REVIEW 2 major objections 5 minor 5 cited by
This paper establishes an infinite tower of two-sided positivity bounds that every effective field theory of heavy scalar fields on de Sitter must satisfy if it is to come from a unitary, causal UV completion.
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 14:19 UTC pith:SMPYQM3Y
load-bearing objection First analytic two-sided positivity bounds for in-in dS EFTs, but the pivotal Eq. (30) bridging moments to EFT coefficients is asserted without derivation. the 2 major comments →
Propagator positivity bounds for cosmological correlators
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
The paper's main result is a tower of two-sided positivity bounds, displayed in (24): for the EFT combinations g_n defined by the subtraction formula (30), one must have g_2 > 0, 0 < g_4/g_2 < g_3/g_2 < 1 and (g_3/g_2)^2 < g_4/g_2, at every order in the EFT expansion. These g_n are the positive moments of the spectral density ρ of the de Sitter self-energy after subtracting the dissipative (decay) part, which is why unitarity (ρ > 0) implies the inequalities. Because on de Sitter there is no mass gap — a light particle can decay into heavier particles — the usual Minkowski positivity of the coefficient c_2 is replaced by c_2 > ∫_{−Λ}^{Λ} dμ/(π μ) Im Σ(μ)/μ^4, with the H→0 limit recovering c_
What carries the argument
The central object is the Källén-Lehmann representation of the in-in (Bunch-Davies) self-energy, Σ(ν) = ∫ dμ'^2/π ρ(μ')/(μ'^2 − ν^2 − iε), with positive spectral density ρ = Im Σ > 0 enforcing unitarity and the prescribed analytic structure enforcing causality. Because the EFT must capture both the conservative and dissipative parts of the propagation, the paper doubles the fields (ϕ±) and writes the EFT self-energy as Σ_EFT(ν) = Σ_n (c_n + i γ_n tanh(πν)) ν^{2n}. The load-bearing identity is the subtraction formula g_n(Λ) = Λ^{2n} c_n − Σ_j 2Λ^{2j+1} γ'_j/(1 + 2j − 2n), which maps the physical EFT coefficients onto the positive spectral moments (28). It is the absence of a mass gap on de Si
Load-bearing premise
The subtraction formula (30), which converts the EFT coefficients c_n and γ_n into the positive moments g_n, is asserted without derivation; if this subtraction is incorrect or needs additional counterterms, the bounds (24) do not apply to the physical EFT coefficients.
What would settle it
Start from a unitary, causal UV completion (e.g. the ϕχ^2 bubble in d=3) and add a local counterterm that shifts c_2 by an arbitrary real constant while leaving the spectral density ρ unchanged. If for some counterterm value the combinations g_4/g_2 − (g_3/g_2)^2 or 1 − g_3/g_2 computed via (30) become negative, the bounds are violated by a healthy theory and (30) must be incomplete; alternatively, if every such shift keeps the combinations in the allowed leaf, the bounds survive this test.
If this is right
- EFT correlators that violate the inequalities (24) — for instance with (g_3/g_2)^2 > g_4/g_2 — cannot be produced by any unitary, causal UV completion, so they are ruled out as descriptions of an inflationary phase.
- In the flat-space limit H→0 the bounds reduce to the familiar Minkowski positivity c_n > 0; on de Sitter the sign of c_2 is instead controlled by the decay width via c_2 > ∫ dμ/(π μ) Im Σ(μ)/μ^4.
- In the squeezed bispectrum, the damping rate γ̃ of the oscillatory cosmological-collider signal is set by Im Σ, and the bounds translate into concrete restrictions on the non-oscillating EFT background — e.g. c_2 Λ^3 > −4γ̃/(3π) at leading order — so a measured decay rate forces a minimum size of background corrections.
- The in-in EFT has a radius of convergence set by the smallest mass difference (|ν|^2 = |μ1−μ2|^2 + d^2/4), not the lightest mass, so truncation errors at intermediate ν can be O(1) unless enough orders are kept — an explicit warning for EFT truncation in cosmology.
- Positivity of Σ(iα) for imaginary ν — an extra condition beyond the g_n bounds — implies the EFT background is always made larger by heavy physics in the squeezed limit, a distinct, testable prediction.
Where Pith is reading between the lines
- If the subtraction formula (30) fails for some UV completion with additional counterterms, the bounds would not apply to c_n and γ_n as stated; a complete proof (or a counterexample) of (30) would settle this and is a natural next step the paper does not take.
