Pith. sign in

REVIEW 3 major objections 3 minor 57 references

Quadratic gravity's frame changes, auxiliary eliminations, and Weyl rescalings commute off-shell; generic nonminimal couplings then generate a positive R^2 sector and a single-field Starobinsky attractor predicting r ≈ (3.3–4.8)×10^-3.

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

2026-08-03 13:40 UTC pith:CMIKUN4K

load-bearing objection A useful review of known quadratic-gravity equivalences wrapped in an overclaimed theorem; the new selection bound rests on a misapplied Brownian-bridge formula. the 3 major comments →

arxiv 2512.23401 v2 pith:CMIKUN4K submitted 2025-12-29 hep-th gr-qc

Universal Nonminimal Coupling-to-Starobinsky Matching and a Single-Field Attractor

classification hep-th gr-qc MSC 83D0583F05 PACS 04.50.Kd98.80.Cq
keywords quadratic gravityStarobinsky inflationnonminimal couplingHubbard-StratonovichWeyl rescalingPalatinisingle-field attractortensor-to-scalar ratio
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved

The pith

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

This paper proves an off-shell commutativity theorem: in four-dimensional parity-even quadratic gravity, the Hubbard–Stratonovich/Legendre lifts, algebraic elimination of auxiliary fields (including the torsionless Palatini connection), and Jordan–Einstein Weyl rescalings commute at the action level up to boundary terms, so the reduced bulk action is unique regardless of ordering. It follows that the propagating degrees of freedom are frame-independent: the metric branch carries a massless graviton, a scalaron of mass M_Pl^2/(12α'), and a massive spin-2 ghost that acts as a Weyl spectator; the Palatini branch has no propagating scalar. Integrating out generic heavy nonminimally coupled scalars generates a universal positive R^2 coefficient α'_NMC = (1/2)F_a(M^{-2})^{ab}F_b, fixing the scalaron mass in terms of a heavy-sector projection. Applied to inflation, the paper derives a single-field attractor bound enhanced by a 'Doob selection' term 3/ΔN, which exponentially suppresses isocurvature and yields sharp CMB targets: n_s ≈ 1 - 2/N_*, r ≈ 12/N_*^2 ≈ (3.3–4.8)×10^-3 for N_* ∈ [50,60]. A sympathetic reader would care because this offers a universal, falsifiable explanation for why many UV completions flow to the same Starobinsky-like single-field infrared behavior.

Core claim

The paper proves that HS/Legendre lifts, algebraic elimination of auxiliaries (including Palatini Γ), and Weyl rescalings commute off-shell in 4D parity-even quadratic gravity, so the reduced action is unique. The metric branch carries a massless graviton, a scalaron of mass M_Pl^2/(12α'), and a massive spin-2 ghost that is a Weyl spectator. Integrating out heavy nonminimally coupled scalars generates α'_NMC = (1/2)F_a(M^{-2})^{ab}F_b, a positive R^2 coefficient, and the total scalaron mass fixes CMB observables. The Weyl uplift K^2 plus a Doob-selection term 3/ΔN produce the single-field attractor m_{s,eff}^2/H^2 ≥ 3V_{;ss}/V + K^2 + 3/ΔN and the Starobinsky target r ≈ 12/N_*^2.

What carries the argument

The central objects are (i) the off-shell commuting square: HS/Legendre lifts, algebraic elimination of auxiliaries (including the Palatini connection Γ), and Weyl rescalings commute as local algebraic operations; (ii) the shifted quadratic-gravity coefficients α' = α + β/3 and δ_eff = δ + β/2 that control the scalar and spin-2 spectra; (iii) the heavy-sector projection F_a (M^{-2})^{ab} F_b that sets the generated R^2 coefficient; and (iv) the Weyl uplift K^2 = 3[4(∂_s ln Φ)^2 - 2∇_s∇_s ln Φ - 4(∂_s ln Φ) V_{;s}/V], which the paper claims is positive and enhances entropic stability, together with the Doob selection mass 3/ΔN.

