REVIEW 2 major objections 4 minor 3 cited by
The Speed of Gravity
T0 review · 2 major / 4 minor · reviewed 2026-08-14 · deepseek-v4-flash
Pith's one-line read Gravitational waves slightly outrun light on cosmological backgrounds, this paper argues.
desk verdict A carefully derived EFT calculation of gravitational wave speed corrections on FLRW whose superluminality headline is honestly conditional on the unproven sign of C_W2; the finite dimension-6 part is the most durable piece. read the letter →
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
The reading
What carries the argument
The central object is the low-energy effective action for gravity organized in curvature operators, truncated at the Weyl-squared (dimension-4) and curvature-cubed (dimension-6) level. The speed is defined through the lightcone of the second-order hyperbolic equation obtained after perturbatively reducing the higher-derivative terms; it is the coefficient of $k^2$ in the tensor dispersion relation. At leading order the Weyl-squared coefficient $C_{W^2}$, the coupling of the conformal curvature-squared operator, carries the whole effect via $c_s^2 = 1 + 16 C_{W^2}(-\dot H)/M_{\rm Pl}^2$. Positivity bounds on matter amplitudes, together with the Källén–Lehmann spectral representation of the two-point function of the stress tensor, are the machinery that fixes $C_{W^2}>0$; the assumption of neglecting the massless graviton t-channel pole is what lets those bounds go through. At next order the finite one-loop coefficients for fields of spin 0, 1/2, and 1 supply the species-dependent terms that make the speed epoch-dependent.
What would settle it
In an explicit weakly coupled UV completion containing an infinite tower of massive spin-2 states, compute the full two-to-two amplitude without dropping the massless graviton t-channel pole; if the twice-subtracted forward amplitude does not force the Weyl-squared coefficient to be positive, the sign conclusion fails. A complementary observation would be a cosmological multi-messenger event whose gravitational-wave and photon arrival times imply a subluminal tensor speed in the matter frame.
Extended reading notes
Core claim
The paper's central claim is that in the effective field theory of gravity the sound speed of tensor modes on a spontaneously Lorentz-breaking background is modified by irrelevant curvature operators, and for the signs selected by positivity bounds the modification is generically superluminal. On FLRW spacetime the Weyl-squared interaction gives $c_s^2 = 1 + 16 C_{W^2}(-\dot H)/M_{\rm Pl}^2$; since ordinary matter obeys the null energy condition and hence $\dot H<0$, a positive $C_{W^2}$ makes gravitational waves outpace the lightcone of the metric to which Standard Model fields are minimally coupled. A positive $C_{W^2}$ is what follows from Källén–Lehmann spectral positivity of the stress-tensor two-point function and from weakly coupled tree-level completions with massive spin-2 states, provided the massless graviton t-channel pole in the relevant amplitudes can be neglected. When the leading curvature-squared terms are set to zero, the finite one-loop dimension-6 effective action produces a speed shift of order $H^4/(M_{\rm Pl}^2 M^2)$ whose sign depends on the spin and mass of the lightest integrated-out particles: scalar-dominated content gives superluminal gravitational waves for most of standard cosmological history, while the radiation era is subluminal for all spins.
Load-bearing premise
The argument assumes that standard positivity bounds apply to matter scattering once the massless graviton t-channel pole is neglected, and that the Källén–Lehmann spectral integrals need at most one subtraction; if either premise fails, the sign of $C_{W^2}$ is unconstrained and the generic superluminality conclusion does not follow.
Editorial extensions
If this is right
- If the central claim survives, low-frequency gravitational waves on a cosmological background arrive slightly earlier than photons emitted from the same source, with the departure growing toward the infrared.
- No field redefinition can make both sectors luminal at low energies: the ratio of tensor to matter sound speeds is frame invariant, so a frame with luminal gravity leaves matter fluctuations subluminal through gravitationally induced $T\bar T$-type interactions.
- The front velocity is luminal in the high-frequency limit, so the low-energy superluminal group velocity does not imply propagation of information outside the lightcone.
- Setting the curvature-squared corrections to zero does not restore luminality; the finite dimension-6 loop corrections still shift the speed, and scalar-dominated heavy spectra make gravitational waves superluminal through most of standard cosmological history.
- Cosmological model builders should not impose subluminality of all fluctuations as a consistency criterion; the operative causality criterion becomes S-matrix analyticity, which for this system selects superluminal gravitational waves.
