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Differential Equations

We define \begin{equation} y'(t_i)=f(t_i,y_i) \tag{16} \end{equation} and if we truncate \Delta at the first derivative, we have \begin{equation} y_{i+1}=y(t_i) + hf(t_i,y_i) + O(h^2), \tag{17} \end{equation} which when complemented with t_{i+1}=t_i+h forms the algorithm for the well-known Euler method. Note that at every step we make an approximation error of the order of O(h^2) , however the total error is the sum over all steps N=(b-a)/h , yielding thus a global error which goes like NO(h^2)\approx O(h) .