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Eq. (4.9): −fNL=53A4∑iki3=−512(ns+f(k)nt)-f_{NL} = \frac53\frac{\mathcal A}{4\sum_ik_i^3} = -\frac{5}{12}(n_s+f(k)n_t)−fNL​=35​4∑i​ki3​A​=−125​(ns​+f(k)nt​)

Proved
Maldacena2003.fNL_eq_tilts

by Lucas · Oct 12, 2026 · Mathlib 0df444a (Lean v4.33.1)

cosmologyinflationmathematical-physics

Let ρ˙∗>0\dot\rho_*>0ρ˙​∗​>0, ϕ˙∗≠0\dot\phi_*\neq0ϕ˙​∗​=0, ϕ¨∗\ddot\phi_*ϕ¨​∗​ real, and let (k1,k2,k3)(k_1,k_2,k_3)(k1​,k2​,k3​) be a momentum triangle with positive sides. Then

53 A4∑iki3  =  512[2ϕ¨∗ϕ˙∗ρ˙∗+ϕ˙∗2ρ˙∗2(2+f(k))]  =  −512(ns+f(k) nt),\frac53\,\frac{\mathcal A}{4\sum_ik_i^3} \;=\; \frac{5}{12}\Big[2\frac{\ddot\phi_*}{\dot\phi_*\dot\rho_*}+\frac{\dot\phi_*^2}{\dot\rho_*^2}\big(2+f(k)\big)\Big] \;=\; -\frac{5}{12}\big(n_s+f(k)\,n_t\big),35​4∑i​ki3​A​=125​[2ϕ˙​∗​ρ˙​∗​ϕ¨​∗​​+ρ˙​∗2​ϕ˙​∗2​​(2+f(k))]=−125​(ns​+f(k)nt​),

where A\mathcal AA is the amplitude (4.6), f(k)f(k)f(k) is the shape function of (4.9), and nsn_sns​, ntn_tnt​ are the scalar and tensor tilts (2.22), (2.30).

This expresses the paper's kkk-dependent fNLf_{NL}fNL​ through the two observable tilts and a purely geometric shape function of the momentum triangle.

Formalization Note The shape function shapeF is defined so that the first equality holds. The content of the statement is the consistency of that definition with A\mathcal AA and the second equality with the tilts.

Preamble
import Mathlib
import Definitions.Def_Maldacena2003_InflationDefs
open Filter Topology
Formal statement
namespace Maldacena2003

theorem fNL_eq_tilts (ρd φd φdd k₁ k₂ k₃ : ℝ) (hρ : 0 < ρd) (hφ : φd ≠ 0)
    (hk : IsMomentumTriangle k₁ k₂ k₃) :
    (5 / 3) * (amplitudeA ρd φd φdd k₁ k₂ k₃ / (4 * (k₁ ^ 3 + k₂ ^ 3 + k₃ ^ 3)))
        = (5 / 12) * (2 * (φdd / (φd * ρd)) + φd ^ 2 / ρd ^ 2 * (2 + shapeF k₁ k₂ k₃)) ∧
      (5 / 12) * (2 * (φdd / (φd * ρd)) + φd ^ 2 / ρd ^ 2 * (2 + shapeF k₁ k₂ k₃))
        = -(5 / 12) * (scalarTilt ρd φd φdd + shapeF k₁ k₂ k₃ * tensorTilt ρd φd) := by sorry

end Maldacena2003
Source
J. Maldacena, Non-Gaussian features of primordial fluctuations in single field inflationary models, JHEP 05 (2003) 013, https://doi.org/10.1088/1126-6708/2003/05/013 (arXiv:astro-ph/0210603), p. 18, eq. (4.9)
Human review
  • Endorsed by Shuze Chen · Oct 13, 2026

    Confirmed by the moderator at approval.

  • Endorsed by Lucas · Oct 13, 2026

    Confirmed by the mission captain (proposal self-audit).

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