Math 320 - Fall 2010 HW #7 Selected Solutions Problem 5.1.32 Let ...
Math 320 - Fall 2010 HW #7 Selected Solutions Problem 5.1.32 Let ...
Math 320 - Fall 2010 HW #7 Selected Solutions Problem 5.1.32 Let ...
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<strong>Math</strong> <strong>320</strong> - <strong>Fall</strong> <strong>2010</strong><br />
<strong>HW</strong> <strong>#7</strong> <strong>Selected</strong> <strong>Solutions</strong><br />
<strong>Problem</strong> <strong>5.1.32</strong><br />
<strong>Let</strong> y1 and y2 be two solutions of A(x)y ′′ + B(x)y ′ + C(x)y = 0 on an open interval I where A, B and<br />
C are continuous and A(x) is never zero.<br />
(a) <strong>Let</strong> W = W (y1, y2). Show that<br />
A(x) dW<br />
dx<br />
= (y1)(Ay ′′<br />
2 ) − (y2)(Ay ′′<br />
1 )<br />
Then substitute for Ay ′′<br />
2 and Ay ′′<br />
1 from the original differential equation to show that<br />
A(x) dW<br />
dx<br />
= −B(x)W (x).<br />
(b) Solve this first-order equation to deduce Abel’s formula<br />
� �<br />
B(x)<br />
W (x) = K exp −<br />
A(x) dx<br />
�<br />
where K is a constant.<br />
(c) Why does Abel’s formula imply that the Wronskian W (y1, y2) is either zero everywhere or nonzero<br />
everywhere (as stated in [EP10, 5.1, Theorem 3])?<br />
(a) First, since y1 and y2 are solutions to the given differential equation, we have that the Wronskian<br />
W (y1, y2) = y1y ′ 2 − y ′ 1y2. This is a differentiable function of x (it’s the product and difference of<br />
differentiable functions), and so we can compute<br />
Then, we have<br />
dW<br />
dx = y′ 1y ′ 2 + y1y ′′<br />
2 − (y ′ 1y ′ 2 + y ′′<br />
1 y2) = y1y ′′<br />
2 − y ′′<br />
1 y2<br />
A(x) dW<br />
′′<br />
= A(x)(y1y 2 − y<br />
dx ′′<br />
1 y2) = y1(Ay ′′<br />
2 ) − y2(Ay ′′<br />
1 )<br />
as desired. Next, following the hint, observe that y1 is a solution to our given differential equation, so we<br />
have that A(x)y ′′<br />
1 + B(x)y ′ 1 + C(x)y1 = 0. Solving this for A(x)y ′′<br />
1 yields A(x)y ′′<br />
1 = −B(x)y ′ 1 − C(x)y1.<br />
Since y2 is also solution to our given differential equation, we can repeat this process and write A(x)y ′′<br />
2 =<br />
−B(x)y ′ 2 − C(x)y2. Substituting these quantities above, we obtain<br />
A(x) dW<br />
dx<br />
which is what we set out to show.<br />
= y1(Ay ′′<br />
2 ) − y2(Ay ′′<br />
1 ) = y1(−B(x)y ′ 2 − C(x)y2) − y2(−B(x)y ′ 1 − C(x)y1)<br />
= −B(x)y1y ′ 2 + B(x)y2y ′ 1<br />
= −B(x)(y1y ′ 2 − y ′ 1y2) = −B(x)W (x)<br />
(b) Next, observe that A(x)dW/dx = −B(x)W is a first order separable equation that we can solve using<br />
1
our techniques from earlier in the semester.<br />
dW −B(x)<br />
=<br />
W A(x) dx<br />
� �<br />
dW B(x)<br />
= −<br />
W A(x) dx<br />
�<br />
B(x)<br />
ln |W | + C1 = −<br />
A(x) dx<br />
�<br />
B(x)<br />
ln |W | = − dx + C<br />
A(x)<br />
Now, first assume that W > 0. Then we have ln |W | = ln W , and then, taking exp of both sides, and<br />
setting K = eC , we obtain<br />
� �<br />
B(x)<br />
W = exp −<br />
A(x) dx<br />
�<br />
e C � �<br />
B(x)<br />
= K exp −<br />
A(x) dx<br />
�<br />
In this case, note that K = eC is a positive constant.<br />
On the other hand, if W < 0, then ln |W | = ln −W , and so taking exp of both sides yields<br />
� �<br />
B(x)<br />
W = −K exp −<br />
A(x) dx<br />
�<br />
Now, since K = e C is positive, −K is negative. Then, we can label the value −K as the new constant<br />