Reading between the lines
- One testable extension: the predicted speed shift is frequency-dependent and grows in the IR, so a multi-messenger gravitational-wave event at cosmological distance could in principle measure the sign of the effect and thereby test $C_{W^2}>0$ in the matter frame.
- If positivity bounds are invalidated by the t-channel pole, the leading-order sign is unknown, but the finite dimension-6 loop effect remains; the same measurement strategy could still extract the spin and mass content of the lightest states above the Hubble scale.
- The lightcone ordering implied by the paper (matter cone inside gravity cone) reverses for NEC-violating sources, so these sign arguments could sharpen consistency conditions on phantom dark energy or other negative-energy cosmological models.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper studies the low-energy speed of gravitational waves in the standard effective field theory of general relativity coupled to matter, on backgrounds that spontaneously break Lorentz invariance such as FLRW. The central technical result is Eq. (3.36): on NEC-preserving FLRW backgrounds, the tensor-mode sound speed is c_s^2 = 1 + 16 C_W2 (-\(\dot H\))/M_Pl^2 to leading order in the curvature-squared EFT, so the sign of the Weyl-squared coefficient C_W2 controls whether gravitational waves are superluminal. The paper argues that positivity bounds, applied to matter scattering amplitudes after a field redefinition, select C_W2 > 0 and hence superluminal gravitational waves. It also analyzes dimension-6 and dimension-8 curvature operators: after tuning the IR curvature-squared coefficients to zero, finite one-loop corrections from massive scalars, spinors, and vectors produce an epoch- and species-dependent modification of the speed, given in Eq. (5.10), with superluminal behavior for scalar-dominated contributions over most of standard cosmological history and subluminal behavior in the radiation era. The appendices reproduce the one-loop effective action for a massive scalar and provide the detailed FLRW reduction for dimension-6 operators.
Significance. If the sign assumption on C_W2 is eventually justified, the paper establishes a concrete, potentially observable consequence of a standard gravitational EFT: a tiny but nonzero difference between the gravitational-wave speed and the matter lightcone, scaling as |\(\dot H\)|/\Lambda^2. The derivation of the speed formula is careful, the field-frame invariance argument (Section 2.2) is a useful clarification, and the explicit one-loop coefficients from Avramidi are reproduced rather than fitted. The dimension-6 result is especially valuable because it is finite, calculable, and predicts a sign that depends on the spin of the lightest integrated-out field, including the interesting statement that radiation-era gravitational waves are subluminal for all three spin species considered. The paper is also honest in its main bullet by including the qualifier that the t-channel-pole contribution is ignored; the problem is that this qualifier is not consistently carried through the abstract and discussion.
major comments (2)
- [§4.2, §4.3.3; Eq. (3.36)] The paper's headline claim that positivity bounds 'enforce' superluminal gravitational waves is not established, because the sign of C_W2 is never proven. The speed formula (3.36) gives c_s^2 = 1 + 16 C_W2(-\dot H)/M_Pl^2, so on NEC backgrounds (\dot H < 0) the conclusion c_s^2 > 1 requires C_W2 > 0. The arguments for C_W2 > 0 are explicitly conditional: Section 4.2 applies positivity bounds only 'provided we argue or assume that the contribution of the graviton exchange t-channel pole can be neglected', and Section 4.3.3 states that if the Kallen-Lehmann integrals in (4.37) require subtractions, 'it is hence not possible to conclude positivity of the LHS'. No proof of convergence of (4.37), and no independent justification of the t-channel-pole prescription beyond citation to [27], is supplied. The valid conclusion is therefore a conditional theorem, not the generic statement in the abstract and Section 6 that the speed is 'in general superluminal'. The abstract, introduction, and discussion should be revised so that the logical dependence on the unproven t-channel/subtraction assumption is explicit in every statement of the main result.
- [§5.1.4; Eq. (5.11)] The phenomenological discussion of scalar dark matter in Section 5.1.4 applies the dimension-6 result to 'the whole standard cosmological history', but this application is only valid on the tuned subspace C_IR^{W2} = C_IR^{R2} = 0 introduced at the start of Section 5. If positivity bounds do select C_W2 > 0, the dimension-4 contribution generically dominates the dimension-6 one, and the epoch-dependent conclusions, including the subluminal radiation-era statement, would not hold. The paper partially acknowledges this in the 'Discriminator Redux' paragraph, but the abstract's claim that finite loop corrections 'lead to an epoch dependent modification' should be framed as a statement about a deliberately tuned EFT, not about the generic EFT. The section would benefit from a clear summary stating which conclusions are generic and which require the tuning.
minor comments (4)
- [§4.3.5; Eq. (4.46)] Equation (4.46) contains an apparent typo: the inequality '|1-c_s^2(M_2)| < |1-c_s^2(M_2)|' for M_2 > M_1 is trivially false; the right-hand side should presumably refer to M_1. The surrounding text makes the intended RG monotonicity clear.
