Runge–Kutta methods
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In numerical analysis, the Runge–Kutta methods are an important family of implicit and explicit iterative methods for the approximation of solutions of ordinary differential equations. These techniques were developed around 1900 by the German mathematicians C. Runge and M.W. Kutta.
See the article on numerical ordinary differential equations for more background and other methods.
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[edit] The classical fourth-order Runge–Kutta method
One member of the family of Runge–Kutta methods is so commonly used that it is often referred to as "RK4" or simply as "the Runge–Kutta method".
Let an initial value problem be specified as follows.
Then, the RK4 method for this problem is given by the following equation:
where
Thus, the next value (yn+1) is determined by the present value (yn) plus the product of the size of the interval (h) and an estimated slope. The slope is a weighted average of slopes:
- k1 is the slope at the beginning of the interval;
- k2 is the slope at the midpoint of the interval, using slope k1 to determine the value of y at the point tn + h/2 using Euler's method;
- k3 is again the slope at the midpoint, but now using the slope k2 to determine the y-value;
- k4 is the slope at the end of the interval, with its y-value determined using k3.
In averaging the four slopes, greater weight is given to the slopes at the midpoint:
The RK4 method is a fourth-order method, meaning that the error per step is on the order of h5, while the total accumulated error has order h4.
Note that the above formulas are valid for both scalar- and vector-valued functions (i.e., y can be a vector).
[edit] Explicit Runge–Kutta methods
The family of explicit Runge–Kutta methods is a generalization of the RK4 method mentioned above. It is given by
where
(Note: the above equations have different but equivalent definitions in different texts).
To specify a particular method, one needs to provide the integer s (the number of stages), and the coefficients aij (for 1 ≤ j < i ≤ s), bi (for i = 1, 2, ..., s) and ci (for i = 2, 3, ..., s). These data are usually arranged in a mnemonic device, known as a Butcher tableau (after John C. Butcher):
0 | ||||||
c2 | a21 | |||||
c3 | a31 | a32 | ||||
cs | as1 | as2 | as,s − 1 | |||
b1 | b2 | bs − 1 | bs |
The Runge–Kutta method is consistent if
There are also accompanying requirements if we require the method to have a certain order p, meaning that the truncation error is O(hp+1). These can be derived from the definition of the truncation error itself. For example, a 2-stage method has order 2 if b1 + b2 = 1, b2c2 = 1/2, and b2a21 = 1/2.
[edit] Examples
The RK4 method falls in this framework. Its tableau is:
0 | |||||
1/2 | 1/2 | ||||
1/2 | 0 | 1/2 | |||
1 | 0 | 0 | 1 | ||
1/6 | 1/3 | 1/3 | 1/6 |
However, the simplest Runge–Kutta method is the (forward) Euler method, given by the formula yn + 1 = yn + hf(tn,yn). This is the only consistent explicit Runge–Kutta method with one stage. The corresponding tableau is:
0 | ||
1 |
An example of a second-order method with two stages is provided by the midpoint method
The corresponding tableau is:
0 | |||
1/2 | 1/2 | ||
0 | 1 |
Note that this 'midpoint' method is not the optimal RK2 method. If one wants to minimize the truncation error, the method below should be used (Atkinson p. 423). Other important methods are Fehlberg, Cash-Karp and Dormand-Prince. Also, read the article on Adaptive Stepsize.
[edit] Usage
The following is an example usage of a two-stage explicit Runge–Kutta method, viz.,
0 | |||
2/3 | 2/3 | ||
1/4 | 3/4 |
to solve the initial-value problem
with step size h=0.025.
The tableau above yields the equivalent corresponding equations below defining the method:
t0 = 1 | |||
y0 = 1 | |||
t1 = 1.025 | |||
k1 = y0 = 1 | f(t0,k1) = 2.557407725 | k2 = y0 + 2 / 3hf(t0,k1) = 1.042623462 | |
y1 = y0 + h(1 / 4 * f(t0,k1) + 3 / 4 * f(t0 + 2 / 3h,k2)) = 1.066869388 | |||
t2 = 1.05 | |||
k1 = y1 = 1.066869388 | f(t1,k1) = 2.813524695 | k2 = y1 + 2 / 3hf(t1,k1) = 1.113761467 | |
y2 = y1 + h(1 / 4 * f(t1,k1) + 3 / 4 * f(t1 + 2 / 3h,k2)) = 1.141332181 | |||
t3 = 1.075 | |||
k1 = y2 = 1.141332181 | f(t2,k1) = 3.183536647 | k2 = y2 + 2 / 3hf(t2,k1) = 1.194391125 | |
y3 = y2 + h(1 / 4 * f(t2,k1) + 3 / 4 * f(t2 + 2 / 3h,k2)) = 1.227417567 | |||
t4 = 1.1 | |||
k1 = y3 = 1.227417567 | f(t3,k1) = 3.796866512 | k2 = y3 + 2 / 3hf(t3,k1) = 1.290698676 | |
y4 = y3 + h(1 / 4 * f(t3,k1) + 3 / 4 * f(t3 + 2 / 3h,k2)) = 1.335079087 |
The numerical solutions correspond to the underlined values. Note that f(ti,k1) has been calculated to avoid recalculation in the yis.
[edit] References
- George E. Forsythe, Michael A. Malcolm, and Cleve B. Moler. Computer Methods for Mathematical Computations. Englewood Cliffs, NJ: Prentice-Hall, 1977. (See Chapter 6.)
- Ernst Hairer, Syvert Paul Nørsett, and Gerhard Wanner. Solving ordinary differential equations I: Nonstiff problems, second edition. Berlin: Springer Verlag, 1993. ISBN 3-540-56670-8.
- William H. Press, Brian P. Flannery, Saul A. Teukolsky, William T. Vetterling. Numerical Recipes in C. Cambridge, UK: Cambridge University Press, 1988. (See Sections 16.1 and 16.2.)
- Runge-Kutta 4th-order method textbook notes, PPT, Matlab Mathematica Maple Mathcad at Holistic Numerical Methods Institute
- Kendall E. Atkinson. An Introduction to Numerical Analysis. John Wiley & Sons - 1989
- F. Cellier, E. Kofman. Continuous System Simulation. Springer Verlag, 2006. ISBN 0-387-26102-8.