Blowup Time AE #
Almost-everywhere time-slice bounds used in endpoint compactness.
theorem
ESS.blowupTimeExtendedPressure_aestronglyMeasurable
(p₁ : CKN.Foundation.Parabolic.ParabolicPoint → ℝ)
(hp₁ : MeasureTheory.AEStronglyMeasurable p₁ (MeasureTheory.volume.restrict (Set.univ ×ˢ Set.Ioo (-1) 0)))
:
Zero extension in time preserves joint strong measurability of a whole-space pressure.
theorem
ESS.blowupRieszPressure_aestronglyMeasurable
(p₁ : CKN.Foundation.Parabolic.ParabolicPoint → ℝ)
(hp₁ : MeasureTheory.AEStronglyMeasurable p₁ (MeasureTheory.volume.restrict (Set.univ ×ˢ Set.Ioo (-1) 0)))
(x₀ : CKN.Foundation.Parabolic.Vec3)
(t₀ r : ℝ)
(hr : 0 < r)
:
The rescaled whole-space pressure remains jointly strongly measurable.
theorem
ESS.blowup_ae_time_pullback
(r t₀ : ℝ)
(hr : 0 < r)
(I : Set ℝ)
(hI : MeasurableSet I)
(P : ℝ → Prop)
(hP : ∀ᵐ (s : ℝ) ∂MeasureTheory.volume.restrict I, P s)
:
∀ᵐ (t : ℝ) ∂MeasureTheory.volume.restrict (CKN.rescaledTime r t₀ I), P (CKN.scalingTime r t₀ t)
An almost everywhere source-time property pulls back through a positive parabolic time rescaling.
theorem
ESS.blowup_ae_time_pullback_on
(r t₀ : ℝ)
(hr : 0 < r)
(I J : Set ℝ)
(hI : MeasurableSet I)
(hJ : J ⊆ CKN.rescaledTime r t₀ I)
(P : ℝ → Prop)
(hP : ∀ᵐ (s : ℝ) ∂MeasureTheory.volume.restrict I, P s)
:
∀ᵐ (t : ℝ) ∂MeasureTheory.volume.restrict J, P (CKN.scalingTime r t₀ t)
The pulled-back property also holds on every smaller rescaled time interval.
theorem
ESS.blowupRieszPressure_slice_bound_ae
(p₁ : CKN.Foundation.Parabolic.ParabolicPoint → ℝ)
(x₀ : CKN.Foundation.Parabolic.Vec3)
(t₀ r : ℝ)
(hr : 0 < r)
(J : Set ℝ)
(hJmeas : MeasurableSet J)
(hJ : J ⊆ CKN.rescaledTime r t₀ (Set.Ioo (-1) 0))
(M : ENNReal)
(hsource :
∀ᵐ (s : ℝ) ∂MeasureTheory.volume.restrict (Set.Ioo (-1) 0), MeasureTheory.AEStronglyMeasurable (fun (x : CKN.Foundation.Parabolic.Vec3) => p₁ (x, s)) MeasureTheory.volume ∧ MeasureTheory.eLpNorm (fun (x : CKN.Foundation.Parabolic.Vec3) => p₁ (x, s)) (3 / 2) MeasureTheory.volume ≤ M)
:
∀ᵐ (t : ℝ) ∂MeasureTheory.volume.restrict J, MeasureTheory.eLpNorm (fun (x : CKN.Foundation.Parabolic.Vec3) => blowupRieszPressure x₀ t₀ r p₁ (x, t)) (3 / 2)
MeasureTheory.volume ≤ M
A source-time uniform whole-space pressure bound persists on a rescaled past time interval contained in the source interval.
theorem
ESS.blowupRieszPressure_time_threeHalves_bound
(p₁ : CKN.Foundation.Parabolic.ParabolicPoint → ℝ)
(x₀ : CKN.Foundation.Parabolic.Vec3)
(t₀ r : ℝ)
(hr : 0 < r)
(J : Set ℝ)
(hJmeas : MeasurableSet J)
(hJ : J ⊆ CKN.rescaledTime r t₀ (Set.Ioo (-1) 0))
(M : ENNReal)
(hsource :
∀ᵐ (s : ℝ) ∂MeasureTheory.volume.restrict (Set.Ioo (-1) 0), MeasureTheory.AEStronglyMeasurable (fun (x : CKN.Foundation.Parabolic.Vec3) => p₁ (x, s)) MeasureTheory.volume ∧ MeasureTheory.eLpNorm (fun (x : CKN.Foundation.Parabolic.Vec3) => p₁ (x, s)) (3 / 2) MeasureTheory.volume ≤ M)
:
∫⁻ (t : ℝ) in J, MeasureTheory.eLpNorm (fun (x : CKN.Foundation.Parabolic.Vec3) => blowupRieszPressure x₀ t₀ r p₁ (x, t)) (3 / 2)
MeasureTheory.volume ^ (3 / 2) ≤ MeasureTheory.volume J * M ^ (3 / 2)
A uniform source-time pressure bound controls the time-integrated
rescaled L^(3/2) norm.
theorem
ESS.blowupRieszPressure_spaceTime_mass_bound
(p₁ : CKN.Foundation.Parabolic.ParabolicPoint → ℝ)
(hp₁ : MeasureTheory.AEStronglyMeasurable p₁ (MeasureTheory.volume.restrict (Set.univ ×ˢ Set.Ioo (-1) 0)))
(x₀ : CKN.Foundation.Parabolic.Vec3)
(t₀ r : ℝ)
(hr : 0 < r)
(J : Set ℝ)
(hJmeas : MeasurableSet J)
(hJ : J ⊆ CKN.rescaledTime r t₀ (Set.Ioo (-1) 0))
(M : ENNReal)
(hsource :
∀ᵐ (s : ℝ) ∂MeasureTheory.volume.restrict (Set.Ioo (-1) 0), MeasureTheory.AEStronglyMeasurable (fun (x : CKN.Foundation.Parabolic.Vec3) => p₁ (x, s)) MeasureTheory.volume ∧ MeasureTheory.eLpNorm (fun (x : CKN.Foundation.Parabolic.Vec3) => p₁ (x, s)) (3 / 2) MeasureTheory.volume ≤ M)
:
∫⁻ (z : CKN.Foundation.Parabolic.Vec3 × ℝ), ENNReal.ofReal |blowupRieszPressure x₀ t₀ r p₁ z| ^ (3 / 2) ∂(MeasureTheory.volume.restrict Set.univ).prod (MeasureTheory.volume.restrict J) ≤ MeasureTheory.volume J * M ^ (3 / 2)
The rescaled whole-space pressure has a uniform space-time
L^(3/2) mass bound on a past time interval.