Real quadratic mass in the shifted initial-time strip #
The shifted trace estimate is expressed as an ordinary space-time integral for the subsequent weighted cutoff estimate.
theorem
ESS.bu_short_shifted_real_trace_strip_tendsto_zero
(scale R : ℝ)
(hscale : 0 < scale)
(hscale1 : scale ≤ 1)
(hR : 0 < R)
(w : CKN.Foundation.Parabolic.ParabolicPoint → CKN.Foundation.Parabolic.Vec3)
(Dw : CKN.Foundation.Parabolic.ParabolicPoint → Fin 3 → CKN.Foundation.Parabolic.Vec3)
(D2w : CKN.Foundation.Parabolic.ParabolicPoint → Fin 3 → Fin 3 → CKN.Foundation.Parabolic.Vec3)
(Dtw : CKN.Foundation.Parabolic.ParabolicPoint → CKN.Foundation.Parabolic.Vec3)
(hcont : ContinuousOn w ({x : CKN.Foundation.Parabolic.Vec3 | 0 < x 2} ×ˢ Set.Ico 0 1))
(hinit : ∀ (x : CKN.Foundation.Parabolic.Vec3), 0 < x 2 → w (x, 0) = 0)
(hweak : CKN.HasSpaceTimeWeakDerivs {x : CKN.Foundation.Parabolic.Vec3 | 0 < x 2} (Set.Ioo 0 1) w Dw D2w Dtw)
(hL2 :
∀ S ⊆ CKN.spaceTimeSet {x : CKN.Foundation.Parabolic.Vec3 | 0 < x 2} (Set.Ioo 0 1),
Bornology.IsBounded S →
∫⁻ (z : CKN.Foundation.Parabolic.ParabolicPoint) in S, ‖Dw z‖ₑ ^ 2 + ‖D2w z‖ₑ ^ 2 + ‖Dtw z‖ₑ ^ 2 < ⊤)
:
Filter.Tendsto
(fun (ε : ℝ) =>
(∫ (q : CKN.Foundation.Parabolic.Vec3 × ℝ) in buShortTraceBall R ×ˢ Set.Ioc (1 / 2 + ε) (1 / 2 + 2 * ε), CKN.Foundation.Parabolic.vec3EuclideanNorm
(buAffineField (-scale ^ 2 / 2) scale w (CKN.Foundation.Parabolic.parabolicHomeomorph.symm q)) ^ 2) / ε ^ 2)
(nhdsWithin 0 (Set.Ioi 0)) (nhds 0)
The shifted field has vanishing normalized real quadratic mass on the bounded trace ball as its lower-time strip shrinks.