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 is
p′(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
∑∞
1
sin(ρnx)sin(ρnt)
ρ^3 nsin(ρn).