations, Phys. Rev. Lett.24, 737 (1970)
1970
-
[18]
Chandrasekhar, On the equations governing the pertur- bations of the Schwarzschild black hole, Proc
S. Chandrasekhar, On the equations governing the pertur- bations of the Schwarzschild black hole, Proc. Roy. Soc. Lond. A343, 289 (1975)
1975
-
[19]
R. Kallosh, J. Rahmfeld, and W. K. Wong, One loop supergravity corrections to the black hole entropy and residual supersymmetry, Phys. Rev. D57, 1063 (1998), arXiv:hep-th/9706048
-
[20]
K. Glampedakis, A. D. Johnson, and D. Kennefick, Dar- boux transformation in black hole perturbation theory, Phys. Rev. D96, 024036 (2017), arXiv:1702.06459 [gr-qc]
-
[21]
M. Lenzi and C. F. Sopuerta, Darboux covariance: A hidden symmetry of perturbed Schwarzschild black holes, Phys. Rev. D104, 124068 (2021), arXiv:2109.00503 [gr- qc]
-
[22]
M. Lenzi and C. F. Sopuerta, Master functions and equations for perturbations of vacuum spherically sym- metric spacetimes, Phys. Rev. D104, 084053 (2021), arXiv:2108.08668 [gr-qc]
-
[23]
M. Lenzi and C. F. Sopuerta, Black hole greybody factors from Korteweg–de Vries integrals: Theory, Phys. Rev. D 107, 044010 (2023), arXiv:2212.03732 [gr-qc]
-
[24]
M. Lenzi and C. F. Sopuerta, Black hole greybody factors from Korteweg–de Vries integrals: Computation, Phys. 7 Rev. D107, 084039 (2023), arXiv:2301.01096 [gr-qc]
- [25]
-
[26]
D. A. Nichols, A. Zimmerman, Y. Chen, G. Lovelace, K. D. Matthews, R. Owen, F. Zhang, and K. S. Thorne, Visualizing Spacetime Curvature via Frame-Drag Vor- texes and Tidal Tendexes III. Quasinormal Pulsations of Schwarzschild and Kerr Black Holes, Phys. Rev. D86, 104028 (2012), arXiv:1208.3038 [gr-qc]
- [27]
- [28]
-
[29]
V. Cardoso, M. Kimura, A. Maselli, E. Berti, C. F. B. Macedo, and R. McManus, Parametrized black hole quasinormal ringdown: Decoupled equations for non- rotating black holes, Phys. Rev. D99, 104077 (2019), arXiv:1901.01265 [gr-qc]
-
[30]
R. McManus, E. Berti, C. F. B. Macedo, M. Kimura, A. Maselli, and V. Cardoso, Parametrized black hole quasi- normal ringdown. II. Coupled equations and quadratic corrections for nonrotating black holes, Phys. Rev. D100, 044061 (2019), arXiv:1906.05155 [gr-qc]
- [31]
- [32]
- [33]
- [34]
-
[35]
H. O. Silva, G. Tambalo, K. Glampedakis, and K. Yagi, Quasinormal modes and their excitation beyond general relativity. II. Isospectrality loss in gravitational waveforms, Phys. Rev. D113, 084012 (2026), arXiv:2601.13411 [gr- qc]
work page internal anchor Pith review Pith/arXiv arXiv 2026
- [36]
- [37]
-
[38]
M. K. Gaillard and B. Zumino, Duality Rotations for Interacting Fields, Nucl. Phys. B193, 221 (1981)
1981
-
[39]
G. W. Gibbons and D. A. Rasheed, Electric - magnetic duality rotations in nonlinear electrodynamics, Nucl. Phys. B454, 185 (1995), arXiv:hep-th/9506035
work page Pith review arXiv 1995
-
[40]
Duality in Gauge Theory, Gravity and String Theory,
U. Kol and S.-T. Yau, Duality in Gauge Theory, Gravity and String Theory, (2023), arXiv:2311.07934 [hep-th]
-
[41]
Penrose, A Spinor approach to general relativity, An- nals Phys.10, 171 (1960)
R. Penrose, A Spinor approach to general relativity, An- nals Phys.10, 171 (1960)
1960
- [42]
- [43]
-
[44]
Duality in linearized gravity,
M. Henneaux and C. Teitelboim, Duality in linearized gravity, Phys. Rev. D71, 024018 (2005), arXiv:gr- qc/0408101
-
[45]
Free spin 2 duality invariance cannot be extended to GR,
S. Deser and D. Seminara, Free spin 2 duality invariance cannot be extended to GR, Phys. Rev. D71, 081502 (2005), arXiv:hep-th/0503030
- [46]
-
[47]
Gravitational duality and rotating solutions,
R. Argurio and F. Dehouck, Gravitational duality and rotating solutions, Phys. Rev. D81, 064010 (2010), arXiv:0909.0542 [hep-th]
-
[48]
Manifest spin 2 dual- ity with electric and magnetic sources,
G. Barnich and C. Troessaert, Manifest spin 2 dual- ity with electric and magnetic sources, JHEP01, 030, arXiv:0812.0552 [hep-th]
-
[49]
Nonlocality and gravitoelectro- magnetic duality,
J. Boos and I. Kolář, Nonlocality and gravitoelectro- magnetic duality, Phys. Rev. D104, 024018 (2021), arXiv:2103.10555 [gr-qc]
-
[50]
No U(1) ‘electric-magnetic’ duality in Ein- stein gravity,
R. Monteiro, No U(1) ‘electric-magnetic’ duality in Ein- stein gravity, JHEP04, 093, arXiv:2312.02351 [hep-th]
-
[51]
A. del Rio, J. Olmedo, and A. Torres Manso, Dual- ity symmetry and anomaly for gravitational waves in curved spacetimes, Phys. Rev. D112, 085023 (2025), arXiv:2507.22588 [gr-qc]