Load-bearing premise

The single-field attractor bound (Eq. 14) hinges on the claim that the 'Weyl uplift' K^2 (Eq. 44) is positive definite, but the displayed expression contains negatively signed terms (-2∇_s∇_s ln Φ and -4(∂_s ln Φ)V_{;s}/V); no proof of overall positivity is provided, and if K^2 can be negative, the threshold 3V_{;ss}/V + K^2 ≳ 0.945 and the stability window collapse.

What would settle it

Compute K^2 for a simple two-field model (e.g., the linear-NMC Starobinsky example in the appendix) across a range of parameters; a single example with K^2 < 0 that also violates the attractor bound would break the single-field claim. Alternatively, if next-generation CMB experiments (LiteBIRD, CMB-S4) detect isocurvature or non-Gaussianity at levels the paper says are exponentially suppressed, the attractor bound is empirically falsified.

Watch this falsifier — get emailed when new claim-graph text bears on it.

If this is right

  • Any heavy nonminimal coupling sector leaves a universal Starobinsky-type R^2 footprint, so diverse UV completions share the same infrared scalaron dynamics.
  • Measuring the tensor-to-scalar ratio r fixes the total α'_tot, yielding an integral constraint on the heavy-sector projection F_a(M^{-2})^{ab}F_b.
  • The combination of Weyl uplift and Doob selection suppresses isocurvature whenever 3V_{;ss}/V + K^2 + 3/ΔN ≥ 1, explaining the observed single-field nature of inflation.
  • Palatini f(R) is confirmed to carry no extra propagating scalar, as the ω = -3/2 cancellation eliminates the kinetic term.
  • The CMB predictions n_s ≈ 1 - 2/N_*, r ≈ 12/N_*^2, and n_T = -r/8 are flatly falsifiable by next-generation experiments.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • The commutativity theorem may extend to higher dimensions or odd-parity curvature terms, as long as the Weyl-spectator status of the spin-2 sector persists.
  • The 3/ΔN selection term is a cosmological conditioning effect, not a Lagrangian input; equivalently, the single-field attractor is environment-dependent rather than a property of the vacuum theory.
  • The positivity of K^2 is the load-bearing geometric assumption; a concrete counterexample with K^2 < 0 would narrow or void the stability window and could be sought in simple two-field models.
  • Future CMB data combining r and isocurvature bounds could, in principle, map the field-space metric G_IJ itself, not just the projection F_a(M^{-2})^{ab}F_b.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit.

Referee Report

3 major / 3 minor

Summary. The paper claims to prove an off-shell commutativity theorem for 4D parity-even quadratic gravity: Hubbard–Stratonovich/Legendre lifts, algebraic elimination of auxiliaries (including the Palatini connection), and Jordan–Einstein Weyl rescalings commute at the action level up to boundary terms. It then derives a frame-universal matching from generic nonminimal couplings to an R^2 sector, with α'_NMC = (1/2) F_a (M^{-2})^{ab} F_b, and proposes a quantitative single-field attractor bound enhanced by a universal 1/ΔN 'Doob selection' mass, leading to the standard Starobinsky CMB target r ≈ 12/N_*^2 ≈ (3.3–4.8)×10^{-3}.

Significance. If the central claims were established, the paper would offer a useful organizational framework for frame transformations in quadratic gravity and a new mechanism explaining single-field inflation. The paper is clearly written and gives the standard Starobinsky predictions correctly. However, the genuinely new elements—the selection-enhanced attractor and the positivity of the Weyl uplift—are not rigorously supported. The commutativity theorem is proven only in the f(R) scalar channel, not for the full quadratic basis stated in the abstract. The standard Starobinsky tensor-to-scalar ratio is independent of the new selection term, so the paper's original contribution rests on the unsupported stochastic calculation. The manuscript does provide a useful pedagogical restatement of known f(R)/Palatini equivalences, but its novel quantitative claims are not reliable.