K, and obtain the same formula as above W = K exp(− � B(x)/A(x) dx), except now the constant K<br />
is negative.<br />
Finally, if W = 0, then we don’t need to solve a separable equation (in fact, if you look at the<br />
separable equation above, it doesn’t make sense when W = 0 since we’re integrating 1/W ). However,<br />
in this case, when W = 0, we can still use our formula W = K exp(− � B(x)/A(x) dx) simply by<br />
setting K = 0.<br />
(c) [EP10, 5.1 Theorem 3] says something quite peculiar. It claims that the Wronskian W (y1, y2) of two<br />
solutions to a homogeneous second order linear equation is either always zero (in which case y1 and y2<br />
are linearly dependent), or, W (y1, y2) is never zero (in which case y1 and y2 are linearly independent).<br />
However, this seems to leave a gap - what if the Wronskian is sometimes zero, but not always zero?<br />
The formula we proved in [part (b)] explains why this can’t happen.<br />
� �<br />
B(x)<br />
W (x) = K exp −<br />
A(x) dx<br />
�<br />
We know that an exponential function is never zero. Thus, the Wronskian, when it exists, is either<br />
always non-zero (if K �= 0) or, always zero (if K = 0). There are no other possibilities, and so [EP10,<br />
5.1 Theorem 3] makes sense.<br />
2
<strong>Problem</strong> 5.1.51<br />
A second-order Euler equation is one of the form<br />
where a, b, c are constants.<br />
ax 2 y ′′ + bxy ′ + cy = 0, (1)<br />
(a) Show that if x > 0, then the substitution v = ln x transforms [Equation 1] into the constantcoefficient<br />
linear equation<br />
a d2y + (b − a)dy + cy = 0 (2)<br />
dv2 dv<br />
with independent variable v.<br />
(b) If the roots r1 and r2 of the characteristic equation of [Equation 2] are real and distinct, conclude<br />
that a general solution of the Euler equation in [Equation 1] is y(x) = c1x r1 + c2x r2 .<br />
Observe that [Equation 1] is a second order linear equation, but with non-constant coefficients. The point<br />
of this problem is to transform this non-constant equation into an equation with constant coefficients that<br />
we can easily solve.<br />
One important observation before we get started. The y ′ and y ′′ in [Equation 1] are derivatives with<br />
respect to x. We want to transform them into derivatives with respect to v, so we’ll have to apply the chain<br />
rule.<br />
(a) Note: There’s a slightly shorter way of doing this part; see the paragraph immediately<br />
before [part b]. Since v = ln x, we have x = e v . Then, since y is a function of x, we have<br />
y = y(x) = y(e v ), and so y is also a function of v. Thus, it makes sense to differentiate y with respect<br />
to v, but we must use the chain rule. Recall that if y(x) = y(g(v)), the chain rule can be written<br />
dy<br />
dv<br />
dy<br />
�<br />
� dx<br />
= �<br />
dx g(v) dv<br />
Where dy<br />
dx | g(v) simply denotes the derivative of y with respect to x evaluated at g(v). To obtain an<br />
expression d2 y<br />
dv 2 , we differentiate the above expression<br />
d2y dv2 = d2y dx2 �<br />
� dg dx<br />
�<br />
g(v) dv dv<br />
dy<br />
�<br />
� d<br />
+ �<br />
dx g(v)<br />
2x dv2 This expression follows from [Equation 3]: simply differentiate [Equation 3] with respect to v, using<br />
the product rule, and remember to apply the chain rule when differentiating dy<br />
�<br />
�<br />
dx�<br />
.<br />
g(v)<br />
Returning to the problem, suppose that x = e v , and so dx/dv = d(e v )/dv = e v . Then, y(x) = y(e v ),<br />