- [Fig. 3] The axes of Figure 3 are not fully labeled; the approximate numerical boundaries (-1.8, 0.2, 1.2, -1.5) are given only in the caption. Adding explicit axis labels and marking the NEC boundary \omega = -1 directly on the figure would improve readability.
- [§5.1.2, Eq. (5.2)] The effective numbers N_*^s weight fields by M^2/M_i^2, so the statement that the effect is 'determined by the lightest particle' is only true when there is no large multiplicity of heavier fields. This is stated implicitly, but a one-sentence caveat at Eq. (5.2) would prevent a common misreading.
- [§6] The discussion says that the magnitude of the effect is of order |\dot H|/\Lambda^2, which is correct for the dimension-4 case, but the dimension-6 contributions scale as |\dot H| H^2/(M^2 M_Pl^2) and are suppressed by an additional H^2/M^2 factor. A sentence distinguishing the two parametric regimes would avoid confusion.
Circularity Check
No significant circularity: the gravitational-wave speed is a direct EFT computation, and the positivity-sign input is an explicit external assumption rather than a recycled output.
full rationale
The paper's central speed formula, Eq. (3.36), is obtained by starting from the EFT action (3.16), expanding tensor modes on an FLRW background, perturbatively reducing the fourth-order equation of motion to the second-order hyperbolic form (3.7)-(3.10), and reading off the coefficient beta_1 as the propagation speed. No parameter is fitted to data, and no quantity is defined in terms of the claimed prediction. The later conclusion that gravitational waves are generically superluminal depends on the sign of C_W2, which is argued from S-matrix and spectral-density positivity bounds. Those arguments are explicitly conditional in the paper itself: Section 4.2 says the bounds apply 'provided we argue or assume that the contribution of the graviton exchange t-channel pole can be neglected', and Section 4.3.3 concedes that if the Kallen-Lehmann integrals (4.37) require subtractions then 'it is hence not possible to conclude positivity of the LHS'. These are external assumptions and caveats, not circular reductions: the existence of a possible sign ambiguity or an unproven assumption does not make the derivation circular. The references used for the t-channel-pole treatment and spectral positivity are independent works, not author-uniqueness claims, and the paper's own self-citations are peripheral to the main derivation. Therefore no significant circularity is present.
Assumptions & free parameters
free parameters (4)
- C_W2 (Weyl-squared coefficient)
- C_R2 (Ricci-squared coefficient)
- UV subtraction constants C_UV^{W2}, C_UV^{R2}
- C4 (non-minimal light-field curvature coupling)
assumptions (5)
- domain assumption The massless graviton t-channel pole can be neglected when applying forward-limit positivity bounds to matter scattering amplitudes.
- domain assumption The spectral densities rho_2(mu) and rho_0(mu) in the Kallen-Lehmann representation of the TT correlator are non-negative and the integrals in Eq. (4.37) converge without additional subtractions.
- domain assumption Matter fields sourcing the background and light fields are minimally coupled to the metric and have spin less than 2.
- domain assumption Graviton loops are not included when integrating out heavy fields; only matter loops are included.
- ad hoc to paper The IR curvature-squared coefficients are tuned to zero, C_IR^{W2} = C_IR^{R2} = 0, for the dimension-6 analysis.
Cite this review
Pith. "Pith review of The Speed of Gravity." pith.science (2026). https://pith.science/paper/ZWP7WXTF
@misc{pith2026190900881,
author = {Pith},
title = {Pith review of: The Speed of Gravity},
year = {2026},
howpublished = {\url{https://pith.science/paper/ZWP7WXTF}},
note = {Machine review of arXiv:1909.00881}
}
abstract
Within the standard effective field theory of General Relativity, we show that the speed of gravitational waves deviates, ever so slightly, from luminality on cosmological and other spontaneously Lorentz-breaking backgrounds. This effect results from loop contributions from massive fields of any spin, including Standard Model fields, or from tree level effects from massive higher spins $s \ge 2$. We show that for the choice of interaction signs implied by S-matrix and spectral density positivity bounds suggested by analyticity and causality, the speed of gravitational waves is in general superluminal at low-energies on NEC preserving backgrounds, meaning gravitational waves travel faster than allowed by the metric to which photons and Standard Model fields are minimally coupled. We show that departure of the speed from unity increases in the IR and argue that the speed inevitably returns to luminal at high energies as required by Lorentz invariance. Performing a special tuning of the EFT so that renormalization sensitive curvature-squared terms are set to zero, we find that finite loop corrections from Standard Model fields still lead to an epoch dependent modification of the speed of gravitational waves which is determined by the precise field content of the lightest particles with masses larger than the Hubble parameter today. Depending on interpretation, such considerations could potentially have far-reaching implications on light scalar models, such as axionic or fuzzy cold dark matter.