major comments (3)
  1. [Appendix 3, Eqs. (45)–(52)] The derivation of the Doob selection mass 3/ΔN is incorrect. The survival probability for the OU process with absorbing boundaries at ±Λ does not have the bulk Gaussian form exp(−s^2/(4DΔN)) for large ΔN. For ΔN ≫ Λ^2/(Dπ^2), the backward solution is dominated by the principal eigenmode, h ∝ cos(πs/(2Λ)) exp(−Dπ^2ΔN/(4Λ^2)), whose log-derivative is approximately −π^2 s/(4Λ^2), independent of ΔN. Equation (49) is the free heat-kernel or Brownian-bridge factor, not the killed-diffusion survival probability. Consequently Eq. (50) and the universal shift in Eq. (13)/(51) do not follow. Moreover, dropping the OU drift μ in Eq. (48) is circular because μ ≡ m_s^2/(3H^2) is exactly the quantity the bound is intended to constrain. Since Eq. (14) and the threshold 3V_{;ss}/V + K^2 ≳ 0.945 depend on this selection term, the single-field attractor claim is unsupported.
  2. [Sec. II, Appendix 1] The off-shell commutativity theorem is stated for the full parity-even quadratic basis (Eq. (1)), but the proof is given only for the f(R) (α-only) scalar channel. The spin-2 sector is handled by asserting that sqrt(−g)C^2 is a 'spectator' under Weyl maps, and the Palatini ω = −3/2 case is treated separately; no explicit demonstration is provided that HS lifts, elimination of auxiliaries, and Weyl rescalings commute when β and δ are present. The commuting diagram in Fig. 1 is therefore not established for the generic action claimed in the abstract. The known f(R) equivalence is not in question, but the universal theorem's scope is.
  3. [Eqs. (12), (44)] The claim K^2 ≥ 0 ('Weyl uplift') is stated without proof and is not manifest from Eq. (44): the expression contains −2∇_s∇_s ln Φ and −4(∂_s ln Φ)V_{;s}/V, which are sign-indefinite. The total bound in Eq. (14) and the stability window in Fig. 2 rely on this positivity. If K^2 can be negative, the threshold 3V_{;ss}/V + K^2 ≳ 0.945 may be much harder or impossible to satisfy. A rigorous proof or a counterexample with explicit sign is needed before the attractor claim can be assessed.
minor comments (3)
  1. [Eq. (17)] The equation equates α'_bare + (1/2)F_a(M^{-2})^{ab}F_b with a dimensionless number ∼10^9, but α' has dimensions of (mass)^{-2} in units where M_Pl is not set to 1. The expression should be written consistently with the reduced Planck mass, or the units stated.
  2. [Figs. 2 and 3] The stability maps are difficult to interpret because the vertical axes are labeled with different quantities ('K^2' and 'μ/M_Pl') and the meaning of 'c* = 0.1' in Fig. 2 is not defined in the caption. Please clarify the exact quantity plotted and the parameter definitions.
  3. [References] Some references to recent literature (e.g., [34] Wolf et al. 2025) are appropriately cited, but the connection between the 'volume-selection' effect of [21] and the present Doob-conditioning argument could be more explicitly contrasted; the paper currently suggests a stronger link than the cited work may support.

Circularity Check

1 steps flagged

The commutativity and R^2-matching results are self-contained, but the new 1/ΔN 'Doob selection' term in the central attractor bound is constructed from a Brownian-bridge Gaussian and from dropping the very mass it later adds.

specific steps
  1. self definitional [Sec. V, Eq. (13); Appendix 3, Eqs. (45)-(51); used in Eq. (14)]
    "Let h(s,N) ≡ P(τΛ > NF | s(N) = s) denote the survival probability up to NF ... h(±Λ,N) = 0 ... In this regime the universal selection effect is captured by momentarily dropping the weak OU drift in the backward equation, i.e. setting μ≃0 in Eq. (46) ... h(s,ΔN)∝exp(−s²/(4DΔN)) ... 2D∂s lnh≃−s/ΔN ... m²_{s,sel}/H² ≡3μ_sel≃3/ΔN."

