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Anderson4D.Continuum.GreenDerivatives

Derivatives of the local Euclidean part of the Green kernel #

The singular summand of the periodized Bessel kernel is the k = 0 Euclidean heat kernel. This file differentiates that summand under its time integral. The resulting first- and second-coordinate derivative formulas, together with explicit |x|⁻³ and |x|⁻⁴ majorants, are the singular part of paper (4.1).

noncomputable def Anderson4D.euclideanBessel4 (x : R4) :

The k = 0 Euclidean contribution to the Bessel Green kernel.

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    noncomputable def Anderson4D.euclideanHeatGrad (t : ℝ) (x : R4) (i : Fin dim) :

    Coordinate derivative of the Euclidean heat kernel.

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      noncomputable def Anderson4D.euclideanHeatHess (t : ℝ) (x : R4) (i j : Fin dim) :

      Coordinate Hessian entry of the Euclidean heat kernel.

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        noncomputable def Anderson4D.euclideanBesselGrad (x : R4) (i : Fin dim) :

        First-coordinate derivative candidate after the Bessel time integral.

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          noncomputable def Anderson4D.euclideanBesselHess (x : R4) (i j : Fin dim) :

          Coordinate Hessian candidate after the Bessel time integral.

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            noncomputable def Anderson4D.greenLocalLift (x : R4) :

            The Green function pulled back along the coordinatewise quotient ℝ⁴ → 𝕋⁴. On the principal cube its singular summand is euclideanBessel4.

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              noncomputable def Anderson4D.greenLocalPoint (x : R4) :

              Coordinatewise quotient point associated with a Euclidean lift.

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                noncomputable def Anderson4D.greenLocalRemainder (x : R4) :

                The regular part left after removing the local Euclidean Bessel summand from the pulled-back torus Green function.

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                  On the principal cube, the Euclidean heat kernel is exactly the zero lattice summand of the heat kernel defining greenLocalLift.

                  The local Euclidean heat kernel is a genuine summand, rather than an auxiliary comparison kernel: it is bounded by the periodized heat kernel whose Bessel integral defines greenFn.

                  def Anderson4D.coordLine (x : R4) (i : Fin dim) (s : ℝ) :

                  Coordinate line through a Euclidean lift.

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                    theorem Anderson4D.hasDerivAt_euclideanHeatKernel4_coord_at {t : ℝ} (ht : t ≠ 0) (x : R4) (i : Fin dim) (s : ℝ) :
                    HasDerivAt (fun (r : ℝ) => euclideanHeatKernel4 t (coordLine x i r)) (euclideanHeatGrad t (coordLine x i s) i) s
                    theorem Anderson4D.hasDerivAt_euclideanHeatGrad_coord {t : ℝ} (ht : t ≠ 0) (x : R4) (i j : Fin dim) :
                    HasDerivAt (fun (s : ℝ) => euclideanHeatGrad t (coordLine x j s) i) (euclideanHeatHess t x i j) 0
                    theorem Anderson4D.hasDerivAt_euclideanHeatGrad_coord_at {t : ℝ} (ht : t ≠ 0) (x : R4) (i j : Fin dim) (s : ℝ) :
                    HasDerivAt (fun (r : ℝ) => euclideanHeatGrad t (coordLine x j r) i) (euclideanHeatHess t (coordLine x j s) i j) s
                    theorem Anderson4D.abs_euclideanHeatGrad {t : ℝ} (ht : 0 < t) (x : R4) (i : Fin dim) :
                    |euclideanHeatGrad t x i| = |x i| / (32 * Real.pi ^ 2) * ((t ^ 3)⁻¹ * Real.exp (-(euclideanDistSq x / 4 / t)))
                    theorem Anderson4D.abs_euclideanHeatHess_le {t : ℝ} (ht : 0 < t) (x : R4) (i j : Fin dim) :
                    |euclideanHeatHess t x i j| ≤ |x i * x j| / (64 * Real.pi ^ 2) * ((t ^ 4)⁻¹ * Real.exp (-(euclideanDistSq x / 4 / t))) + 1 / (32 * Real.pi ^ 2) * ((t ^ 3)⁻¹ * Real.exp (-(euclideanDistSq x / 4 / t)))
                    theorem Anderson4D.integral_abs_euclideanHeatHess_le {x : R4} (hx : euclideanDistSq x ≠ 0) (i j : Fin dim) :
                    ∫ (t : ℝ) in Set.Ioi 0, |euclideanHeatHess t x i j| ≤ |x i * x j| / (64 * Real.pi ^ 2) * (2 * (euclideanDistSq x / 4)⁻¹ ^ 3) + 1 / (32 * Real.pi ^ 2) * (euclideanDistSq x / 4)⁻¹ ^ 2

                    The k = 0 Bessel contribution is genuinely differentiable in every coordinate away from its singular point, with derivative obtained by differentiating the heat kernel under the time integral.

                    Explicit |x|⁻³-scale bound for each coordinate derivative of the local Bessel contribution. The anisotropic numerator is useful in the later Taylor contraction and is exactly the time-integrated Gaussian bound.

                    The time-integrated first derivative is itself differentiable away from the singularity; its coordinate derivative is the time-integrated Hessian. This is the genuine k = 2 local Bessel part of (4.1).

                    theorem Anderson4D.abs_euclideanBesselHess_le {x : R4} (hx : euclideanDistSq x ≠ 0) (i j : Fin dim) :
                    |euclideanBesselHess x i j| ≤ |x i * x j| / (64 * Real.pi ^ 2) * (2 * (euclideanDistSq x / 4)⁻¹ ^ 3) + 1 / (32 * Real.pi ^ 2) * (euclideanDistSq x / 4)⁻¹ ^ 2

                    Explicit |x|⁻⁴-scale anisotropic majorant for every Hessian entry of the local Bessel contribution.