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Mathematical Methods for Physicists: A concise introduction - Site Map

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SECOND-ORDER EQUATIONS WITH CONSTANT COEFFICIENTS<br />

We can <strong>for</strong>m a polynomial function of D and write<br />

F…D† ˆa 0 D n ‡ a 1 D n1 ‡‡a n1 D ‡ a n<br />

so that<br />

F…D† f …t† ˆa 0 D n f ‡ a 1 D n1 f ‡‡a n1 Df ‡ a n f<br />

and we can interpret D 1 as follows<br />

D 1 Df …t† ˆf …t†<br />

and<br />

Z<br />

…Df †dt ˆ f :<br />

Hence D 1 indicates the operation of integration (the inverse of di€erentiation).<br />

Similarly D m f means `integrate f …t†m times'.<br />

These properties of the linear operator D can be used to ®nd the particular<br />

integral of Eq. (2.15):<br />

d 2 y<br />

dt 2 ‡ a dy<br />

dt ‡ by ˆ <br />

D2 ‡ aD ‡ b y ˆ f …t†<br />

from which we obtain<br />

where<br />

y ˆ<br />

1<br />

D 2 ‡ aD ‡ b f …t† ˆ 1<br />

F…D† f …t†;<br />

F…D† ˆD 2 ‡ aD ‡ b:<br />

…2:22†<br />

The trouble with Eq. (2.22) is that it contains an expression involving Ds in the<br />

denominator. It requires a fair amount of practice to use Eq. (2.22) to express y in<br />

terms of conventional functions. For this, there are several rules to help us.<br />

Given a power series of D<br />

and since D n e t ˆ n e t , it follows that<br />

Thus we have<br />

Rules <strong>for</strong> D operators<br />

G…D† ˆa 0 ‡ a 1 D ‡‡a n D n ‡<br />

G…D†e t ˆ…a 0 ‡ a 1 D ‡‡a n D n ‡†e t ˆ G…†e t :<br />

Rule (a): G…D†e t ˆ G…†e t provided G…† is convergent.<br />

When G…D† is the expansion of 1=F…D† this rule gives<br />

1<br />

F…D† et ˆ 1<br />

F…† et provided F…† 6ˆ0:<br />

79

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