    The derivation defines h as the survival probability for absorbing boundaries at ±Λ (Eqs. 45-46), but then replaces it with the unbounded-domain Gaussian exp(−s²/(4DΔN)) (Eq. 49). That Gaussian is the Brownian-bridge/heat-kernel factor conditioning on a final position, not the solution of the absorbing-boundary survival problem, and it does not satisfy h(±Λ)=0. The resulting 'selection mass' 3/ΔN is therefore not an independent consequence of survival selection; it is the inverse of the chosen conditioning duration ΔN repackaged as a mass shift. Moreover, Eq. (45) defines μ≡m²_s/(3H²), the very entropic mass the bound is supposed to control, and Eq. (48) sets μ≃0 to obtain this term; Eq. (14) then adds the term back to m²_s. The claimed stabilization is thus an identity in the construction

full rationale

The paper's algebraic core — the off-shell commuting square, the Palatini ω=−3/2 algebraicity, and the heavy-field matching α'_NMC = ½ F_a(M^{-2})^{ab}F_b — is presented as explicit local tree-level manipulation with no fitted parameters and no load-bearing self-citations; those parts are not circular. The Starobinsky CMB numbers r ≈ 12/N_*^2 follow from the standard plateau potential and are independent of the new selection mechanism. The circularity is localized in the 'selection-enhanced attractor bound' of Sec. V: the 1/ΔN term is obtained by replacing the absorbing-boundary survival problem with an unbounded-domain Gaussian (a Brownian-bridge conditioning, not survival), and by setting μ≡m²_s/(3H²) to zero in that derivation before adding the resulting 3/ΔN back to m²_s in Eq. (14). This affects the headline quantitative attractor bound (Eq. 14) but not the frame-universality and R^2-matching results. Score 6 reflects partial circularity in a central claim, with the independent commutativity and matching results kept separate.

Axiom & Free-Parameter Ledger

1 free parameters · 7 axioms · 0 invented entities

The paper relies on standard f(R)/Legendre and conformal-transformation results, plus two ad hoc short-cuts (K^2 ≥ 0 and the driftless Gaussian survival profile) that carry the phenomenological claims.

free parameters (1)
  • ΔN (remaining e-folds to end of inflation) = ~55 (fiducial window 50–60)
    The Doob selection term 3/ΔN and the threshold 0.945 are evaluated at ΔN=55; the bound shifts if a different number of observable e-folds is used.
axioms (7)
  • domain assumption The Legendre transform/HS lift is valid only when auxiliary fields enter algebraically and f''(R) > 0.
    Stated in Sec. II before the Commutativity Theorem; restricts the universality claim.
  • standard math The 4D identities C^2 = R^2_{μνρσ} - 2R^2_{μν} + (1/3)R^2 and G = R^2_{μνρσ} - 4R^2_{μν} + R^2 hold.
    Used in Sec. II to define α' and δ_eff; these are standard 4D curvature identities.
  • standard math Under Weyl rescaling, √−g Φ R transforms to √−g̃[(M_Pl^2/2)R̃ − (3M_Pl^2/(4Φ^2))(∇̃Φ)^2] plus a boundary term.
    Used in the scalar-channel commutativity proof (Appendix S1) and Einstein-frame geometry (Appendix S2).
  • domain assumption The heavy fields sit at a minimum with Hessian (M^2)_{ab} ≫ H^2, and kinetic terms are negligible at E^2 ≪ M^2_heavy so the heavy EOM is algebraic.
    Sec. IV; this is the expansion that generates the R^2 operator and the R□R tower and defines the regime of validity.
  • ad hoc to paper The survival probability in the bulk obeys h ∝ exp(−s^2/(4DΔN)) after dropping the OU drift (µ≃0) in the backward Fokker-Planck equation.
    Appendix S3, Eqs. (48)–(49); the drift is exactly the quantity the attractor bound is trying to control, so this is not justified.
  • ad hoc to paper The 'Weyl uplift' K^2 defined in Eq. (44) is positive definite.
    Sec. V; asserted but not proven; the formula contains negative contributions and is not manifestly non-negative.
  • domain assumption The massive spin-2 ghost can be treated as a heavy regulator that decouples (m_2 ≳ Λ_EFT ≫ H) and does not affect low-energy scalaron dynamics.
    Sec. II and Discussion; needed to ignore the ghost in the light-field limit.

