Non-Gaussianity and Strong-Coupling Problem in a Two-Field DHOST Bouncing Model
Pith reviewed 2026-06-28 09:11 UTC · model grok-4.3
The pith
Refined two-field DHOST bouncing model matches observed non-Gaussianity while remaining weakly coupled and stable.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
By refining the model parameters to align the local non-Gaussianity f_NL with observational bounds, the two-field DHOST bouncing cosmology remains free of instabilities and superluminality at linear order, and maintains a strong-coupling scale well above the characteristic energy scale throughout its evolution, establishing it as a fully viable model consistent with data.
What carries the argument
The parameter refinement in the two-field DHOST action that tunes the cubic interactions controlling f_NL while preserving the degeneracy conditions and background solution.
If this is right
- The model remains free of ghost, gradient and BKL instabilities at linear order.
- Propagation stays subluminal throughout the evolution.
- Predictions for the scalar spectral index and tensor-to-scalar ratio stay within observational limits.
- The theory stays weakly coupled at all relevant energy scales.
Where Pith is reading between the lines
- The same tuning procedure could be applied to other multi-field DHOST constructions to achieve nonlinear viability.
- Future tighter bounds on primordial non-Gaussianity would directly constrain the allowed parameter window in this class of models.
- If the strong-coupling scale remains high, the effective-field-theory description is reliable through the entire bounce phase.
Load-bearing premise
The specific parameter refinement chosen to match f_NL does not introduce new instabilities or alter the linear-level viability already established in the cited prior work.
What would settle it
A measurement of the local non-Gaussianity parameter f_NL lying outside the narrow range produced by the refined parameters, or detection of strong-coupling effects at energies below the claimed scale during the bounce.
read the original abstract
We recently constructed a two-field Degenerate Higher-Order Scalar-Tensor (DHOST) bouncing model which is fully viable at the linear level [1]. This model is completely free of Belinski-Khalatnikov-Lifshitz (BKL) instability, ghost instability, gradient instability and superluminality. It also predicts the scalar spectral index and tensor-toscalar ratio consistent with observations. The aim of this paper is to extend the viability of the model to the non-linear level. To this end, we first refine the original model such that its prediction on the (local) non-Gaussianity parameter fNL agrees with observations, leaving the viability of the model at the linear level intact. We furthermore demonstrate that the strong-coupling scale is well above the characteristic background energy scale all the time. Our model indeed exemplifies the fully viable two-field DHOST bouncing model, in the sense that it is weakly-coupled, stable and non-superluminal as well as consistent with observations.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper refines a two-field DHOST bouncing model from prior work [1] by adjusting parameters to match the observed local non-Gaussianity f_NL, asserts that this leaves the linear-level stability (no ghosts, no gradient instabilities, no superluminality, no BKL) and observational consistency (n_s, r) intact, demonstrates that the strong-coupling scale remains above the background energy scale at all times, and concludes that the model is fully viable at both linear and nonlinear levels.
Significance. If the claims hold, this would constitute a concrete example of a weakly coupled, stable, non-superluminal two-field DHOST bounce that is also consistent with CMB constraints on non-Gaussianity. The explicit treatment of the strong-coupling scale is a strength relative to many bouncing constructions.
major comments (1)
- [Abstract and §1] Abstract and §1: The central viability claim requires that the refined parameters chosen to match f_NL preserve the linear no-ghost, no-gradient-instability, and no-superluminality conditions established in [1]. The manuscript states that linear viability remains intact but does not show an explicit recomputation of the quadratic action coefficients or the associated stability criteria with the new parameter values across the full background evolution (including near the bounce). This step is load-bearing and must be supplied.
Simulated Author's Rebuttal
We thank the referee for the careful reading of our manuscript and for highlighting this important point regarding the central viability claim. We address the major comment below and will incorporate the requested verification in the revision.
read point-by-point responses
-
Referee: [Abstract and §1] Abstract and §1: The central viability claim requires that the refined parameters chosen to match f_NL preserve the linear no-ghost, no-gradient-instability, and no-superluminality conditions established in [1]. The manuscript states that linear viability remains intact but does not show an explicit recomputation of the quadratic action coefficients or the associated stability criteria with the new parameter values across the full background evolution (including near the bounce). This step is load-bearing and must be supplied.
