6.3 Partial Differential Equations 381
Part a. (r 0 =0.) The limit assapproaches zero ofsU(x,s)may be found by
L’Hôpital’s rule or by using the Taylor series for sinh and cosh. From the latter,
sU(x,s)=sx(
1 +s 22 +···)
−
(
sx+s^36 x^3 +···)
s^2(
1 +s 22 +···)
=
s^3(x
2 −x^3
6 −···)
s^2(
1 +s 22 +···)→ 0.
Thus, in spite of the formidable appearance ofs^3 in the denominator,s=0is
not really a significant value and contributes nothing tou(x,t).
Part b. It is convenient to take the remaining roots in pairs. We label
±i( 2 n− 1 )π
2 =±iρn.
The derivative of the denominator isp′(s)= 3 s^2 cosh(s)+s^3 sinh(s),
p′(±iρn)=±i^3 ρ^3 nsinh(±iρn)
=ρ^3 nsin(ρn)since sinh(iρ)=isin(ρ)and(±i)^4 =1. The contribution of these two roots
together may be calculated using the exponential definition of sine:
q(iρn)
p′(iρn)exp(iρnt)+q(−iρn)
r′(−iρn)exp(−iρnt)=−sinh(iρnx)exp(iρnt)+sinh(iρnx)exp(−iρnt)
ρn^3 sin(ρn)=ρsin 3 (ρnx)
nsin(ρn)i(
−exp(iρnt)+exp(−iρnt))
=
2sin(ρnx)sin(ρnt)
ρ^3 nsin(ρn).Part c. The final form ofu(x,t), found by adding up all the contributions
from Part b, is the same as would be found by separation of variables
u(x,t)= 2∑∞
1sin(ρnx)sin(ρnt)
ρ^3 nsin(ρn).