Nonlinear finite elements/Partial differential equations

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Partial differential equations (PDEs) are the most common method by which we model physical problems in engineering. Finite element methods are one of many ways of solving PDEs. This handout reviews the basics of PDEs and discusses some of the classes of PDEs in brief. The contents are based on Partial Differential Equations in Mechanics volumes 1 and 2 by A.P.S. Selvadurai and Nonlinear Finite Elements of Continua and Structures by T. Belytschko, W.K. Liu, and B. Moran.

Definition of a PDE

A PDE is a relationship between an unknown function of several variables and its partial derivatives.

Let u(x_1, x_2, x_3, t) be an unknown function. The independent variables are x_1, x_2, x_3, and t. We usually write


    u = u(x_1, x_2, x_3, t)

and say that u is the dependent variable.

Partial derivatives are denoted by expressions such as


    u_{,1} = \frac{\partial u}{\partial x_1} ~;~~  
    u_{,2} = \frac{\partial u}{\partial x_2} ~;~~  
    u_{,11} = \frac{\partial^2 u}{\partial x_1\partial x_1} \equiv \frac{\partial^2 u}{\partial x_1^2} ~;~~  
    u_{,12} = \frac{\partial^2 u}{\partial x_1\partial x_2}~.

Some examples of partial differential equations are

\begin{align}
    u_{,t} = u_{,1} + u_{,2} &\Leftrightarrow \frac{\partial u}{\partial t} = \frac{\partial u}{\partial x_1} +
         \frac{\partial u}{\partial x_2} \\
    \nabla^2 u = 0 \Leftrightarrow  u_{,11} + u_{,22} + u_{,33} = 0 &\Leftrightarrow 
      \frac{\partial^2 u}{\partial x_1^2} + \frac{\partial^2 u}{\partial x_2^2} + \frac{\partial^2 u}{\partial x_3^2} = 0 \\
    u_{,1111} = u_{,22} + u &\Leftrightarrow  \frac{\partial^4 u}{\partial x_1^4} = \frac{\partial^2 u}{\partial x_2^2} + u
    ~.
  \end{align}

An example of a system of partial differential equations is


    \boldsymbol{\nabla} (\boldsymbol{\nabla} \bullet \mathbf{u}) + \nabla^2 \mathbf{u} + \mathbf{f} = \mathbf{0} \Leftrightarrow  
    u_{k,ki} + u_{i,jj} + f_i = 0

In expanded form this system of equations is

\begin{align}
    \frac{\partial^2 u_1}{\partial x_1^2} + \frac{\partial^2 u_2}{\partial x_2\partial x_1} + \frac{\partial^2 u_3}{\partial x_3\partial x_1}
    + \frac{\partial^2 u_1}{\partial x_1^2} + \frac{\partial^2 u_1}{\partial x_2^2} + \frac{\partial^2 u_1}{\partial x_3^2} + f_1 
    & = 0 \\
    \frac{\partial^2 u_1}{\partial x_1\partial x_2} + \frac{\partial^2 u_2}{\partial x_2^2} + \frac{\partial^2 u_3}{\partial x_3\partial x_2}
    + \frac{\partial^2 u_2}{\partial x_1^2} + \frac{\partial^2 u_2}{\partial x_2^2} + \frac{\partial^2 u_2}{\partial x_3^2} + f_2 
    & = 0 \\
    \frac{\partial^2 u_1}{\partial x_1\partial x_3} + \frac{\partial^2 u_2}{\partial x_2\partial x_3} + \frac{\partial^2 u_3}{\partial x_3^2}
    + \frac{\partial^2 u_3}{\partial x_1^2} + \frac{\partial^2 u_3}{\partial x_2^2} + \frac{\partial^2 u_3}{\partial x_3^2} + f_3 
    & = 0 
  \end{align}

It is often more convenient to write PDEs in vector notation or index notation.

Order of a PDE

The order of a PDE is determined by the highest derivative in the equation. For example,

\begin{align}
    \frac{\partial u}{\partial x_1} - \frac{\partial u}{\partial x_2} & = 0 ~~~\text{is a first-order PDE.}\\
    \frac{\partial^2 u}{\partial x_1^2} + \frac{\partial^2 u}{\partial x_2^2} + \frac{\partial^2 u}{\partial x_3^2} & = 0 
          ~~~~\text{is a second-order PDE.}\\
    \frac{\partial^4 u}{\partial x_1^4} + \frac{\partial^2 u}{\partial x_2^2} - u & = 0
          ~~~~\text{is a fourth-order PDE.}\\
    \left(\frac{\partial u}{\partial x_1}\right)^3 + \frac{\partial u}{\partial x_2} + u^4 & = 0 
          ~~~\text{is a first-order PDE.}
  \end{align}