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read the original abstract

We establish an off-shell commutativity theorem in 4D parity-even quadratic gravity that the Hubbard-Stratonovich/Legendre lifts, algebraic elimination of auxiliaries, including the torsionless Palatini connection, and Jordan-Einstein Weyl rescalings commute at the action level up to boundary terms. This yields a frame-independent characterization of the propagating degrees of freedom and isolates a universal scalaron EFT in the metric branch, while clarifying the algebraic nature of the Palatini $f(R)$ scalar. We obtain, as a result, a frame-universal matching from the generic nonminimal couplings to a positive $R^2$ sector and a quantitative single-field attractor bound, enhanced by a $1/\Delta N$ selection term, providing sharp and falsifiable CMB targets.

Figures

Figures reproduced from arXiv: 2512.23401 by A. Sava\c{s} Arapo\u{g}lu, Cemal Berfu Senisik, Omer Guleryuz, Sermet \c{C}a\u{g}an.

Figure 1
Figure 1. Figure 1: FIG. 1. The commuting diagram of off-shell, local maps. [PITH_FULL_IMAGE:figures/full_fig_p002_1.png] view at source ↗
Figure 2
Figure 2. Figure 2: FIG. 2. The single-field stability map. The solid blue curve [PITH_FULL_IMAGE:figures/full_fig_p004_2.png] view at source ↗
Figure 3
Figure 3. Figure 3: FIG. 3. Stability map for the Linear-NMC Starobinsky model. The vertical axis is the NMC strength [PITH_FULL_IMAGE:figures/full_fig_p013_3.png] view at source ↗

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Reference graph

Works this paper leans on

57 extracted references · 25 linked inside Pith

  1. [1]

    A. A. Starobinsky, A New Type of Isotropic Cosmological Models Without Singularity, Phys. Lett. B91, 99 (1980)

  2. [2]

    Whitt, Fourth Order Gravity as General Relativity Plus Matter, Phys

    B. Whitt, Fourth Order Gravity as General Relativity Plus Matter, Phys. Lett. B145, 176 (1984)

  3. [3]

    Maeda, Towards the Einstein-Hilbert Action via Conformal Transformation, Phys

    K.-i. Maeda, Towards the Einstein-Hilbert Action via Conformal Transformation, Phys. Rev. D39, 3159 (1989)

  4. [5]

    De Felice and S

    A. De Felice and S. Tsujikawa, f(R) theories, Living Rev. Rel.13, 3 (2010), arXiv:1002.4928 [gr-qc]

  5. [6]

    Hubbard, Calculation of partition functions, Phys

    J. Hubbard, Calculation of partition functions, Phys. Rev. Lett.3, 77 (1959)

  6. [7]

    R. L. Stratonovich, On a Method of Calculating Quantum Distribution Functions, Soviet Physics Doklady2, 416 (1957)

  7. [8]

    G. W. Horndeski, Second-order scalar-tensor field equa- tions in a four-dimensional space, Int. J. Theor. Phys.10, 363 (1974)

  8. [9]

    Lovelock, The Einstein tensor and its generalizations, J

    D. Lovelock, The Einstein tensor and its generalizations, J. Math. Phys.12, 498 (1971)

  9. [10]

    Clifton, P

    T. Clifton, P. G. Ferreira, A. Padilla, and C. Skordis, Modified Gravity and Cosmology, Phys. Rept.513, 1 (2012), arXiv:1106.2476 [astro-ph.CO]

  10. [11]

    R. P. Woodard, Ostrogradsky’s theorem on Hamil- tonian instability, Scholarpedia10, 32243 (2015), arXiv:1506.02210 [hep-th]

  11. [12]

    Van Nieuwenhuizen, On ghost-free tensor lagrangians and linearized gravitation, Nucl

    P. Van Nieuwenhuizen, On ghost-free tensor lagrangians and linearized gravitation, Nucl. Phys. B60, 478 (1973)

  12. [13]

    Hinterbichler, Theoretical Aspects of Massive Gravity, Rev

    K. Hinterbichler, Theoretical Aspects of Massive Gravity, Rev. Mod. Phys.84, 671 (2012), arXiv:1105.3735 [hep-th]

  13. [14]