Authors: We agree that an explicit recomputation of the quadratic action coefficients and stability criteria with the refined parameters is necessary to fully substantiate the claim. In the revised manuscript we will add this analysis, verifying the absence of ghosts, gradient instabilities and superluminality for the new parameter values throughout the background evolution, including near the bounce. The updated results will be presented in §1 (or a dedicated subsection) to support the linear-level viability statement. revision: yes
Circularity Check
Linear viability of f_NL-refined parameters asserted via self-citation without re-derivation
specific steps
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self citation load bearing
[Abstract]
"We recently constructed a two-field Degenerate Higher-Order Scalar-Tensor (DHOST) bouncing model which is fully viable at the linear level [1]. ... we first refine the original model such that its prediction on the (local) non-Gaussianity parameter fNL agrees with observations, leaving the viability of the model at the linear level intact. ... Our model indeed exemplifies the fully viable two-field DHOST bouncing model, in the sense that it is weakly-coupled, stable and non-superluminal as well as consistent with observations."
The claim that the refined model remains fully viable (stable, non-superluminal) at linear level is justified only by self-citation to [1] plus the bare assertion that refinement leaves viability intact; no re-derivation or recomputation of no-ghost/no-gradient conditions for the new parameters is provided in the quoted text.
full rationale
The paper's central viability claim for the refined model rests on the assertion that linear-level stability from prior self-cited work [1] remains intact after parameter adjustment for f_NL matching. This is a moderate self-citation load-bearing step, but the paper provides independent content on strong-coupling scale and non-linear checks. No equations reduce by construction to inputs, and no fitted quantity is renamed as an independent prediction.
Axiom & Free-Parameter Ledger
Reference graph
Works this paper leans on
-
[1]
O. S. An, J. U. Kang, Y. J. Kim, U. R. Mun and U. G. Ri,Fully viable DHOST bounce with extra scalar,JHEP05(2025) 005 [2501.09985]
arXiv 2025
-
[2]
M. Novello and S. E. P. Bergliaffa,Bouncing Cosmologies,Phys. Rept.463(2008) 127 [0802.1634]
Pith/arXiv arXiv 2008
-
[3]
D. Battefeld and P. Peter,A Critical Review of Classical Bouncing Cosmologies,Phys. Rept. 571(2015) 1 [1406.2790]
Pith/arXiv arXiv 2015
-
[4]
R. Brandenberger and P. Peter,Bouncing Cosmologies: Progress and Problems,Found. Phys.47(2017) 797 [1603.05834]
Pith/arXiv arXiv 2017
-
[5]
A. H. Guth,The Inflationary Universe: A Possible Solution to the Horizon and Flatness Problems,Phys. Rev. D23(1981) 347
1981
-
[6]
A. A. Starobinsky,A New Type of Isotropic Cosmological Models Without Singularity,Phys. Lett. B91(1980) 99
1980
-
[7]
A. D. Linde,A New Inflationary Universe Scenario: A Possible Solution of the Horizon, Flatness, Homogeneity, Isotropy and Primordial Monopole Problems,Phys. Lett. B108 (1982) 389
