Numerical methods for ordinary differential equations

Numerical ordinary differential equations is the part of numerical analysis which studies the numerical solution of ordinary differential equations (ODEs). This field is also known under the name numerical integration, but some people reserve this term for the computation of integrals.

Many differential equations cannot be solved analytically; however, in science and engineering, a numeric approximation to the solution is often good enough to solve a problem. The algorithms studied here can be used to compute such an approximation. An alternative method is to use techniques from calculus to obtain a series expansion of the solution.

Ordinary differential equations occur in many scientific disciplines, for instance in physics, chemistry, biology, and economics. In addition, some methods in numerical partial differential equations convert the partial differential equation into an ordinary differential equation, which must then be solved.

Contents

The problem

We want to approximate the solution of the differential equation

y'(t) = f(t,y(t)), \qquad y(t_0)=y_0, \qquad\qquad (1)

where f is a function that maps [t0,∞) × Rd to Rd, and the initial condition y0 ∈ Rd is a given vector.

The above formulation is called an initial value problem (IVP). The Picard–Lindelöf theorem states that there is a unique solution, if f is Lipschitz continuous. In contrast, boundary value problems (BVPs) specify (components of) the solution y at more than one point. Different methods need to be used to solve BVPs, for example the shooting method (and its variants) or global methods like finite differences, Galerkin methods, or collocation methods.

Note that we restrict ourselves to first-order differential equations (meaning that only the first derivative of y appears in the equation, and no higher derivatives). However, a higher-order equation can easily be converted to a system of first-order equations by introducing extra variables. For example, the second-order equation y'' = −y can be rewritten as two first-order equations: y' = z and z' = −y.

Methods

Three elementary methods are discussed to give the reader a feeling for the subject. After that, pointers are provided to other methods (which are generally more accurate and efficient). The methods mentioned here are analysed in the next section.

The Euler method

For more details on this topic, see Euler method.

A brief explanation: From any point on a curve, you can find an approximation of a nearby point on the curve by moving a short distance along a line tangent to the curve.

Rigorous development: Starting with the differential equation (1), we replace the derivative y' by the finite difference approximation

y'(t) \approx \frac{y(t%2Bh) - y(t)}{h}, \qquad\qquad (2)

which when re-arranged yields the following formula

y(t%2Bh) \approx y(t) %2B hy'(t) \qquad\qquad

and using (1) gives:

y(t%2Bh) \approx y(t) %2B hf(t,y(t)). \qquad\qquad (3)

This formula is usually applied in the following way. We choose a step size h, and we construct the sequence t0, t1 = t0 + h, t2 = t0 + 2h, … We denote by yn a numerical estimate of the exact solution y(tn). Motivated by (3), we compute these estimates by the following recursive scheme

y_{n%2B1} = y_n %2B hf(t_n,y_n). \qquad\qquad (4)

This is the Euler method (or forward Euler method, in contrast with the backward Euler method, to be described below). The method is named after Leonhard Euler who described it in 1768.

The Euler method is an example of an explicit method. This means that the new value yn+1 is defined in terms of things that are already known, like yn.

The backward Euler method

If, instead of (2), we use the approximation

y'(t) \approx \frac{y(t) - y(t-h)}{h}, \qquad\qquad (5)

we get the backward Euler method:

y_{n%2B1} = y_n %2B hf(t_{n%2B1},y_{n%2B1}). \qquad\qquad (6)

The backward Euler method is an implicit method, meaning that we have to solve an equation to find yn+1. One often uses fixed point iteration or (some modification of) the Newton–Raphson method to achieve this. Of course, it costs time to solve this equation; this cost must be taken into consideration when one selects the method to use. The advantage of implicit methods such as (6) is that they are usually more stable for solving a stiff equation, meaning that a larger step size h can be used.

The exponential Euler method

If the differential equation is of the form

y'(t) = A-By(t) \qquad\qquad\qquad (7)

then an approximate explicit solution can be given by

y_{n%2B1} = y_n e^{-Bh}%2B\frac{A}{B}(1-e^{-Bh})\ . \qquad\qquad (8)

This method is commonly employed in neural simulations and it is the default integrator in the GENESIS neural simulator.[1]

Generalizations

The Euler method is often not accurate enough. In more precise terms, it only has order one (the concept of order is explained below). This caused mathematicians to look for higher-order methods.