Forward citations
Cited by 3 Pith papers
-
Gravitational waveforms from binaries in higher-derivative gravity: a Love story
In higher-derivative gravity, the leading correction to extreme-mass-ratio inspiral waveforms and fluxes enters at 5PN order and is controlled by the ℓ=2 tidal Love number.
-
Propagator positivity bounds for cosmological correlators
An infinite tower of two-sided positivity bounds constrains the EFT coefficients of heavy fields on de Sitter, ruling out correlators with no unitary/causal UV completion.
-
Causality bounds from charged shockwaves in 5d
Causality on 5d charged shockwaves gives positivity bounds on four-derivative Einstein-Maxwell couplings, with gravity weakening the pure-field-theory bounds and near-horizon photons providing the strongest constraints.
Reference graph
Works this paper leans on
-
[27]
B. Bellazzini, M. Lewandowski and J. Serra, Amplitudes’ Positivity, Weak Gravity Conjecture, and Modified Gravity, 1902.03250
arXiv 1902
-
[1]
Virgo, LIGO Scientific collaboration, B. Abbott et al., GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral , Phys. Rev. Lett. 119 (2017) 161101, [ 1710.05832]
arXiv 2017
-
[2]
Virgo, Fermi-GBM, INTEGRAL, LIGO Scientific collaboration, B. P. Abbott et al., Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A , Astrophys. J. 848 (2017) L13, [ 1710.05834]
arXiv 2017
-
[3]
B. P. Abbott et al., Multi-messenger Observations of a Binary Neutron Star Merger , Astrophys. J. 848 (2017) L12, [ 1710.05833]. – 49 –
arXiv 2017
-
[4]
J. F. Donoghue, General relativity as an effective field theory: The leading quantum corrections , Phys. Rev. D50 (1994) 3874–3888, [ gr-qc/9405057]
arXiv 1994
-
[5]
J. F. Donoghue, Introduction to the effective field theory description of gravity , in Advanced School on Effective Theories Almunecar, Spain, June 25-July 1, 1995 , 1995. gr-qc/9512024
arXiv 1995
-
[6]
C. P. Burgess, Quantum gravity in everyday life: General relativity as an effective field theory , Living Rev. Rel. 7 (2004) 5–56, [ gr-qc/0311082]
arXiv 2004
-
[7]
J. F. Donoghue, The effective field theory treatment of quantum gravity , AIP Conf. Proc. 1483 (2012) 73–94, [1209.3511]
arXiv 2012
Show all 91 references
-
[8]
Ruhdorfer, J
M. Ruhdorfer, J. Serra and A. Weiler, Effective Field Theory of Gravity to All Orders , 1908.08050
1908 arXiv
-
[9]
Aharonov, A
Y. Aharonov, A. Komar and L. Susskind, Superluminal behavior, causality, and instability , Phys. Rev. 182 (1969) 1400–1403
1969
-
[10]
Adams, N
A. Adams, N. Arkani-Hamed, S. Dubovsky, A. Nicolis and R. Rattazzi, Causality, analyticity and an IR obstruction to UV completion , JHEP 10 (2006) 014, [ hep-th/0602178]
2006 arXiv
-
[11]
Gruzinov and M
A. Gruzinov and M. Kleban, Causality Constrains Higher Curvature Corrections to Gravity , Class. Quant. Grav. 24 (2007) 3521–3524, [ hep-th/0612015]
2007 arXiv
-
[12]
Cheung, P
C. Cheung, P. Creminelli, A. L. Fitzpatrick, J. Kaplan and L. Senatore, The Effective Field Theory of Inflation, JHEP 03 (2008) 014, [ 0709.0293]
2008 arXiv
-
[13]
Gubitosi, F
G. Gubitosi, F. Piazza and F. Vernizzi, The Effective Field Theory of Dark Energy , JCAP 1302 (2013) 032, [1210.0201]
2013 arXiv
-
[14]
Gleyzes, D
