Math 3D Homework 6: Solving 2nd-Order Linear Homogeneous Diff. Equations, Assignments of Mathematics

The solutions to problems 8 and 19 from section 2.2 of math 3d homework 6. The problems involve finding the solutions to second-order linear homogeneous differential equations with constant coefficients using the method of characteristic roots. The solutions are presented in both general and specific forms.

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MATH 3D Homework 6 Name: Solutions
Feb. 17, 2006
Section 2.2 (p. 140) Problems
8. Solve the initial-value problem
d2y
dt26dy
dt +y= 0; y(2) = 1, y0(2) = 1.
Solution: (10 points) This is a second-order, linear homogeneous problem
with constant coefficients. So, we look for solutions of the form y=ert:
r26r+ 1 = 0 =r= 3 ±22.
Let us name r1= 3 22 and r2= 3 + 22. Noting that the initial time is 2,
the general solution is
y(t) = c1er1(t2) +c2er2(t2).
So, by the initial conditions, we have
1 = y(2) = c1+c2
1 = y0(2) = r1c1+r2c2.
If we multiply the first equation by r1and subtract the second equation from
the first, then
(r1r2)c2=r11 =c2=r11
r1r2
.
So,
c1= 1 c2=1r2
r1r2
.
Plugging back in r1and r2, we can find y(t):
y(t) = µ1r2
r1r2e(322)(t2) +µr11
r1r2e(3+22)(t2)
=Ã2+1
22!e(322)(t2) +Ã21
22!e(3+22)(t2)
=Ã2+1
22!e6+42e(322)t+Ã21
22!e642e(3+22)t.
Section 2.2 (p. 144) Problems
19. Find the general solution of
t2d2y
dt2+ 2tdy
dt + 2y= 0, t > 0.
Solution: (10 points) This is a second-order, linear homogeneous equation,
and it’s an Euler’s equation. So, we look for solutions of the form y=tr:
t2r(r1)tr2+ 2trtr1+ 2tr=tr¡r2+r+ 2¢= 0.
Document URL: http://math.uci.edu/~pmacklin/Math3Dwinter2006.html
Date: February 22, 2006 Page 1 of 2
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MATH 3D Homework 6 Name: Solutions

Feb. 17, 2006

Section 2.2 (p. 140) Problems

  1. Solve the initial-value problem

d^2 y

dt^2

dy

dt

  • y = 0; y(2) = 1, y ′ (2) = 1.

Solution: (10 points) This is a second-order, linear homogeneous problem with constant coefficients. So, we look for solutions of the form y = e rt :

r 2 − 6 r + 1 = 0 =⇒ r = 3 ± 2

Let us name r 1 = 3 − 2

2 and r 2 = 3 + 2

  1. Noting that the initial time is 2, the general solution is

y(t) = c 1 e r 1 (t−2)

  • c 2 e r 2 (t−2) .

So, by the initial conditions, we have

1 = y(2) = c 1 + c 2

1 = y ′ (2) = r 1 c 1 + r 2 c 2.

If we multiply the first equation by r 1 and subtract the second equation from the first, then

(r 1 − r 2 )c 2 = r 1 − 1 =⇒ c 2 =

r 1 − 1

r 1 − r 2

So,

c 1 = 1 − c 2 =

1 − r 2

r 1 − r 2

Plugging back in r 1 and r 2 , we can find y(t):

y(t) =

1 − r 2

r 1 − r 2

e (3− 2

√ 2)(t−2)

r 1 − 1

r 1 − r 2

e (3+

√ 2)(t−2)

e (3− 2

√ 2)(t−2)

e (3+

√ 2)(t−2)

e −6+

√ 2 e (3− 2

√ 2)t

e − 6 − 4

√ 2 e (3+

√ 2)t .

Section 2.2 (p. 144) Problems

  1. Find the general solution of

t^2

d^2 y

dt^2

  • 2t

dy

dt

  • 2y = 0, t > 0.

Solution: (10 points) This is a second-order, linear homogeneous equation, and it’s an Euler’s equation. So, we look for solutions of the form y = tr:

t 2 r(r − 1)t r− 2

  • 2trt r− 1
  • 2t r = t r

r 2

  • r + 2

Document URL: http://math.uci.edu/~pmacklin/Math3Dwinter2006.html Date: February 22, 2006

Page 1 of 2

The roots of the polynomial are r = − 1 2 ±^ i

√ 7

  1. Let’s find two solutions:

t r = t − 12 +i

√ 7 2

= t − (^12) t i

√ 7 2

= t − (^12) e

ln

 ti

√ 7 2



= t − (^12) e i

√ 7 2 ln^ t

= t − (^12)

cos

ln t

  • i sin

ln t

Because this is a complex-valued solution, the real and imaginary parts are two independent solutions. So, the general solution is

y(t) = c 1 t − (^12) cos

ln t

  • c 1 t − (^12) sin

ln t

Completeness Points

(5 points) 1 2 point per seriously-attempted, assigned problem.

Document URL: http://math.uci.edu/~pmacklin/Math3Dwinter2006.html Date: February 22, 2006

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