and so applying the chain rule above, we have<br />
dy dy<br />
�<br />
� dx<br />
= �<br />
dv dx ev dv<br />
= dy<br />
�<br />
�<br />
� e<br />
dx ev v<br />
d2y dv2 = d2y dx2 �<br />
� de<br />
�<br />
ev v dx dy<br />
�<br />
� d<br />
+ �<br />
dv dv dx ev 2x dv2 = d2y dx2 �<br />
�<br />
�<br />
ev eve v + dy<br />
�<br />
� de<br />
�<br />
dx ev v<br />
dv<br />
= d2y dx2 �<br />
�<br />
� e<br />
ev 2v + dy<br />
�<br />
�<br />
� e<br />
dx ev v<br />
3<br />
(3)
Now, we wish to show that a d2y dv2 + (b − a) dy<br />
dv + cy = 0, so we simply substitute in the expressions we’ve<br />
computed for d 2 y/dv 2 and dy/dv.<br />
a d2 � 2 y<br />
d y<br />
+ (b − a)dy + cy = a<br />
dv2 dv dx2 �<br />
�<br />
� e<br />
ev 2v + dy<br />
�<br />
�<br />
� e<br />
dx ev v<br />
� �<br />
dy<br />
�<br />
�<br />
+ (b − a) � e<br />
dx ev v<br />
�<br />
+ cy<br />
= a d2y dx2 �<br />
�<br />
� e<br />
ev 2v + b dy<br />
�<br />
�<br />
�<br />
dx ev = a d2y dx2 �<br />
�<br />
� x<br />
x<br />
2 + b dy<br />
�<br />
�<br />
� x + cy<br />
dx x<br />
= ay ′′ x 2 + by ′ x + cy<br />
= 0<br />
e v + cy now, recall that x = e v<br />
We obtain the third from last line, since d 2 y/dx 2 |x is simply the second derivative of y with respect to<br />
x evaluated at x - in other words, our good old y ′′ , and similarly dy/dx|x is simply y ′ . The fact that<br />
the last line is 0 is simply because y is a solution to the original [Equation 1].<br />
Alternative: We can get the same derivation as above, going the other way, which has a little<br />
clearer notation. Suppose that y(v) is a function such that y(ln x) is a solution to [Equation 1]. We<br />
wish to show that ay ′′ (v) + (b − a)y ′ (v) + cy(v) = 0. To start off, note that (y(ln x)) ′ = y ′ (ln x)(1/x)<br />
and (y(ln x)) ′′ = y ′′ (ln x)(1/x 2 ) + y ′ (ln x)(−1/x 2 ). Then, we have the following:<br />
0 = ax 2 (y(ln x)) ′′ + bx(y(ln x)) ′ + cy(ln x)<br />
= ax 2 (y ′′ (ln x)(1/x 2 ) − y ′ (ln x)(1/x 2 )) + bxy ′ (ln x)(1/x) + cy(ln x)<br />
= ay ′′ (ln x) − ay ′ (ln x) + by ′ (ln x) + cy(ln x)<br />
= ay ′′ (ln x) + (b − a)y ′ (ln x) + cy(ln x)<br />
= ay ′′ (v) + (b − a)y ′ (v) + cy(v)<br />
(b) After transforming [Equation 1] to [Equation 2] we obtain a second order linear equation with constant<br />
coefficients. Thus, we can solve [Equation 2] simply by finding roots of the characteristic equation<br />
ar 2 + (b − a)r + c = 0. Suppose that we’re in a situation where this characteristic equation has distinct<br />
real roots r1 and r2. Then we know that a general solution to [Equation 2] is given by y = c1e r1v +c2e r2v<br />
(note that the independent variable here is v, since [Equation 2] has independent variable v).<br />
But since v = ln x, by substitution we have that<br />
y = c1e r1v + c2e r2v = c1e r1 ln x + c2e r2 ln x = c1x r1 + c2x r2<br />
is a solution to [Equation 1], which is what we set out to show.<br />
4
<strong>Problem</strong> (<strong>HW</strong> 7, <strong>Problem</strong> 2)<br />
Given one solution y1(x) to the ODE: (i) verify that y1(x) is a solution to the given ODE, and (ii) use<br />
the method of Reduction of Order to find the general solution:<br />
x 2 y ′′ − 4xy ′ + 6y = 0, x > 0, y1 = x 2<br />
4x 2 y ′′ − 4xy ′ + 3y = 0, x > 0, y1 = x 1/2<br />
x 2 y ′′ + xy ′ + y = 0, x > 0, y1 = cos(ln(x))<br />
For these problems we’ll use the following fact from reduction of order: If y1 is a solution to a second order<br />
