http://fourier.eng.hmc.edu/e176/lectures/NM/node42.html
Example
Solve the famous 2nd order constant-coefficient ordinary differential equation

with zero initial conditions










- Euler's method
- Modified Euler's method
- Runge-Kutta 2
- Runge-Kutta 4

where

The results of these numerical integral methods and the ground truth closed-form solution are compared as shown below for three different step sizes: 0.5 (left), 0.05 (middle), and 0.01 (right):



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