Blowup Energy Density #
Local energy bounds for the rescaled sequence in the endpoint regularity argument.
theorem
ESS.blowupEnergyCutoff_localEnergyRhs_le
(R : ℝ)
(hR : 0 < R)
:
∃ (C : ℝ),
0 ≤ C ∧ ∀ (a b : ℝ),
b < 0 →
∀ (u : CKN.Foundation.Parabolic.Vec3 × ℝ → CKN.Foundation.Parabolic.Vec3)
(p : CKN.Foundation.Parabolic.Vec3 × ℝ → ℝ) (z : CKN.Foundation.Parabolic.Vec3 × ℝ),
CKN.localEnergyRhs u p 0 (blowupEnergyCutoff R a b) z ≤ CKN.Foundation.Parabolic.vec3EuclideanNorm (u z) ^ 2 * (8 + 3 * C) + |CKN.Foundation.Parabolic.vec3EuclideanNorm (u z) ^ 2 + 2 * p z| * (3 * C * CKN.Foundation.Parabolic.vec3EuclideanNorm (u z))
The local-energy right-hand density for the fixed spatial cutoff is bounded by the velocity and pressure densities with one coefficient that does not depend on the upper time cutoff.
theorem
ESS.blowupEnergyCutoff_localEnergyRhs_power_le
(R : ℝ)
(hR : 0 < R)
:
∃ (C : ℝ),
0 ≤ C ∧ ∀ (a b : ℝ),
b < 0 →
∀ (u : CKN.Foundation.Parabolic.Vec3 × ℝ → CKN.Foundation.Parabolic.Vec3)
(p : CKN.Foundation.Parabolic.Vec3 × ℝ → ℝ) (z : CKN.Foundation.Parabolic.Vec3 × ℝ),
CKN.localEnergyRhs u p 0 (blowupEnergyCutoff R a b) z ≤ (8 + 3 * C) * CKN.Foundation.Parabolic.vec3EuclideanNorm (u z) ^ 2 + 3 * C * CKN.Foundation.Parabolic.vec3EuclideanNorm (u z) ^ 3 + 6 * C * |p z| * CKN.Foundation.Parabolic.vec3EuclideanNorm (u z)
The same density bound in the power form used with slice L³ and
pressure L^(3/2) estimates.