- The leaf-shaped allowed region for {g_3/g_2, g_4/g_2} is the seed of a de Sitter 'EFThedron'; adding further physical requirements (spin dominance, fixed spatial dimension d=3) is likely to shrink the allowed region and produce sharper bounds.
- Because the bounds tie the oscillatory and non-oscillatory parts of the bispectrum, they provide a direct falsifiable link between future measurements of primordial non-Gaussianity and the unitarity/causality of the underlying inflation model — a logical template that could extend to boost-breaking correlators if the spectral representation can be generalised.
- The numerical verification of (30) in tree, bubble and sunset examples is suggestive but not exhaustive; testing the bounds in a UV completion with a known local counterterm that changes c_2 without changing ρ would stress the subtraction scheme.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper constructs an in-in effective field theory for a light scalar field propagating on a fixed de Sitter background, with quadratic Wilson coefficients c_n (conservative) and γ_n (dissipative). Using a Källén-Lehmann representation for the self-energy with a positive spectral density, it defines cut-off moments g_n(Λ) and asserts a formula (Eq. (30)) relating these moments to the EFT coefficients. From positivity of the spectral density it derives two-sided moment inequalities (Eq. (24)) and states that any unitary/causal UV completion must produce EFT coefficients satisfying them. It then checks the bounds in explicit UV completions: tree-level mass mixing, a one-loop bubble, and a two-loop sunset, all using spectral densities from prior work. Finally it discusses implications for the cosmological collider signal, claiming that the damping rate of oscillations is tied to the non-oscillating EFT background.
Significance. If the central relation (30) is established, the paper would provide a genuinely new class of analytic positivity constraints on de Sitter EFTs, going beyond Minkowski bounds by explicitly incorporating the particle-production (dissipative) part of the self-energy. The claimed two-sided bounds constrain combinations of EFT coefficients that have not previously been bounded, and the connection to cosmological collider phenomenology is potentially impactful. The paper has real strengths: it uses a physically motivated Källén-Lehmann representation with positive spectral density, considers nontrivial UV completions with explicit spectral densities, and includes numerical verification of the inequalities as well as a careful discussion of when the EFT expansion breaks down. However, the bridge between the positive moments and the EFT coefficients—Eq. (30)—is asserted without derivation, and this is the load-bearing step for the main claim. The significance is therefore conditional on that gap being filled.
major comments (2)
- [§IV, Eq. (30)] Equation (30) is the only connection between the positive moments g_n(Λ) defined in (28) and the EFT coefficients c_n, γ'_n appearing in (15)/(19), yet it is introduced with the phrase 'we therefore have' and no derivation. Substituting the EFT spectral density (29) into the sub-Λ part of the moment integral yields integrals of the form ∫_0^{Λ^2} dµ'^2 ρ(µ')/µ'^{2n+2}, which are IR-divergent whenever 2j−2n+1≤0. Equation (30) is precisely what one obtains by discarding the divergent lower-limit contributions, i.e. by an analytic/minimal subtraction, but the paper does not state this prescription or specify the renormalization scheme in which the c_n of the action (15) are defined. Different IR regulators or finite counterterm choices shift c_n by scheme-dependent constants, and the inequalities (24) do not automatically survive such shifts. The UV-completion checks in §V are suggestive bu
- [§V.B] The EFT expansion (29) converges only for |ν| below the lowest singularity (e.g. for the bubble, |ν| ≲ 2μ in the d=2 example). For cut-offs Λ above that scale, the infinite sum in (30) diverges and cannot be used to compute g_n from the EFT coefficients. The text acknowledges this in footnote 76, but the abstract and §IV state that the bounds hold 'at every order in the EFT expansion' without this caveat. The distinction between bounds on the UV-defined g_n and bounds on the low-energy EFT coefficients must be made explicit in the main text; as written, a reader could apply (30) outside its domain of validity.
minor comments (5)
- [Eq. (1)] The illustrative bound in Eq. (1), c_2 > ∫_{-Λ}^{Λ} dµ/(πµ) ImΣ(µ)/µ^4, appears inconsistent with the bound derived later in §VI, c_2Λ^3 > −2γ'_0/3 + ... . The integral as written is IR-divergent and does not reduce to the stated combination. Please correct or clarify the intended expression.
- [Eqs. (28)–(30)] The notation for the spectral density is inconsistent: (28) integrates over dµ'^2 with ρ(µ'), while (29) defines ρ(ν) as a function of ν. The change of variables from µ' to ν should be stated explicitly, since the powers in (30) depend on this convention.
