Related estimates used together by the same construction modules.
The true heat-time evolution of Gaussian averaging on ordinary space.
The literal time derivative of the Gaussian density and local domination.
Time envelope, given by (15*t⁻¹*normalization (t/2))*Real.exp (-(4*t)⁻¹*‖y‖^2).
Equations
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Differentiating the explicit kernel under its ordinary Bochner integral.
Second average, given by ∑ i : Fin 3, average t (fun z => fderiv ℝ (fun y => fderiv ℝ f y (EuclideanSpace.single i 1)) z (EuclideanSpace.single i 1)) x.
Equations
- One or more equations did not get rendered due to their size.
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The explicit time-kernel integral equals one quarter of the sum of the actual second spatial derivatives averaged against the same Gaussian.
The low-frequency derivative of the true Gaussian average is controlled by the ordinary L² norm of the original field.
Low cost, given by Real.sqrt (8*normalization 1*(2:ℝ)^((3:ℝ)/2)).
Equations
- EulerWholeSpaceGaussian.lowCost = √(8 * EulerWholeSpaceGaussian.normalization 1 * 2 ^ (3 / 2))