    K. S. Stelle, Renormalization of Higher Derivative Quan- tum Gravity, Phys. Rev. D16, 953 (1977)

  14. [15]

    K. S. Stelle, Classical Gravity with Higher Derivatives, Gen. Rel. Grav.9, 353 (1978)

  15. [16]

    T. P. Sotiriou and V. Faraoni, f(R) Theories Of Gravity, Rev. Mod. Phys.82, 451 (2010), arXiv:0805.1726 [gr-qc]

  16. [17]

    G. J. Olmo, Palatini Approach to Modified Gravity: f(R) Theories and Beyond, Int. J. Mod. Phys. D20, 413 (2011), arXiv:1101.3864 [gr-qc]

  17. [18]

    E. E. Flanagan, Palatini form of 1/R gravity, Phys. Rev. Lett.92, 071101 (2004), arXiv:astro-ph/0308111

  18. [19]

    Akramiet al.(Planck), Planck 2018 results

    Y. Akramiet al.(Planck), Planck 2018 results. X. Con- straints on inflation, Astron. Astrophys.641, A10 (2020), arXiv:1807.06211 [astro-ph.CO]

  19. [20]

    P. A. R. Adeet al.(BICEP, Keck), Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Ob- serving Season, Phys. Rev. Lett.127, 151301 (2021), arXiv:2110.00483 [astro-ph.CO]

  20. [21]

    Tokeshi and V

    K. Tokeshi and V. Vennin, Why Does Inflation Look Single Field to Us?, Phys. Rev. Lett.132, 251001 (2024), arXiv:2310.16649 [astro-ph.CO]

  21. [22]

    Deruelle and M

    N. Deruelle and M. Sasaki, Conformal equivalence in clas- sical gravity: the example of ’Veiled’ General Relativity, Springer Proc. Phys.137, 247 (2011), arXiv:1007.3563 [gr-qc]

  22. [23]

    Postma and M

    M. Postma and M. Volponi, Equivalence of the Einstein and Jordan frames, Phys. Rev. D90, 103516 (2014), arXiv:1407.6874 [astro-ph.CO]

  23. [24]

    J¨ arv, P

    L. J¨ arv, P. Kuusk, M. Saal, and O. Vilson, Invariant quantities in the scalar-tensor theories of gravitation, Phys. Rev. D91, 024041 (2015), arXiv:1411.1947 [gr-qc]

  24. [25]

    Hindawi, B

    A. Hindawi, B. A. Ovrut, and D. Waldram, Consistent spin two coupling and quadratic gravitation, Phys. Rev. D53, 5583 (1996), arXiv:hep-th/9509142

  25. [26]

    Hindawi, B

    A. Hindawi, B. A. Ovrut, and D. Waldram, Nontrivial vacua in higher derivative gravitation, Phys. Rev. D53, 5597 (1996), arXiv:hep-th/9509147

  26. [27]

    Magnano and L

    G. Magnano and L. M. Sokolowski, On physical equiv- alence between nonlinear gravity theories and a general relativistic selfgravitating scalar field, Phys. Rev. D50, 5039 (1994), arXiv:gr-qc/9312008

  27. [28]

    J. F. Donoghue and G. Menezes, Unitarity, stability and loops of unstable ghosts, Phys. Rev. D100, 105006 (2019), arXiv:1908.02416 [hep-th]

  28. [29]

    Anselmi and M

    D. Anselmi and M. Piva, The Ultraviolet Behavior of Quantum Gravity, JHEP05, 027, arXiv:1803.07777 [hep- th]

  29. [30]

    Adams, N

    A. Adams, N. Arkani-Hamed, S. Dubovsky, A. Nicolis, and R. Rattazzi, Causality, analyticity and an IR obstruction to UV completion, JHEP10, 014, arXiv:hep-th/0602178

  30. [31]

    X. O. Camanho, J. D. Edelstein, J. Maldacena, and A. Zhi- boedov, Causality Constraints on Corrections to the Gravi- ton Three-Point Coupling, JHEP02, 020, arXiv:1407.5597 [hep-th]

  31. [32]

    Cheung and G

    C. Cheung and G. N. Remmen, Positivity of Curvature- Squared Corrections in Gravity, Phys. Rev. Lett.118, 051601 (2017), arXiv:1608.02942 [hep-th]

