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Mathematical Methods for Physics and Engineering - Matematica.NET

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HIGHER-ORDER ORDINARY DIFFERENTIAL EQUATIONSIf the original equation (15.1) has f(x) = 0 (i.e. it is homogeneous) then ofcourse the complementary function y c (x) in (15.3) is already the general solution.If, however, the equation has f(x) ≠ 0 (i.e. it is inhomogeneous) then y c (x) isonlyone part of the solution. The general solution of (15.1) is then given byy(x) =y c (x)+y p (x), (15.7)where y p (x)istheparticular integral,whichcanbeany function that satisfies (15.1)directly, provided it is linearly independent of y c (x). It should be emphasised <strong>for</strong>practical purposes that any such function, no matter how simple (or complicated),is equally valid in <strong>for</strong>ming the general solution (15.7).It is important to realise that the above method <strong>for</strong> finding the general solutionto an ODE by superposing particular solutions assumes crucially that the ODEis linear. For non-linear equations, discussed in section 15.3, this method cannotbe used, <strong>and</strong> indeed it is often impossible to find closed-<strong>for</strong>m solutions to suchequations.15.1 Linear equations with constant coefficientsIf the a m in (15.1) are constants rather than functions of x then we haved n ya ndx n + a d n−1 yn−1dx n−1 + ···+ a dy1dx + a 0y = f(x). (15.8)Equations of this sort are very common throughout the physical sciences <strong>and</strong>engineering, <strong>and</strong> the method <strong>for</strong> their solution falls into two parts as discussedin the previous section, i.e. finding the complementary function y c (x) <strong>and</strong> findingthe particular integral y p (x). If f(x) = 0 in (15.8) then we do not have to finda particular integral, <strong>and</strong> the complementary function is by itself the generalsolution.15.1.1 Finding the complementary function y c (x)The complementary function must satisfyd n ya ndx n + a d n−1 yn−1dx n−1 + ···+ a dy1dx + a 0y = 0 (15.9)<strong>and</strong> contain n arbitrary constants (see equation (15.3)). The st<strong>and</strong>ard method<strong>for</strong> finding y c (x) is to try a solution of the <strong>for</strong>m y = Ae λx , substituting this into(15.9). After dividing the resulting equation through by Ae λx , we are left with apolynomial equation in λ of order n; thisistheauxiliary equation <strong>and</strong> readsa n λ n + a n−1 λ n−1 + ···+ a 1 λ + a 0 =0. (15.10)492

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