OAI/Geometry/RCD/Heat/DyadicTimeIntegral.lean

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2 declarations, 0 contain sorry, 0 declared as axioms

Finite dyadic time decomposition for actual integrable sources

  1. theorem OAI.RegularPointCoordinates.dyadic_time_integral_eq_sum line 17

    Source documentation

    Consecutive dyadic time blocks telescope exactly. Integrability is explicit, so no use is made of the undefined-integral zero convention.

    theorem dyadic_time_integral_eq_sum (f : ℝ → ℝ) {R : ℝ} (hR : 0 < R) (i : ℕ)
        (hf : IntervalIntegrable f volume ((R / (2 : ℝ) ^ i) ^ 2) (R ^ 2)) :
        (∫ t in (R / (2 : ℝ) ^ i) ^ 2..R ^ 2, f t) =
          ∑ j ∈ Finset.range i, ∫ t in (R / (2 : ℝ) ^ j) ^ 2 / 4..(R / (2 : ℝ) ^ j) ^ 2, f t := by
    …
  2. theorem OAI.RegularPointCoordinates.dyadic_time_integral_abs_le line 43

    Source documentation

    A bound on each actual block gives the corresponding finite weighted sum on the entire long-time interval.

    theorem dyadic_time_integral_abs_le (f : ℝ → ℝ) {R : ℝ} (hR : 0 < R) (i : ℕ)
        (hf : IntervalIntegrable f volume ((R / (2 : ℝ) ^ i) ^ 2) (R ^ 2))
        (B : ℕ → ℝ) (hb : ∀ j < i,
          |∫ t in (R / (2 : ℝ) ^ j) ^ 2 / 4..(R / (2 : ℝ) ^ j) ^ 2, f t| ≤ B j) :
        |∫ t in (R / (2 : ℝ) ^ i) ^ 2..R ^ 2, f t| ≤ ∑ j ∈ Finset.range i, B j := by
    …