J. Gleyzes, D. Langlois, F. Piazza and F. Vernizzi, Essential Building Blocks of Dark Energy , JCAP 1308 (2013) 025, [ 1304.4840]
2013 arXiv
-
[15]
De Rham, L
C. De Rham, L. Keltner and A. J. Tolley, Generalized galileon duality, Phys. Rev. D90 (2014) 024050, [1403.3690]
2014 arXiv
-
[16]
N. E. J. Bjerrum-Bohr, J. F. Donoghue, B. R. Holstein, L. Plant´ e and P. Vanhove, Bending of Light in Quantum Gravity, Phys. Rev. Lett. 114 (2015) 061301, [ 1410.7590]
2015 arXiv
-
[17]
Bai and Y
D. Bai and Y. Huang, More on the Bending of Light in Quantum Gravity , Phys. Rev. D95 (2017) 064045, [1612.07629]
2017 arXiv
-
[18]
Chi, Graviton Bending in Quantum Gravity from One-Loop Amplitudes , Phys
H.-H. Chi, Graviton Bending in Quantum Gravity from One-Loop Amplitudes , Phys. Rev. D99 (2019) 126008, [1903.07944]
2019 arXiv
-
[19]
X. O. Camanho, J. D. Edelstein, J. Maldacena and A. Zhiboedov, Causality Constraints on Corrections to the Graviton Three-Point Coupling , JHEP 02 (2016) 020, [ 1407.5597]
2016 arXiv
-
[20]
Afkhami-Jeddi, S
N. Afkhami-Jeddi, S. Kundu and A. Tajdini, A Bound on Massive Higher Spin Particles , JHEP 04 (2019) 056, [ 1811.01952]
2019 arXiv
-
[21]
T. J. Hollowood and G. M. Shore, Causality Violation, Gravitational Shockwaves and UV Completion , JHEP 03 (2016) 129, [ 1512.04952]
2016 arXiv
-
[22]
T. N. Pham and T. N. Truong, Evaluation of the Derivative Quartic Terms of the Meson Chiral Lagrangian From Forward Dispersion Relation, Phys. Rev. D31 (1985) 3027
1985
-
[23]
Ananthanarayan, D
B. Ananthanarayan, D. Toublan and G. Wanders, Consistency of the chiral pion pion scattering amplitudes with axiomatic constraints , Phys. Rev. D51 (1995) 1093–1100, [ hep-ph/9410302]
1995 arXiv
-
[24]
de Rham, S
C. de Rham, S. Melville, A. J. Tolley and S.-Y. Zhou, Positivity bounds for scalar field theories , Phys. Rev. D96 (2017) 081702, [ 1702.06134]. – 50 –
2017 arXiv
-
[25]
de Rham, S
C. de Rham, S. Melville, A. J. Tolley and S.-Y. Zhou, UV complete me: Positivity Bounds for Particles with Spin, JHEP 03 (2018) 011, [ 1706.02712]
2018 arXiv
-
[26]
Bellazzini, C
B. Bellazzini, C. Cheung and G. N. Remmen, Quantum Gravity Constraints from Unitarity and Analyticity, Phys. Rev. D93 (2016) 064076, [ 1509.00851]
2016 arXiv
-
[28]
Mirbabayi, A Weak Gravity Theorem, 1905.02736
M. Mirbabayi, A Weak Gravity Theorem, 1905.02736
1905 arXiv
-
[29]
Cheung, J
C. Cheung, J. Liu and G. N. Remmen, Proof of the Weak Gravity Conjecture from Black Hole Entropy , JHEP 10 (2018) 004, [ 1801.08546]
2018 arXiv
-
[30]
I. T. Drummond and S. J. Hathrell, QED Vacuum Polarization in a Background Gravitational Field and Its Effect on the Velocity of Photons , Phys. Rev. D22 (1980) 343
1980
-
[31]
Lafrance and R
R. Lafrance and R. C. Myers, Gravity’s rainbow, Phys. Rev. D51 (1995) 2584–2590, [ hep-th/9411018]
1995 arXiv
-
[32]
T. J. Hollowood and G. M. Shore, Causality and Micro-Causality in Curved Spacetime , Phys. Lett. B655 (2007) 67–74, [ 0707.2302]
2007 arXiv
-
[33]
T. J. Hollowood and G. M. Shore, The Refractive index of curved spacetime: The Fate of causality in QED, Nucl. Phys. B795 (2008) 138–171, [ 0707.2303]
2008 arXiv
-
[34]
T. J. Hollowood and G. M. Shore, The Causal Structure of QED in Curved Spacetime: Analyticity and the Refractive Index, JHEP 12 (2008) 091, [ 0806.1019]