linear differential equation y ′′ + p(x)y ′ + q(x)y = 0, then we can obtain the general solution yg = vy1, where<br />
the function v satisfies the differential equation v ′′ + v ′ (2y ′ 1 + y1p)/y1 = 0<br />
(a) We have y ′ 1 = 2x and y ′′<br />
1 = 2, so substituting we have x 2 2 − 4x(2x) + 6x 2 = 0, and so indeed y1<br />
is a solution. To find the general solution, we’ll use reduction of order. First, our given equation in<br />
standard form is y ′′ − (4/x)y ′ + (6/x 2 )y = 0. Then, we must find the unknown function v that satisfies<br />
v ′′ + v ′ (2y ′ 1 + y1p)/y1 = 0. Substituting, we wish to solve the differential equation<br />
v ′′ + v ′<br />
� �<br />
2 −4 4x + x x<br />
x2 = v ′′ = 0<br />
This equation is easy to solve: Integrating twice yields v = c1x + c2, and so our general solution is<br />
given by y = y1v = x 2 (c1x + c2) = c1x 3 + c2x 2 .<br />
(b) Proceeding exactly as before, we have y ′ 1 = (1/2)x−1/2 and y ′′<br />
1 = (−1/4)x−3/2 , and then 4x2 (−1/4)x−3/2− 4x(1/2)x−1/2 +3x1/2 = −x1/2−2x1/2 +3x1/2 = 0, and so y1 is indeed a solution. To find the general solution,<br />
we proceed with reduction of order with the standard form equation y ′′ −(1/x)y ′ +(3/(4x2 ))y = 0<br />
� �<br />
−1/2 1/2 x + x (−1/x)<br />
v ′′ + v ′<br />
x 1/2<br />
= v ′′ = 0<br />
Once again, we simply have to solve v ′′ = 0, and so integrating twice yields v = c1x + c2. Then, our<br />
general solution is given by y = vy1 = c1x 3/2 + c2x 1/2 .<br />
(c) We first verify that y1 is indeed a solution. We have y ′ 1 = − sin(ln(x))(1/x) and y ′′<br />
1 = −(cos(ln(x)))(1/x 2 )−<br />
sin(ln(x))(−1/x 2 ). Then, substituting, we have<br />
x 2 (−(cos(ln(x)))(1/x 2 )− sin(ln(x))(−1/x 2 )) + x(− sin(ln(x))(1/x)) + cos(ln(x))<br />
= − cos(ln x) + sin(ln x) − sin(ln x) + cos(ln x)<br />
= 0,<br />
and so y1 is a solution to our equation. In standard form our equation is given by y ′′ +y ′ /x+y/x 2 = 0.<br />
To find the general solution, we must find the function v that satisfies<br />
v ′′ ′ (2(− sin(ln x)(1/x)) + cos(ln x)(1/x))<br />
+ v = v<br />
cos(ln x)<br />
′′ ′ cos(ln x) − 2 sin(ln x)<br />
+ v = 0<br />
x cos(ln x)<br />
If we set w = v ′ , then this is a first order linear equation, so we can apply our techniques from earlier<br />
5
in the semester to solve it. First, let’s compute the integrating factor<br />
�� �<br />
cos(ln x) − 2 sin(ln x)<br />
µ(x) = exp<br />
dx u = ln x, du = 1/xdx<br />
x cos(ln x)<br />
�� �<br />
cos u − 2 sin u<br />
= exp<br />
du<br />
cos u<br />
= exp [u + 2 ln | cos u|]<br />
= e u ln | cos u|2<br />
e = e u (cos u) 2 = e ln x (cos(ln x)) 2 = x(cos(ln x)) 2<br />
Observe that we’re justified in removing our absolute values since, for any x, |x| 2 = x 2 . Proceeding<br />
further with the integrating factor method, we have<br />
d<br />
dx (v′ x(cos(ln x)) 2 ) = 0<br />
v ′ =<br />
c1<br />
x(cos(ln x)) 2<br />
Now, to find v we simply integrate once more<br />
�<br />
c1<br />
v =<br />
dx<br />
x(cos(ln x)) 2<br />
�<br />
c1<br />
v =<br />
cos<br />
u = ln x, du = 1/xdx<br />
2 u du<br />
�<br />
v = c1 sec 2 u du<br />
v = c1 tan u + c2<br />
v = c1 tan(ln x) + c2<br />
Then, we have that the general solution is given by y = vy1 = c1 tan(ln x) cos(ln x) + c2 cos(ln x) =<br />
c1 sin(ln x) + c2 cos(ln x).<br />
References<br />
[EP10] C. Henry Edwards and David E. Penney. Differential Equations & Linear Algebra. Prentice Hall,<br />
Third edition, <strong>2010</strong>.<br />
6