One possibility is to use not only the previously computed value yn to determine yn+1, but to make the solution depend on more past values. This yields a so-called multistep method. Perhaps the simplest is the Leapfrog method which is second order and (roughly speaking) relies on two time values.

Almost all practical multistep methods fall within the family of linear multistep methods, which have the form

\alpha_k y_{n%2Bk} %2B \alpha_{k-1} y_{n%2Bk-1} %2B \cdots %2B \alpha_0 y_n
= h \left[ \beta_k f(t_{n%2Bk},y_{n%2Bk}) %2B \beta_{k-1} f(t_{n%2Bk-1},y_{n%2Bk-1}) %2B \cdots %2B \beta_0 f(t_n,y_n) \right].

Another possibility is to use more points in the interval [tn,tn+1]. This leads to the family of Runge–Kutta methods, named after Carl Runge and Martin Kutta. One of their fourth-order methods is especially popular.

Advanced features

A good implementation of one of these methods for solving an ODE entails more than the time-stepping formula.

It is often inefficient to use the same step size all the time, so variable step-size methods have been developed. Usually, the step size is chosen such that the (local) error per step is below some tolerance level. This means that the methods must also compute an error indicator, an estimate of the local error.

An extension of this idea is to choose dynamically between different methods of different orders (this is called a variable order method). Methods based on Richardson extrapolation, such as the Bulirsch–Stoer algorithm, are often used to construct various methods of different orders.

Other desirable features include:

Alternative methods

Many methods do not fall within the framework discussed here. Some classes of alternative methods are:

Analysis

Numerical analysis is not only the design of numerical methods, but also their analysis. Three central concepts in this analysis are:

Convergence

A numerical method is said to be convergent if the numerical solution approaches the exact solution as the step size h goes to 0. More precisely, we require that for every ODE (1) with a Lipschitz function f and every t* > 0,

\lim_{h\to0%2B} \max_{n=0,1,\dots,\lfloor t^*/h\rfloor} \| y_{n,h} - y(t_n) \| = 0.

All the methods mentioned above are convergent. In fact, convergence is a condition sine qua non (necessary condition) for any numerical scheme.

Consistency and order

Suppose the numerical method is

y_{n%2Bk} = \Psi(t_{n%2Bk}; y_n, y_{n%2B1}, \dots, y_{n%2Bk-1}; h). \,

The local error of the method is the error committed by one step of the method. That is, it is the difference between the result given by the method, assuming that no error was made in earlier steps, and the exact solution:

\delta^h_{n%2Bk} = \Psi \left( t_{n%2Bk}; y(t_n), y(t_{n%2B1}), \dots, y(t_{n%2Bk-1}); h \right) - y(t_{n%2Bk}).

The method is said to be consistent if

\lim_{h\to 0} \frac{\delta^h_{n%2Bk}}{h} = 0.

The method has order p if

\delta^h_{n%2Bk} = O(h^{p%2B1}) \quad\mbox{as } h\to0.

Hence a method is consistent if it has an order greater than 0. The (forward) Euler method (4) and the backward Euler method (6) introduced above both have order 1, so they are consistent. Most methods being used in practice attain higher order. Consistency is a necessary condition for convergence, but not sufficient; for a method to be convergent, it must be both consistent and zero-stable.

A related concept is the global error, the error sustained in all the steps one needs to reach a fixed time t. Explicitly, the global error at time t is yN − y(t) where N = (t−t0)/h. The global error of a pth order one-step method is O(hp); in particular, such a method is convergent. This statement is not necessarily true for multi-step methods.

Stability and stiffness

Main article: Stiff equation

For some differential equations, application of standard methods—such as the Euler method, explicit Runge–Kutta methods, or multistep methods (e.g., Adams–Bashforth methods)—exhibit instability in the solutions, though other methods may produce stable solutions. This "difficult behaviour" in the equation (which may not necessarily be complex itself) is described as stiffness, and is often caused by the presence of different time scales in the underlying problem. Stiff problems are ubiquitous in chemical kinetics, control theory, solid mechanics, weather forecasting, biology, plasma physics, and electronics.

History

Below is a timeline of some important developments in this field.

See also

Software for ODE solving

References

  1. ^ http://www.genesis-sim.org/BABEL/gum-tutorials/cornelis/doc/html/node9.html

External links

First order methods
Second order methods
Higher order methods