-
[52]
vibrations
C. J. Goebel, Comments on the “vibrations” of a Black Hole., Astrophys. J. Lett.172, L95 (1972)
1972
-
[53]
Ferrari and B
V. Ferrari and B. Mashhoon, New approach to the quasi- normal modes of a black hole, Phys. Rev. D30, 295 (1984)
1984
-
[54]
Mashhoon, Stability of charged rotating black holes in the eikonal approximation, Phys
B. Mashhoon, Stability of charged rotating black holes in the eikonal approximation, Phys. Rev. D31, 290 (1985)
1985
-
[55]
E. Berti and K. D. Kokkotas, Quasinormal modes of Kerr-Newman black holes: Coupling of electromagnetic and gravitational perturbations, Phys. Rev. D71, 124008 (2005), arXiv:gr-qc/0502065
-
[56]
Geodesic stability, Lyapunov exponents and quasinormal modes
V. Cardoso, A. S. Miranda, E. Berti, H. Witek, and V. T. Zanchin, Geodesic stability, Lyapunov exponents and quasinormal modes, Phys. Rev. D79, 064016 (2009), arXiv:0812.1806 [hep-th]
work page Pith review arXiv 2009
- [57]
-
[58]
Penrose, Any space-time has a plane wave as a limit, inDifferential Geometry and Relativity: A Volume in Honour of André Lichnerowicz on His 60th Birthday, edited by M
R. Penrose, Any space-time has a plane wave as a limit, inDifferential Geometry and Relativity: A Volume in Honour of André Lichnerowicz on His 60th Birthday, edited by M. Cahen and M. Flato (Springer Netherlands, Dordrecht, 1976) pp. 271–275
1976
-
[59]
Fransen, Quasinormal modes from Penrose limits, Class
K. Fransen, Quasinormal modes from Penrose limits, Class. Quant. Grav.40, 205004 (2023), arXiv:2301.06999 [gr-qc]
-
[60]
D. Kapec and A. Sheta, pp-waves and the hidden sym- metries of black hole quasinormal modes, Class. Quant. Grav.42, 155002 (2025), arXiv:2412.08551 [hep-th]
-
[61]
K. Fransen, D. Pereñiguez, and J. Redondo-Yuste, Pertur- bations of plane waves and quadratic quasinormal modes on the lightring, JHEP12, 148, arXiv:2509.03598 [gr-qc]
-
[62]
H. W. Brinkmann, Einstein spaces which are mapped conformally on each other, Math. Ann.94, 119 (1925)
1925
-
[63]
A. Kehagias, D. Perrone, and A. Riotto, Non-linear Quasi- 8 Normal Modes of the Schwarzschild Black Hole from the Penrose Limit, (2025), arXiv:2503.09350 [gr-qc]
-
[64]
D. Perrone, A. Kehagias, and A. Riotto, Nonlinearities in Kerr black hole ringdown from the Penrose limit, JCAP 10, 024, arXiv:2507.01919 [gr-qc]
-
[65]
R. P. Geroch, A. Held, and R. Penrose, A space-time calculus based on pairs of null directions, J. Math. Phys. 14, 874 (1973)
1973
-
[66]
J. M. Stewart and M. Walker, Perturbations of spacetimes in general relativity, Proc. Roy. Soc. Lond. A341, 49 (1974)
1974
- [67]
-
[68]
S. Aksteiner and L. Andersson, Linearized gravity and gauge conditions, Class. Quant. Grav.28, 065001 (2011), arXiv:1009.5647 [gr-qc]
-
[69]
S. Aksteiner, L. Andersson, and T. Bäckdahl, New iden- tities for linearized gravity on the Kerr spacetime, Phys. Rev. D99, 044043 (2019), arXiv:1601.06084 [gr-qc]
-
[70]
M. G. Calkin, An Invariance Property of the Free Elec- tromagnetic Field, American Journal of Physics33, 958 (1965)
1965
- [71]
-
[72]
J. H. Schwarz, An SL(2,Z) multiplet of type IIB su- perstrings, Phys. Lett. B360, 13 (1995), [Erratum: Phys.Lett.B 364, 252 (1995)], arXiv:hep-th/9508143
work page Pith review arXiv 1995
-
[73]
R. M. Wald, Construction of Solutions of Gravitational, Electromagnetic, Or Other Perturbation Equations from Solutions of Decoupled Equations, Phys. Rev. Lett.41, 203 (1978)
1978
-
[74]
L. S. Kegeles and J. M. Cohen, Constructive procedure for perturbations of spacetimes, Phys. Rev. D19, 1641 (1979)
1979
- [75]
-
[76]
Infinite-dimensional symmetries in plane wave spacetimes
E. Despontin, S. Detournay, and D. Fontaine, Infinite- dimensional symmetries in plane wave spacetimes 10.1103/2q94-5crl (2025), arXiv:2508.12760 [hep-th]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/2q94-5crl 2025
- [77]
-
[78]
An effective formalism for testing extensions to General Relativity with gravitational waves
S. Endlich, V. Gorbenko, J. Huang, and L. Senatore, An effective formalism for testing extensions to Gen- eral Relativity with gravitational waves, JHEP09, 122, arXiv:1704.01590 [gr-qc]
- [79]
-
[80]
A. Gruzinov and M. Kleban, Causality Constrains Higher Curvature Corrections to Gravity, Class. Quant. Grav. 24, 3521 (2007), arXiv:hep-th/0612015
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