Linear and nonlinear PDEs

A linear PDE is one that is of first degree in all of its field variables and partial derivatives. For example,

\begin{align}
    \frac{\partial u}{\partial x_1} + \frac{\partial u}{\partial x_2} & = 0 ~~~\text{is linear}~.\\
    \frac{\partial u}{\partial x_1} + \left(\frac{\partial u}{\partial x_2}\right)^2 & = 0 
        ~~~\text{is nonlinear}~.\\
    \frac{\partial u}{\partial x_1} + \frac{\partial u}{\partial x_2} + u^2 & = 0 
        ~~~\text{is nonlinear}~.\\
    \frac{\partial^2 u}{\partial x_1^2} + \frac{\partial^2 u}{\partial x_2^2} & = x_1  ~~~\text{is linear}~.\\
    \frac{\partial^2 u}{\partial x_1^2} + u\frac{\partial^2 u}{\partial x_2^2} & = 0  ~~~\text{is quasilinear}~.
  \end{align}

The above equations can also be written in operator notation as

\begin{align}
    D(u) = 0 & ~~\text{where}~~ D := \frac{\partial }{\partial x_1} + \frac{\partial }{\partial x_2}~. \\
    D(u) = 0 & ~~\text{where}~~ D := \frac{\partial }{\partial x_1} + 
            \left(\frac{\partial }{\partial x_2}\right)^2~.\\
    D(u) = 0 & ~~\text{where}~~ D := \frac{\partial }{\partial x_1} + \frac{\partial }{\partial x_2} + u^2~.\\
    D(u) = x_1 & ~~\text{where}~~ D := \frac{\partial^2 }{\partial x_1^2} + \frac{\partial^2 }{\partial x_2^2}~.\\
    D(u) = 0 & ~~\text{where}~~ D := \frac{\partial^2 }{\partial x_1^2} + u\frac{\partial^2 }{\partial x_2^2}~.
  \end{align}

Homogeneous PDEs

Let L be a linear operator. Then an linear partial differential equation can be written in the form


     L(u) = f(x_1,x_2,x_3,t)~.

If f(x_1,x_2,x_3,t) = 0, the PDE is called homogeneous.

Elliptic, Hyperbolic, and Parabolic PDEs

We usually come across three-types of second-order PDEs in mechanics. These are classified as elliptic, hyperbolic, and parabolic.

The equations of elasticity (without inertial terms) are elliptic PDEs. Hyperbolic PDEs describe wave propagation phenomena. The heat conduction equation is an example of a parabolic PDE.

Each type of PDE has certain characteristics that help determine if a particular finite element approach is appropriate to the problem being described by the PDE. Interestingly, just knowing the type of PDE can give us insight into how smooth the solution is, how fast information propagates, and the effect of initial and boundary conditions.

Suppose we have a second-order PDE of the form


    a(x_1,x_2) \frac{\partial^2 u}{\partial x_1^2} + b(x_1,x_2) \frac{\partial^2 u}{\partial x_1\partial x_2} +
    c(x_1,x_2) \frac{\partial^2 u}{\partial x_2^2} + d(x_1,x_2) \frac{\partial u}{\partial x_1} +
    e(x_1,x_2) \frac{\partial u}{\partial x_2} + f(x_1,x_2) u = g(x_1,x_2)

Then, the PDE is called elliptic if


     {
     b^2 - 4ac < 0  ~~~~\implies~~~~ \text{ elliptic} ~.
     }

An example is


     \frac{\partial^2 u}{\partial x_1^2} + \frac{\partial^2 u}{\partial x_1\partial x_2} + \frac{\partial^2 u}{\partial x_2^2} = 
       x_1 \frac{\partial u}{\partial x_1}

The PDE is called hyperbolic if


     {
     b^2 - 4ac > 0  ~~~~\implies~~~~ \text{ hyperbolic} ~.
     }

An example is


     \frac{\partial^2 u}{\partial x_1^2} + 3\frac{\partial^2 u}{\partial x_1\partial x_2} + \frac{\partial^2 u}{\partial x_2^2} = 
       x_1 \frac{\partial u}{\partial x_1}


The PDE is called parabolic if


     {
     b^2 - 4ac = 0  ~~~~\implies~~~~ \text{ parabolic} ~.
     }

An example is


     \frac{\partial^2 u}{\partial x_1^2} + 2\frac{\partial^2 u}{\partial x_1\partial x_2} + \frac{\partial^2 u}{\partial x_2^2} = 
       x_1 \frac{\partial u}{\partial x_1}

Solutions to Common PDEs

Partial differential equation appear in several areas of physics and engineering. A firm grasp of how to solve ordinary differential equations is required to solve PDEs. In particular, solutions to the Sturm-Liouville problems should be familiar to anyone attempting to solve PDEs.

Application of PDEs in Physics and Engineering

There are many applications of partial differential equations in physics and engineering. Here are some examples:

Resources

The Heat conduction equation of 2-D is elliptic in space and parabolic in time.

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