The Fundamental Solution of Heat Equation #
This file formalizes the properties of the heat kernel and its convolution solution following Rustom Choksi's Partial Differential Equations book (Chapter 7.2.2).
We establish:
- Regularity properties (continuity and measurability).
- $L^\infty$ bounds and decay estimates essential for dominated convergence.
- Integrability of the kernel and its derivatives against a function $g$.
- differentiation under the integral sign to prove the convolution solves the heat equation.
Reference #
This formalization follows Chapter 7.2.2, "Partial Differential Equations, A First Course" by Professor Rustom Choksi.
1. Definitions and Derivative Shorthands #
We define the convolution of the heat kernel with a function $g$ and introduce shorthand notation for the partial derivatives of the heat kernel.
The convolution of the heat kernel with an initial data function g.
Equations
- Heat.heatConvolutionHK α g x t = ∫ (y : ℝ), Heat.heatKernel α (x - y) t * g y
Instances For
2. Explicit Derivative Formulas #
We use the explicit calculations of the derivatives of the Heat Kernel from the
previous chapter and make them consistent with the notation HKt, HKx, HKxx
3. Regularity: Continuity and Measurability #
Here we establish that the heat kernel and its derivatives are continuous and strongly measurable functions. These properties are mainly used here as a prerequisite to showing that the solution formula indeed solves the heat equation, which requires us to differentiate under the integral.
4. Pointwise Bounds and L-infinity Estimates #
We define bounding constants K, Kx, Kxx and for the heat kernel's derivatives.
This implies they belong to $L^\infty$.
5. Integrability of the Kernels #
We demonstrate that the heat kernel and its derivatives are integrable when multiplied by an integrable function $g$
6. Differentiation under the Integral Sign #
We establish the validity of swapping the integral and derivative operators. This requires checking the Dominated Convergence Theorem conditions using the bounds established in Section 4.
Swap the time derivative $\partial_t$ with the integral $\int$.
Swap the spatial derivative $\partial_x$ with the integral $\int$.
Swap the second spatial derivative $\partial_{xx}$ with the integral $\int$.
7. Main Result: The Heat Equation #
Finally, we combine the pointwise heat equation property of the kernel with the differentiation-under-integral results to show that the convolution $u(x,t) = (K * g)(x)$ solves the heat equation $u_t = \alpha u_{xx}$.