1982
-
[8]
Penrose,Gravitational collapse and space-time singularities,Phys
R. Penrose,Gravitational collapse and space-time singularities,Phys. Rev. Lett.14(1965) 57
1965
-
[9]
S. W. Hawking and R. Penrose,The Singularities of gravitational collapse and cosmology, Proc. Roy. Soc. Lond. A314(1970) 529
1970
-
[10]
A. Borde and A. Vilenkin,Singularities in inflationary cosmology: A Review,Int. J. Mod. Phys. D5(1996) 813 [gr-qc/9612036]
Pith/arXiv arXiv 1996
-
[11]
A. Borde, A. H. Guth and A. Vilenkin,Inflationary space-times are incompletein past directions,Phys. Rev. Lett.90(2003) 151301 [gr-qc/0110012]
Pith/arXiv arXiv 2003
-
[12]
J. E. Lesnefsky, D. A. Easson and P. C. W. Davies,Past-completeness of inflationary spacetimes,Phys. Rev. D107(2023) 044024 [2207.00955]
arXiv 2023
-
[13]
V. A. Rubakov,The Null Energy Condition and its violation,Phys. Usp.57(2014) 128 [1401.4024]
Pith/arXiv arXiv 2014
-
[14]
S. Mironov and V. Volkova,Non-singular cosmological scenarios in scalar-tensor theories and their stability: a review,2409.16108
-
[15]
S. Mironov, V. Rubakov and V. Volkova,Superluminality in DHOST theory with extra scalar,JHEP04(2021) 035 [2011.14912]. – 30 –
arXiv 2021
-
[16]
D. Langlois and K. Noui,Degenerate higher derivative theories beyond Horndeski: evading the Ostrogradski instability,JCAP02(2016) 034 [1510.06930]
Pith/arXiv arXiv 2016
-
[17]
J. Ben Achour, D. Langlois and K. Noui,Degenerate higher order scalar-tensor theories beyond Horndeski and disformal transformations,Phys. Rev. D93(2016) 124005 [1602.08398]
Pith/arXiv arXiv 2016
-
[18]
D. Langlois, M. Mancarella, K. Noui and F. Vernizzi,Effective Description of Higher-Order Scalar-Tensor Theories,JCAP05(2017) 033 [1703.03797]
Pith/arXiv arXiv 2017
-
[19]
D. Langlois,Dark energy and modified gravity in degenerate higher-order scalar–tensor (DHOST) theories: A review,Int. J. Mod. Phys. D28(2019) 1942006 [1811.06271]
Pith/arXiv arXiv 2019
-
[20]
Kobayashi,Horndeski theory and beyond: a review,Rept
T. Kobayashi,Horndeski theory and beyond: a review,Rept. Prog. Phys.82(2019) 086901 [1901.07183]
Pith/arXiv arXiv 2019
-
[21]
V. Belinsky, I. Khalatnikov and E. Lifshitz,Oscillatory approach to a singular point in the relativistic cosmology,Adv. Phys.19(1970) 525. [22]Planckcollaboration,Planck 2018 results. IX. Constraints on primordial non-Gaussianity, Astron. Astrophys.641(2020) A9 [1905.05697]
Pith/arXiv arXiv 1970
-
[22]
J. Khoury, B. A. Ovrut, P. J. Steinhardt and N. Turok,The Ekpyrotic universe: Colliding branes and the origin of the hot big bang,Phys. Rev. D64(2001) 123522 [hep-th/0103239]
Pith/arXiv arXiv 2001
-
[23]
E. I. Buchbinder, J. Khoury and B. A. Ovrut,New Ekpyrotic cosmology,Phys. Rev. D76 (2007) 123503 [hep-th/0702154]
Pith/arXiv arXiv 2007
-
[24]
A. M. Levy, A. Ijjas and P. J. Steinhardt,Scale-invariant perturbations in ekpyrotic cosmologies without fine-tuning of initial conditions,Phys. Rev. D92(2015) 063524 [1506.01011]
Pith/arXiv arXiv 2015
-
[25]