2008 arXiv
-
[35]
T. J. Hollowood, G. M. Shore and R. J. Stanley, The Refractive Index of Curved Spacetime II: QED, Penrose Limits and Black Holes , JHEP 08 (2009) 089, [ 0905.0771]
2009 arXiv
-
[36]
T. J. Hollowood and G. M. Shore, The Effect of Gravitational Tidal Forces on Vacuum Polarization: How to Undress a Photon , Phys. Lett. B691 (2010) 279–284, [ 1006.0145]
2010 arXiv
-
[37]
T. J. Hollowood and G. M. Shore, ‘Superluminal’ Photon Propagation in QED in Curved Spacetime is Dispersive and Causal , 1006.1238
-
[38]
T. J. Hollowood and G. M. Shore, The Effect of Gravitational Tidal Forces on Renormalized Quantum Fields, JHEP 02 (2012) 120, [ 1111.3174]
2012 arXiv
-
[39]
T. J. Hollowood and G. M. Shore, The Unbearable Beingness of Light, Dressing and Undressing Photons in Black Hole Spacetimes , Int. J. Mod. Phys. D21 (2012) 1241003, [ 1205.3291]
2012 arXiv
-
[40]
Caron-Huot, Z
S. Caron-Huot, Z. Komargodski, A. Sever and A. Zhiboedov, Strings from Massive Higher Spins: The Asymptotic Uniqueness of the Veneziano Amplitude , JHEP 10 (2017) 026, [ 1607.04253]
2017 arXiv
-
[41]
Afkhami-Jeddi, S
N. Afkhami-Jeddi, S. Kundu and A. Tajdini, A Conformal Collider for Holographic CFTs , JHEP 10 (2018) 156, [ 1805.07393]
2018 arXiv
-
[42]
de Rham, S
C. de Rham, S. Melville, A. J. Tolley and S.-Y. Zhou, Positivity Bounds for Massive Spin-1 and Spin-2 Fields, 1804.10624
-
[43]
Y.-Z. Chu, D. M. Jacobs, Y. Ng and G. D. Starkman, It’s Hard to Learn How Gravity and Electromagnetism Couple, Phys. Rev. D82 (2010) 064022, [ 1007.3992]
2010 arXiv
-
[44]
K. S. Stelle, Renormalization of Higher Derivative Quantum Gravity , Phys. Rev. D16 (1977) 953–969
1977
-
[45]
J. F. Donoghue and G. Menezes, Gauge Assisted Quadratic Gravity: A Framework for UV Complete Quantum Gravity, Phys. Rev. D97 (2018) 126005, [ 1804.04980]
2018 arXiv
-
[46]
J. F. Donoghue and G. Menezes, The arrow of causality and quantum gravity , 1908.04170
1908 arXiv
-
[47]
Lehners and K
J.-L. Lehners and K. S. Stelle, A Safe Beginning for the Universe? , 1909.01169. – 51 –
1909 arXiv
-
[48]
Coleman, Acausality, in 7th International School of Subnuclear Physics (Ettore Majorana): Subnuclear Phenomena Erice, Italy, July 3-19, 1969 , pp
S. Coleman, Acausality, in 7th International School of Subnuclear Physics (Ettore Majorana): Subnuclear Phenomena Erice, Italy, July 3-19, 1969 , pp. 282–327, 1969
1969
-
[49]
A. O. Barvinsky and G. A. Vilkovisky, The Generalized Schwinger-Dewitt Technique in Gauge Theories and Quantum Gravity , Phys. Rept. 119 (1985) 1–74
1985
-
[50]
A. O. Barvinsky, Yu. V. Gusev, V. V. Zhytnikov and G. A. Vilkovisky, Asymptotic behaviors of one loop vertices in the gravitational effective action , Class. Quant. Grav. 12 (1995) 2157–2172
1995
-
[51]
A. O. Barvinsky, Yu. V. Gusev, G. A. Vilkovisky and V. V. Zhytnikov, Asymptotic behaviors of the heat kernel in covariant perturbation theory , J. Math. Phys. 35 (1994) 3543–3559, [ gr-qc/9404063]
1994 arXiv
-
[52]
I. G. Avramidi, The Covariant Technique for Calculation of One Loop Effective Action , Nucl. Phys. B355 (1991) 712–754
1991
-
[53]
I. G. Avramidi, The Nonlocal Structure of the One Loop Effective Action via Partial Summation of the Asymptotic Expansion, Phys. Lett. B236 (1990) 443–449
