Partial Differential Equations

Hello and welcome to my ongoing video course about Partial Differential Equations, already consisting of 16 videos. The video series is called Partial Differential Equations (PDEs). The course it’s not finished yet. This course builds on the foundation laid in the Ordinary Differential Equations (ODEs) series, expanding into the more complex and multi-dimensional world of PDEs. Alongside the videos, you’ll find additional text explanations to help reinforce the material. To test your knowledge, use the quizzes, and refer to the PDF versions of the lessons whenever needed. If you have any questions, feel free to participate in the community discussion forum. Without further ado, let’s get started!

Part 1 - Introduction and Definition

Let’s start the video series with some basic notions we will use throughout the course. For example, we have to know what we mean by a partial differential equation and a classical solution of it.


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Part 2 - Laplace’s Equation

One of the most important partial differential equations is Laplace’s equation where the solutions are called harmonic fucntions. We will try to find solutions that respect the radial symmetry because these can be used a base for the construcion of other solutions.


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Part 3 - Fundamental Solution of Laplace’s Equation

The fundamental solution for Laplace’s equation is sometimes also called Newtonian kernel because of its application in physics. Indeed, in three dimensions, we have $\gamma(x) = \frac{1}{4 \pi} \frac{1}{\| x \|}$ for the fundamental solution. Obviously, there is a singularity at the origin, but it turns out that inside an integral it is no problem at all. Let’s show that for an arbitrary dimension $n$ as well.


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Part 4 - Mean-Value Property of Harmonic Functions

The solutions of Laplace’s equation have some nice properties that can be surpring. For example, we can show that the values of the function at a point is already determined by the values of the function on a sphere around this point. This is what we mean by the mean-value property of a function. Let’s prove this by using Green’s identity and the fact that we can move a derivative inside the integral under our assumptions here.


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Part 5 - Maximum Principle for Harmonic Functions

A direct consequence of the mean-value property of harmonic functions is the so-called maximum principle. It roughly says that the maximum of any harmonic function $u : \Omega \rightarrow \mathbb{R}$ is always found on the boundary $\partial \Omega$. We can even distiguish a strong and weak maximum principle depending if we have a connected set $\Omega$ or not.


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Part 6 - Proof of Maximum Principle

Let’s prove the two statements from the last video. We will need some topology knowledge for connected sets, which you can find in the Basic Topology course. In particular, we can use from there that path-connected sets are also connected. Therefore, we will first show the strong maximum principle and use it to prove the weak maximum principle.


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Part 7 - Uniqueness of the Boundary Value Problem for Poisson’s Equation

We can generalize our the important PDE given by Laplace’s equation to Poisson’s equation by changing the right-hand side to a continuous function $f$. So we search for functions $u$ where the Laplacian $\Delta u$ is given by $f$ on the whole open domain $\Omega$. Now, if we also claim that $u$ should be equal to a continuous function $g$ on the boundary $\partial \Omega$, then we speak of a boundary-value problem. In particular, in this case, we have so-called Dirichlet boundary conditions. It turns out that such a boundary-value problem on a bounded set $\Omega$ has at most one solution, so we definitely have uniqueness if a solution exists. As we will show in the video, this property immediately follows from the maximum principle for harmonic functions.


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Part 8 - Standard Mollifier

In the following, we will discuss a common tool in analysis known as the standard mollifier, which can be used to smoothen continuous functions. One uses an exponential functions to define a $C^\infty$-function with compact support. By scaling it appropriately, we get a so-called Dirac sequence that can be used to approximate the original function. Let’s discuss how that works in detail for a function $u : \Omega \rightarrow \mathbb{R}$, where $\Omega$ is an open set in $\mathbb{R}^n$.


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Part 9 - Regularity of Harmonic Functions

The next topic about regularity means that the solutions of Laplace’s equation are much smoother than what the formal equation requires. Instead of $C^2$-functions, we actually get $C^\infty$-functions out.


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Part 10 - Liouville’s Theorem for Harmonic Functions

You might already know Liouville’s theorem for holomorphic functions from Complex Analysis. In fact, the following discussion is a generalization of this result. We will show that every harmonic function defined on the whole space $\mathbb{R}^n$ is either constant or unbounded. The key ingredient for the proof is to have an estimate for the partial derivatives of a harmonic function defined on a ball.


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Part 11 - Normal Derivative of Newtonian Kernel

Our goal is to solve Poisson’s equation $\Delta u = f$ for a given function $f$. It will turn out that the fundamental solution of Laplace’s equation, denoted by $\gamma$ plays the key role there. However, in order to use it correctly, we first have to check some properties of it. Let’s start with the normal derivative of $\gamma$ at the sphere.


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Part 12 - Properties of Newtonian Kernel

We can easily extend the result from the last video to get a property that looks like something we could call delta function. It just means that in a limit process of an integral, we get the value of a function at a given point. This is a nice property of the normal derivative on the sphere and we will use it to find a representation formula for general $C^2$-functions that could be used to solve Poisson’s equation. But let’s first prove this property.


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Part 13 - Representation Formula for Poisson’s Equation

The following representation formula that holds for any $C^2$-functions $u$ is quite interesting. The singularity of $\gamma$ allows to write each value $u(x_0)$ as a combination of a surface integral with a volume integral as long as the point $x_0$ lies inside the domain of the volume integral. Furthermore, for harmonic functions, this representation formula becomes even shorter.


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Part 14 - Newtonian Potential

In this video, we will finally construct a solution of Poisson’s equation. We can do it by using the convolution with the fundamental solution of Laplace’s equation. This function $\gamma \ast f$ is often called Newtonian potential because of the historical usage of the gravitational potential. However, it also occurs as the Coulomb potential in electrostatics. We will also show that this solution of Poisson’s equation is unique if we assume that the solution vanishes at infinity.


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Part 15 - Green’s Function

Let’s go back to the boundary-value problem for Poisson’s equation with Dirichlet boundary conditions. This means that we have two continuous functions $f$ and $g$, where $f$ is on the right of Poisson’s equation and $g$ should give the boundary values of the solution. It turns out that our representation formula for $C^2$-functions almost already catches that problem. We just have get rid of the normal derivative of the solution. This is what can be done by Green’s function, which we can define for every open subset $\Omega \subseteq \mathbb{R}^n$.


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Part 16 - Symmetry Property of Green’s Function

Let’s look at Green’s function more closely. The definition is completely different in the two variables $x$ and $y$ in the function $G(x,y)$. However, we can still show that we the function is symmetric if we concentrate on points in $\Omega$ that don’t coincide. The proof is similar to the proof of the representation formulas we have done before.


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Connections to other courses


Summary of the course Partial Differential Equations


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