W. G. Cook, I. A. Glushchenko, A. Ijjas, F. Pretorius and P. J. Steinhardt,Supersmoothing through Slow Contraction,Phys. Lett. B808(2020) 135690 [2006.01172]
arXiv 2020
- [26]
- [27]
- [28]
-
[29]
L. Leblond and S. Shandera,Simple Bounds from the Perturbative Regime of Inflation, JCAP08(2008) 007 [0802.2290]
Pith/arXiv arXiv 2008
-
[30]
D. Baumann, L. Senatore and M. Zaldarriaga,Scale-Invariance and the Strong Coupling Problem,JCAP05(2011) 004 [1101.3320]
Pith/arXiv arXiv 2011
-
[31]
M. Koehn, J.-L. Lehners and B. Ovrut,Nonsingular bouncing cosmology: Consistency of the effective description,Phys. Rev. D93(2016) 103501 [1512.03807]
Pith/arXiv arXiv 2016
-
[32]
A. Dehghani, G. Geshnizjani and J. Quintin,Cuscuton Bounce Beyond the Linear Regime: Bispectrum and Strong Coupling Constraints,JCAP05(2025) 026 [2503.01992]
arXiv 2025
-
[33]
C. de Rham and S. Melville,Unitary NEC violation in P(X) cosmologies,Phys. Rev. D95 (2017) 123523 [1703.00025]. – 31 –
Pith/arXiv arXiv 2017
-
[34]
A. Fertig, J.-L. Lehners, E. Mallwitz and E. Wilson-Ewing,Converting entropy to curvature perturbations after a cosmic bounce,JCAP10(2016) 005 [1607.05663]
Pith/arXiv arXiv 2016
-
[35]
J.-L. Lehners and P. J. Steinhardt,Multifield Cosmological Perturbations at Third Order and the Ekpyrotic Trispectrum,Phys. Rev. D80(2009) 063533 [0906.0530]
Pith/arXiv arXiv 2009
-
[36]
Lehners,Ekpyrotic Non-Gaussianity: A Review,Adv
J.-L. Lehners,Ekpyrotic Non-Gaussianity: A Review,Adv. Astron.2010(2010) 903907 [1001.3125]
Pith/arXiv arXiv 2010
-
[37]
A. Fertig and J. L. Lehners,The Non-Minimal Ekpyrotic Trispectrum,JCAP01(2016) 026 [1510.03439]
Pith/arXiv arXiv 2016
-
[38]
Y. A. Ageeva, O. A. Evseev, O. I. Melichev and V. A. Rubakov,Horndeski Genesis: strong coupling and absence thereof,EPJ Web Conf.191(2018) 07010 [1810.00465]
Pith/arXiv arXiv 2018
- [39]
- [40]
-
[41]
Y. Ageeva and P. Petrov,On the strong coupling problem in cosmologies with ”strong gravity in the past”,Mod. Phys. Lett. A37(2022) 2250171 [2206.10646]
arXiv 2022
- [42]
-
[43]
A. Ijjas and P. J. Steinhardt,Fully stable cosmological solutions with a non-singular classical bounce,Phys. Lett. B764(2017) 289 [1609.01253]
arXiv 2017
-
[44]
A. Ijjas and P. J. Steinhardt,Classically stable nonsingular cosmological bounces,Phys. Rev. Lett.117(2016) 121304 [1606.08880]
arXiv 2016
-
[45]
M. Libanov, S. Mironov and V. Rubakov,Generalized Galileons: instabilities of bouncing and Genesis cosmologies and modified Genesis,JCAP08(2016) 037 [1605.05992]
Pith/arXiv arXiv 2016
-
[46]
R. Kolevatov, S. Mironov, N. Sukhov and V. Volkova,Cosmological bounce and Genesis beyond Horndeski,JCAP08(2017) 038 [1705.06626]
Pith/arXiv arXiv 2017
-
[47]
S. Mironov, V. Rubakov and V. Volkova,Bounce beyond Horndeski with GR asymptotics and γ-crossing,JCAP10(2018) 050 [1807.08361]
Pith/arXiv arXiv 2018
-
[48]
Y. Cai and Y.-S. Piao,A covariant Lagrangian for stable nonsingular bounce,JHEP09 (2017) 027 [1705.03401]
Pith/arXiv arXiv 2017
-
[49]
T. Qiu, X. Gao and E. N. Saridakis,Towards anisotropy-free and nonsingular bounce cosmology with scale-invariant perturbations,Phys. Rev. D88(2013) 043525 [1303.2372]