1990
-
[54]
A. O. Barvinsky, Yu. V. Gusev, V. V. Zhytnikov and G. A. Vilkovisky, Covariant perturbation theory. 4. Third order in the curvature , 0911.1168
-
[55]
A. O. Barvinsky, Yu. V. Gusev, G. A. Vilkovisky and V. V. Zhytnikov, The Basis of nonlocal curvature invariants in quantum gravity theory. (Third order.) , J. Math. Phys. 35 (1994) 3525–3542, [gr-qc/9404061]
1994 arXiv
-
[56]
G. A. Vilkovisky, Expectation values and vacuum currents of quantum fields , Lect. Notes Phys. 737 (2008) 729–784, [ 0712.3379]
2008 arXiv
-
[57]
Codello and O
A. Codello and O. Zanusso, On the non-local heat kernel expansion , J. Math. Phys. 54 (2013) 013513, [1203.2034]
2013 arXiv
-
[58]
J. F. Donoghue and B. K. El-Menoufi, Nonlocal quantum effects in cosmology: Quantum memory, nonlocal FLRW equations, and singularity avoidance , Phys. Rev. D89 (2014) 104062, [ 1402.3252]
2014 arXiv
-
[59]
Creminelli, J
P. Creminelli, J. Gleyzes, J. Norena and F. Vernizzi, Resilience of the standard predictions for primordial tensor modes, Phys. Rev. Lett. 113 (2014) 231301, [ 1407.8439]
2014 arXiv
-
[60]
Endlich, V
S. Endlich, V. Gorbenko, J. Huang and L. Senatore, An effective formalism for testing extensions to General Relativity with gravitational waves , JHEP 09 (2017) 122, [ 1704.01590]
2017 arXiv
-
[61]
de Rham, G
C. de Rham, G. Gabadadze and A. J. Tolley, Resummation of Massive Gravity , Phys. Rev. Lett. 106 (2011) 231101, [ 1011.1232]
2011 arXiv
-
[62]
de Rham, Massive Gravity, Living Rev
C. de Rham, Massive Gravity, Living Rev. Rel. 17 (2014) 7, [ 1401.4173]
2014 arXiv
-
[63]
De Rham, L
C. De Rham, L. Heisenberg and A. J. Tolley, Spin-2 and the Weak Gravity Conjecture , 1812.01012
-
[64]
R. R. Caldwell, Green’s functions for gravitational waves in FRW space-times , Phys. Rev. D48 (1993) 4688–4692, [gr-qc/9309025]
1993 arXiv
-
[65]
Taylor, TT deformations in general dimensions , 1805.10287
M. Taylor, TT deformations in general dimensions , 1805.10287
-
[66]
M. Park, K. M. Zurek and S. Watson, A Unified Approach to Cosmic Acceleration , Phys. Rev. D81 (2010) 124008, [ 1003.1722]
2010 arXiv
-
[67]
J. K. Bloomfield and E. E. Flanagan, A Class of Effective Field Theory Models of Cosmic Acceleration , JCAP 1210 (2012) 039, [ 1112.0303]
2012 arXiv
-
[68]
Creminelli, M
P. Creminelli, M. A. Luty, A. Nicolis and L. Senatore, Starting the Universe: Stable Violation of the Null Energy Condition and Non-standard Cosmologies , JHEP 12 (2006) 080, [ hep-th/0606090]. – 52 –
2006 arXiv
-
[69]
Creminelli, G
P. Creminelli, G. D’Amico, J. Norena and F. Vernizzi, The Effective Theory of Quintessence: the w¡-1 Side Unveiled, JCAP 0902 (2009) 018, [ 0811.0827]
2009 arXiv
-
[70]
de Rham and S
C. de Rham and S. Melville, Unitary null energy condition violation in P(X) cosmologies , Phys. Rev. D95 (2017) 123523, [ 1703.00025]
2017 arXiv
-
[71]
Dubovsky, T
S. Dubovsky, T. Gregoire, A. Nicolis and R. Rattazzi, Null energy condition and superluminal propagation, JHEP 03 (2006) 025, [ hep-th/0512260]
2006 arXiv
-
[72]
Dvali, Black Holes and Large N Species Solution to the Hierarchy Problem , Fortsch
G. Dvali, Black Holes and Large N Species Solution to the Hierarchy Problem , Fortsch. Phys. 58 (2010) 528–536, [0706.2050]
