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Mathematical Methods for Physicists: A concise introduction - Site Map

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VIBRATING STRINGS<br />

Since the left hand side is a function of x only and the right hand side is a function<br />

of time only, they must be equal to a common separation constant, which we will<br />

call 2 . Then we have<br />

and<br />

d 2 X=dx 2 ˆ 2 X; X…0† ˆX…L† ˆ0 …4:16a†<br />

d 2 T=dt 2 ˆ 2 v 2 T dT=dt ˆ 0 at t ˆ 0: …4:16b†<br />

Both of these equations are typical eigenvalue problems: we have a di€erential<br />

equation containing a parameter , and we seek solutions satisfying certain<br />

boundary conditions. If there are special values of <strong>for</strong> which non-trivial solutions<br />

exist, we call these eigenvalues, and the corresponding solutions eigensolutions<br />

or eigenfunctions.<br />

The general solution of Eq. (4.16a) can be written as<br />

Applying the boundary conditions<br />

and<br />

X…x† ˆA 1 sin…x†‡B 1 cos…x†:<br />

X…0† ˆ0 ) B 1 ˆ 0;<br />

X…L† ˆ0 ) A 1 sin…L† ˆ0<br />

A 1 ˆ 0 is the trivial solution X ˆ 0 (so y ˆ 0); hence we must have sin…L† ˆ0,<br />

that is,<br />

and we obtain a series of eigenvalues<br />

and the corresponding eigenfunctions<br />

L ˆ n; n ˆ 1; 2; ...;<br />

n ˆ n=L; n ˆ 1; 2; ...<br />

X n …x† ˆsin…n=L†x; n ˆ 1; 2; ... :<br />

To solve Eq. (4.16b) <strong>for</strong> T…t† we must use one of the values n found above. The<br />

general solution is of the <strong>for</strong>m<br />

T…t† ˆA 2 cos… n vt†‡B 2 sin… n vt†:<br />

The boundary condition leads to B 2 ˆ 0.<br />

The general solution of Eq. (4.14) is hence a linear superposition of the solutions<br />

of the <strong>for</strong>m<br />

y…x; t† ˆX1<br />

nˆ1<br />

A n sin…nx=L† cos…nvt=L†;<br />

…4:17†<br />

159

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