- [Figure 1] The caption says the bounds 'forbid EFT coefficients in the grey region', but the axes are ratios of g_n, which are nonlinear combinations of c_n and γ'_n via (30). Please clarify that the forbidden region is in the space of these g-combinations, not the bare Wilson coefficients.
- [Footnote 76] Footnote 76 states that Fig. 2 plots all values of Λ even when the EFT series (30) does not converge. It would be helpful to explain in the main text how g_n is obtained in that regime (presumably from the UV integral (28) directly), and to mark the region where the EFT calculation of (30) is valid.
- [General] There are several typos and minor grammatical issues: 'Kallen-Lehamnn' (should be Källén–Lehmann), 'analytiticity', 'phenoemonlogical', 'renormalisaiton'. These should be corrected in a final version.
Circularity Check
No significant circularity: the central bounds follow from an external Källén–Lehmann spectral representation; the self-citations are peripheral and Eq. (30), while terse, is an algebraic moment identity rather than a fitted input.
full rationale
The central derivation is not circular. The de Sitter Källén–Lehmann representation (25)-(26) is imported from prior work with no author overlap ([30,40,44,67-72]), and unitarity is converted into positivity Im Sigma > 0 inside this paper via (11)-(13). The EFT coefficients c_n, gamma_n are fixed by matching Sigma_EFT in (19) to the UV self-energy, not by fitting to any quantity that the bounds are then said to predict. The positive moments g_n in (28) are defined directly from the positive spectral density rho; Eq. (30) is the algebraic expression of those moments once the EFT expansion (29) is substituted. Even though (30) is asserted in a single sentence and its low-nu subtraction is formally divergent without an explicitly specified renormalization scheme, that is a derivation/scheme gap (a correctness risk), not a circular step: the bounds (24) are not equivalent to assuming (30), and the numerical UV completions in Sec. V are used as consistency checks, not to set constants. Self-citations appear but are peripheral: [41] (co-authored by Melville) supplies mode functions/vertex constants used in the phenomenological appendix, and [63] is cited for the elementary moment inequality g_{n+1}<g_n; neither supports the main positivity claim, which would stand if those citations were removed. Thus no prediction is a renamed fit and no load-bearing premise reduces to author self-citation. The score of 2 reflects one minor non-load-bearing self-citation in the appendix, not circularity of the central derivation.
Axiom & Free-Parameter Ledger
axioms (6)
- domain assumption dS Källén-Lehmann representation (25)-(26) with positive spectral density
- domain assumption Unitarity implies Im Σ(ν) > 0 for ν > 0
- domain assumption Causality implies Σ(ν) is analytic in the lower half ν-plane
- domain assumption In-in EFT action (15) with doubled fields and matching condition κ_n = γ_n (18)
- ad hoc to paper Subtraction formula (30): g_n = Λ^{2n} c_n − Σ_j 2Λ^{2j+1} γ'_j/(1+2j−2n)
- domain assumption Principal-series assumption (real μ, m^2 ≥ d^2/4)
read the original abstract
Using unitarity and causality, we derive an infinite tower of two-sided positivity bounds on the effective field theory coefficients which describe the propagation of heavy fields on de Sitter spacetime. We design this EFT to describe propagators with the in-in boundary conditions that are relevant for cosmological correlators. Our positivity bounds therefore identify EFT correlators that can never emerge from a consistent underlying model of inflation. This implies non-trivial constraints on primordial non-Gaussianity; for instance the cosmological collider oscillations in the squeezed bispectrum from the exchange of a heavy scalar are tied to the shape of its EFT background.
Figures
Forward citations
Cited by 5 Pith papers
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Alternatively, notice that the analytic structure of Σ implied by causality means we can express it as 1 2πi H ν dµ′ 2µ′Σ(µ′)/(µ′2 −ν 2 −iϵ) around the pole in the lower half of the complex plane, and then deform this contour so that it runs over R +∞ −∞ dµ′ and then change variables toµ ′2 to produce (26)
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In Figure 2 we have plotted all values of Λ to illustrate that our bounds are always satisfied, regardless of the EFT series (30) converging
Note that a low-energy observer can only deter- mineg n(Λ) from the EFT coefficients when Λ is below threshold, in this case Λ<2µ. In Figure 2 we have plotted all values of Λ to illustrate that our bounds are always satisfied, regardless of the EFT series (30) converging
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discussion (0)
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