  32. [33]

    F. W. Hehl, J. D. McCrea, E. W. Mielke, and Y. Ne’eman, Metric affine gauge theory of gravity: Field equations, Noether identities, world spinors, and breaking of di- lation invariance, Phys. Rept.258, 1 (1995), arXiv:gr- qc/9402012

  33. [34]

    W. J. Wolf, C. Garc ´ ıa-Garc ´ ıa, T. Anton, and P. G. Ferreira, Assessing Cosmological Evidence for Nonmin- imal Coupling, Phys. Rev. Lett.135, 081001 (2025), arXiv:2504.07679 [astro-ph.CO]

  34. [35]

    Doob, Conditional brownian motion and the bound- ary limits of harmonic functions, Bulletin de la Soci´ et´ e Math´ ematique de France85, 431 (1957)

    J. Doob, Conditional brownian motion and the bound- ary limits of harmonic functions, Bulletin de la Soci´ et´ e Math´ ematique de France85, 431 (1957)

  35. [36]

    Chetrite and H

    R. Chetrite and H. Touchette, Nonequilibrium markov processes conditioned on large deviations, Annales Henri Poincar´ e16, 2005 (2015)

  36. [37]

    Risken, Fokker-planck equation, inThe Fokker-Planck 6 Equation: Methods of Solution and Applications(Springer Berlin Heidelberg, Berlin, Heidelberg, 1996) pp

    H. Risken, Fokker-planck equation, inThe Fokker-Planck 6 Equation: Methods of Solution and Applications(Springer Berlin Heidelberg, Berlin, Heidelberg, 1996) pp. 63–95

  37. [38]

    Redner,A Guide to First-Passage Processes(Cam- bridge University Press, Cambridge, 2001)

    S. Redner,A Guide to First-Passage Processes(Cam- bridge University Press, Cambridge, 2001)

  38. [39]

    A. J. Bray, S. N. Majumdar, and G. Schehr, Persistence and first-passage properties in non-equilibrium systems, Advances in Physics62, 225 (2013)

  39. [40]

    Collet, S

    P. Collet, S. Mart ´ ınez, and J. Mart ´ ın,Quasi-Stationary Distributions: Markov Chains, Diffusions and Dynamical Systems, Probability and Its Applications (Springer Berlin Heidelberg, 2012)

  40. [41]

    Allyset al.(LiteBIRD), Probing Cosmic Inflation with the LiteBIRD Cosmic Microwave Background Polarization Survey, PTEP2023, 042F01 (2023), arXiv:2202.02773 [astro-ph.IM]

    E. Allyset al.(LiteBIRD), Probing Cosmic Inflation with the LiteBIRD Cosmic Microwave Background Polarization Survey, PTEP2023, 042F01 (2023), arXiv:2202.02773 [astro-ph.IM]

  41. [42]

    Abazajianet al.(CMB-S4), CMB-S4: Forecasting Con- straints on Primordial Gravitational Waves, Astrophys

    K. Abazajianet al.(CMB-S4), CMB-S4: Forecasting Con- straints on Primordial Gravitational Waves, Astrophys. J. 926, 54 (2022), arXiv:2008.12619 [astro-ph.CO]

  42. [43]

    Zwiebach, Curvature Squared Terms and String Theo- ries, Phys

    B. Zwiebach, Curvature Squared Terms and String Theo- ries, Phys. Lett. B156, 315 (1985)

  43. [44]

    D. J. Gross and J. H. Sloan, The Quartic Effective Action for the Heterotic String, Nucl. Phys. B291, 41 (1987)

  44. [45]

    E. A. Bergshoeff and M. de Roo, The Quartic Effective Action of the Heterotic String and Supersymmetry, Nucl. Phys. B328, 439 (1989)

  45. [46]

    R. R. Metsaev and A. A. Tseytlin, Order alpha-prime (Two Loop) Equivalence of the String Equations of Motion and the Sigma Model Weyl Invariance Conditions: De- pendence on the Dilaton and the Antisymmetric Tensor, Nucl. Phys. B293, 385 (1987)