Pith/arXiv arXiv 2013
-
[50]
Li,Note on the production of scale-invariant entropy perturbation in the Ekpyrotic universe,Phys
M. Li,Note on the production of scale-invariant entropy perturbation in the Ekpyrotic universe,Phys. Lett. B724(2013) 192 [1306.0191]
Pith/arXiv arXiv 2013
-
[51]
A. Fertig, J.-L. Lehners and E. Mallwitz,Ekpyrotic Perturbations With Small Non-Gaussian Corrections,Phys. Rev. D89(2014) 103537 [1310.8133]
Pith/arXiv arXiv 2014
-
[52]
D. Langlois and F. Vernizzi,Nonlinear perturbations of cosmological scalar fields,JCAP 0702(2007) 017 [astro-ph/0610064]
Pith/arXiv arXiv 2007
-
[53]
A. Ijjas, J.-L. Lehners and P. J. Steinhardt,General mechanism for producing scale-invariant perturbations and small non-Gaussianity in ekpyrotic models,Phys. Rev. D89(2014) 123520 [1404.1265]. – 32 –
Pith/arXiv arXiv 2014
-
[54]
L. Battarra, M. Koehn, J.-L. Lehners and B. A. Ovrut,Cosmological Perturbations Through a Non-Singular Ghost-Condensate/Galileon Bounce,JCAP07(2014) 007 [1404.5067]
Pith/arXiv arXiv 2014
-
[55]
J. Maldacena,Non-Gaussian features of primordial fluctuations in single field inflationary models,JHEP05(2003) 013 [astro-ph/0210603]
Pith/arXiv arXiv 2003
-
[56]
T. Kobayashi, M. Yamaguchi and J. Yokoyama,Primordial non-Gaussianity from G-inflation,Phys. Rev. D83(2011) 103524 [1103.1740]
Pith/arXiv arXiv 2011
-
[57]
Wang,Inflation, Cosmic Perturbations and Non-Gaussianities,Commun
Y. Wang,Inflation, Cosmic Perturbations and Non-Gaussianities,Commun. Theor. Phys. 62(2014) 109 [1303.1523]
Pith/arXiv arXiv 2014
-
[58]
M. Braglia and L. Pinol,No time to derive: unraveling total time derivatives in in-in perturbation theory,JHEP08(2024) 068 [2403.14558]
arXiv 2024
-
[59]
C. Burrage, R. H. Ribeiro and D. Seery,Large slow-roll corrections to the bispectrum of noncanonical inflation,JCAP07(2011) 032 [1103.4126]
Pith/arXiv arXiv 2011
-
[60]
R. Kawaguchi, S. Tsujikawa and Y. Yamada,Roles of boundary and equation-of-motion terms in cosmological correlation functions,Phys. Lett. B856(2024) 138962 [2403.16022]
arXiv 2024
-
[61]
M. Koehn, J.-L. Lehners and B. A. Ovrut,Cosmological super-bounce,Physical ReviewD90 (2014) 025005 [1310.7577]
Pith/arXiv arXiv 2014
-
[62]
A. De Felice and S. Tsujikawa,Primordial non-Gaussianities in general modified gravitational models of inflation,JCAP04(2011) 029 [1103.1172]
Pith/arXiv arXiv 2011
-
[63]
Koyama,Non-Gaussianity of quantum fields during inflation,Class
K. Koyama,Non-Gaussianity of quantum fields during inflation,Class. Quant. Grav.27 (2010) 124001 [1002.0600]
Pith/arXiv arXiv 2010
-
[64]
S. Renaux-Petel and G. Tasinato,Nonlinear perturbations of cosmological scalar fields with non-standard kinetic terms,JCAP0901(2009) 012 [0810.2405]
Pith/arXiv arXiv 2009
-
[65]
D. Langlois and F. Vernizzi,A geometrical approach to nonlinear perturbations in relativistic cosmology,Class. Quant. Grav.27(2010) 124007 [1003.3270]. – 33 –
Pith/arXiv arXiv 2010
discussion (0)
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