2010 arXiv
-
[73]
de Rham, S
C. de Rham, S. Melville and A. J. Tolley, Improved Positivity Bounds and Massive Gravity , JHEP 04 (2018) 083, [ 1710.09611]
2018 arXiv
- [74]
-
[75]
Gillioz, X
M. Gillioz, X. Lu and M. A. Luty, Graviton Scattering and a Sum Rule for the c Anomaly in 4D CFT , JHEP 09 (2018) 025, [ 1801.05807]
2018 arXiv
-
[76]
Cheung and G
C. Cheung and G. N. Remmen, Positivity of Curvature-Squared Corrections in Gravity , Phys. Rev. Lett. 118 (2017) 051601, [ 1608.02942]
2017 arXiv
-
[77]
de Rham and S
C. de Rham and S. Melville, Gravitational Rainbows: LIGO and Dark Energy at its Cutoff , Phys. Rev. Lett. 121 (2018) 221101, [ 1806.09417]
2018 arXiv
-
[78]
T. J. Hollowood and G. M. Shore, Causality, Renormalizability and Ultra-High Energy Gravitational Scattering, J. Phys. A49 (2016) 215401, [ 1601.06989]
2016 arXiv
-
[79]
R. R. Metsaev and A. A. Tseytlin, Curvature Cubed Terms in String Theory Effective Actions , Phys. Lett. B185 (1987) 52–58
1987
-
[80]
I. G. Avramidi, Covariant methods for the calculation of the effective action in quantum field theory and investigation of higher derivative quantum gravity . PhD thesis, Moscow State U., 1986. hep-th/9510140
1986 arXiv
-
[81]
Holman, G
R. Holman, G. Lazarides and Q. Shafi, Axions and the Dark Matter of the Universe , Phys. Rev. D27 (1983) 995
1983
-
[82]
D. J. E. Marsh, Axions and ALPs: a very short introduction , in Proceedings, 13th Patras Workshop on Axions, WIMPs and WISPs, (PATRAS 2017): Thessaloniki, Greece, 15 May 2017 - 19, 2017 , pp. 59–74, 2018. 1712.03018. DOI
2017 arXiv
-
[83]
P. W. Graham, I. G. Irastorza, S. K. Lamoreaux, A. Lindner and K. A. van Bibber, Experimental Searches for the Axion and Axion-Like Particles , Ann. Rev. Nucl. Part. Sci. 65 (2015) 485–514, [1602.00039]
2015 arXiv
-
[84]
W. Hu, R. Barkana and A. Gruzinov, Cold and fuzzy dark matter , Phys. Rev. Lett. 85 (2000) 1158–1161, [astro-ph/0003365]
2000 arXiv
-
[85]
D. J. Gross and E. Witten, Superstring Modifications of Einstein’s Equations , Nucl. Phys. B277 (1986) 1
1986
-
[86]
Giusto and S
S. Giusto and S. D. Mathur, Fuzzball geometries and higher derivative corrections for extremal holes , Nucl. Phys. B738 (2006) 48–75, [ hep-th/0412133]
2006 arXiv
-
[87]
P. Milonni, Fast Light, Slow Light and Left-Handed Light, (Series in Optics and Optoelectronics) , Fast Light, Slow Light and Left-Handed Light (2004) 262 pages, [ (Taylor & Francis) ]
2004
-
[88]
Brillouin, Wave Propagation and Group Velocity (Series in Pure & Applied Physics) , Wave Propagation and Group Velocity(1960) 154 pages, [ (Academic Press) ]
L. Brillouin, Wave Propagation and Group Velocity (Series in Pure & Applied Physics) , Wave Propagation and Group Velocity(1960) 154 pages, [ (Academic Press) ]. – 53 –
1960
-
[89]
Baumann, D
D. Baumann, D. Green, H. Lee and R. A. Porto, Signs of Analyticity in Single-Field Inflation , Phys. Rev. D93 (2016) 023523, [ 1502.07304]
2016 arXiv
- [90]
-
[91]
Baumann, D
D. Baumann, D. Green and T. Hartman, Dynamical Constraints on RG Flows and Cosmology , 1906.10226. – 54 –
1906 arXiv
Reviewed August 14, 2026 · model on record in the stance chip above.
Discussion (0). Continue with ORCID to comment.