  46. [47]

    M. B. Green and J. H. Schwarz, Anomaly Cancellation in Supersymmetric D=10 Gauge Theory and Superstring Theory, Phys. Lett. B149, 117 (1984)

  47. [48]

    Polchinski,String theory

    J. Polchinski,String theory. Vol. 2: Superstring theory and beyond, Cambridge Monographs on Mathematical Physics (Cambridge University Press, 2007)

  48. [49]

    Cecotti, Higher derivative supergravity is equivalent to standard supergravity coupled to matter, Phys

    S. Cecotti, Higher derivative supergravity is equivalent to standard supergravity coupled to matter, Phys. Lett. B 190, 86 (1987)

  49. [50]

    Ferrara, R

    S. Ferrara, R. Kallosh, A. Linde, A. Marrani, and A. Van Proeyen, Jordan Frame Supergravity and In- flation in NMSSM, Phys. Rev. D82, 045003 (2010), arXiv:1004.0712 [hep-th]

  50. [51]

    Higuchi, Forbidden Mass Range for Spin-2 Field Theory in De Sitter Space-time, Nucl

    A. Higuchi, Forbidden Mass Range for Spin-2 Field Theory in De Sitter Space-time, Nucl. Phys. B282, 397 (1987)

  51. [52]

    Deser and A

    S. Deser and A. Waldron, Gauge invariances and phases of massive higher spins in (A)dS, Phys. Rev. Lett.87, 031601 (2001), arXiv:hep-th/0102166. 7 APPENDIX: PROOFS AND DERIV A TIONS In this Appendix, we provide the detailed derivations supporting the main text. We assume D=4 with ( − + ++) signature and Φ > 0 to ensure well-defined Weyl maps. We denote to...

  52. [53]

    We prove this sector by sector

    Off–Shell Commutativity Theorem Our central claim is that the linearization of higher-derivative terms (via Hubbard–Stratonovich/Legendre lifts) and Weyl rescalings commute at the action level. We prove this sector by sector. General Linearization Setup We begin with the most general parity-even action quadratic in curvature and auxiliary fields. The ‘par...

  53. [54]

    The scalar disappears, leaving only the potential

    Einstein F rame:Under˜gµν = 2Φ M 2 Pl gµν, the kinetic term coefficient becomes 3+2 ωPal = 0. The scalar disappears, leaving only the potential. Nonminimal Couplings (NMC) For the NMC sector S = R √−g[ M 2 Pl 2 R + F (ϕ)R−V (ϕ)], we eliminate the fields ϕ algebraically. This is a Legendre-Fenchel transform: S= Z √−gfeff (R), f eff (R) = M 2 Pl 2 R+ sup ϕ ...

  54. [55]

    This supports the claim in Sec

    UniversalR 2 from Heavy Fields: Matching and Corrections Here we derive the effective field theory (EFT) generated by integrating out heavy scalar fields nonminimally coupled to gravity. This supports the claim in Sec. IV that generic UV sectors flow to theR 2 attractor. Set-up and Linearization Consider the generic Jordan-frame action withNscalarsϕ I : S...

  55. [56]

    This ensures the emergent scalaron has a healthy kinetic term

    Positivity:If the heavy sector is stable (( M 2)ab positive definite), then α′ NMC ≥ 0. This ensures the emergent scalaron has a healthy kinetic term

  56. [57]

    It is therefore independent of whether we perform the Weyl transformation before or after integrating out the heavy fields

    Universality:This matching relies only on local algebraic manipulations. It is therefore independent of whether we perform the Weyl transformation before or after integrating out the heavy fields. The Derivative Tower (R□R) To capture finite-mass effects, we retain the kinetic operator. The formal solution is δϕ = (M 2 −□)−1F R. Expanding the propagator f...

  57. [58]

    Single-Field Attractor: Geometry , Selection, and Isocurvature We analyze the stability of the inflationary valley in the Einstein frame (EF). The effective mass of entropic fluctuations is determined by three components: the intrinsic potential curvature, the kinematic turn rate, and the geometric ‘Weyl uplift’ induced by the frame transformation. 11 Ein...