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THE WAVE EQUATION 1. Longitudinal Vibrations We describe the ...

THE WAVE EQUATION 1. Longitudinal Vibrations We describe the ...

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4 R. E. SHOWALTERNote that if X(·) and T (·) are solutions of <strong>the</strong>se respective equations, <strong>the</strong>n it followsdirectly that <strong>the</strong>ir product is a solution (3a). <strong>We</strong> have already found <strong>the</strong> non-null solutionsof <strong>the</strong> boundary-value problem{X ′′ (x) + λX(x) = 0, 0 < x < l,(4)X(0) = 0, X(l) = 0.The solutions are <strong>the</strong> normalized eigenfunctionsX n (x) =√2l sin(nπ l x)corresponding to <strong>the</strong> eigenvalues λ n = (nπ/l) 2 . If we combine <strong>the</strong>se with <strong>the</strong> correspondingtime-dependent solutions cos(α √ λ n t) and sin(α √ λ n t) of <strong>the</strong> first differentialequation and take linear combinations, we obtain a large class of solutions of <strong>the</strong> partialdifferential equation (3a) and boundary conditions (3b) in <strong>the</strong> form of a seriesu(x, t) =∞∑ (An cos(α √ λ n t) + B n sin(α √ λ n t) ) X n (x),n=1where <strong>the</strong> sequences {A n } and {B n } are to be determined. From <strong>the</strong> initial conditions(3c), it follows that <strong>the</strong>se coefficients must satisfyso we obtain∞∑A n X n (x) = u 0 (x),n=1∞∑B n α √ λ n X n (x) = v 0 (x), 0 < x < l,n=1A m = (u 0 (·), X m (·)), B m = (v 0(·), X m (·))α √ λ m, m ≥ 1 .In summary, <strong>the</strong> solution of <strong>the</strong> initial-boundary-value problem (3) is given by <strong>the</strong> seriesu(x, t) =∞∑ ( √cos(α λn t)(u 0 (·), X n (·)) + sin(α √ λ n t) (v 0(·), X n (·))α √ )Xn (x).λ nn=1Denote <strong>the</strong> second term in <strong>the</strong> preceding formula by[S(t)v 0 ](x) =∞∑ ( √sin(α λn t) (v 0(·), X n (·))α √ )Xn (x).λ nn=1This defines <strong>the</strong> operator S(t) on <strong>the</strong> space of functions on [0, l]. <strong>We</strong> can use this operatorto represent <strong>the</strong> solution by(5) u(·, t) = S ′ (t)u 0 + S(t)v 0 .Example 2. Suppose <strong>the</strong> rod (0, l) is perfectly elastic and set α 2 = k ρ. Assume that bo<strong>the</strong>nds of <strong>the</strong> rod are fixed, <strong>the</strong> initial displacement and velocity are both null, and that <strong>the</strong>re

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