Kernel #
Part of the Caffarelli–Kohn–Nirenberg partial regularity proof.
The convolution variables are written explicitly so that the causal heat kernel and its spatial derivatives have one common interface.
Space-time displacement used as the argument of the translation-invariant heat kernel.
Instances For
noncomputable def
CKN.Core.HeatPotential.heatPotentialKernel
(w v : Foundation.Parabolic.ParabolicPoint)
:
Causal heat kernel evaluated at the space-time displacement of two points.
Equations
Instances For
noncomputable def
CKN.Core.HeatPotential.heatPotentialSpatialKernel
(i : Fin 3)
(w v : Foundation.Parabolic.ParabolicPoint)
:
Spatial derivative of the causal heat kernel at a space-time displacement.
Equations
- CKN.Core.HeatPotential.heatPotentialSpatialKernel i w v = CKN.Foundation.Heat.heatKernelSpaceDerivative (w.1 - v.1) (w.2 - v.2) i
Instances For
noncomputable def
CKN.Core.HeatPotential.heatPotential
(F : Foundation.Parabolic.ParabolicPoint → ℝ)
(G : Fin 3 → Foundation.Parabolic.ParabolicPoint → ℝ)
(w : Foundation.Parabolic.ParabolicPoint)
:
Heat potential of a scalar source and spatial divergence sources.
Equations
- One or more equations did not get rendered due to their size.
Instances For
theorem
CKN.Core.HeatPotential.heatPotentialKernel_abs_le
{w v : Foundation.Parabolic.ParabolicPoint}
{R : ℝ}
(hR : 0 < R)
(hsep : R ≤ Foundation.Heat.rhoTwo (w.1 - v.1) (w.2 - v.2))
:
theorem
CKN.Core.HeatPotential.heatPotentialSpatialKernel_abs_le
{i : Fin 3}
{w v : Foundation.Parabolic.ParabolicPoint}
{R : ℝ}
(hR : 0 < R)
(hsep : R ≤ Foundation.Heat.rhoTwo (w.1 - v.1) (w.2 - v.2))
:
theorem
CKN.Core.HeatPotential.heatPotentialSpatialTimeKernel_abs_le
{i : Fin 3}
{w v : Foundation.Parabolic.ParabolicPoint}
{R : ℝ}
(hR : 0 < R)
(hsep : R ≤ Foundation.Heat.rhoTwo (w.1 - v.1) (w.2 - v.2))
: