Differential equations and linear algebra 2nd edition farlow solutions manual

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Differential

CHAPTER 2 Linearity and Nonlinearity

2.1 Linear Equations: The Nature of Their Solutions

Classification

1. First-order, nonlinear

2. First-order, linear, nonhomogeneous, variable coefficients

3. Second-order, linear, homogeneous, variable coefficients

4. Second-order, linear, nonhomogeneous, variable coefficients

5. Third-order, linear, homogeneous, constant coefficients

6. Third-order, linear, nonhomogeneous, constant coefficients

7. Second-order, linear, nonhomogeneous, variable coefficients

8. Second-order, nonlinear

9. Second-order, linear, homogeneous, variable coefficients

10. Second-order, nonlinear

Linear Operation Notation

11. Using the common differential operator notation that D(y) = dy dt , we have the following:

(a) 30ytyy′′′+−= can be written as L(y) = 0 for L = D2 + tD 3.

(b) y ′ + y 2 = 0 is not a linear DE.

(c) y ′ + sin y = 1 is not a linear DE.

(d) y ′ + t2 y = 0 can be written as L(y) = 0 for L = D + t2

92
Differential Equations and Linear Algebra 2nd Edition Farlow Solutions Manual Visit TestBankDeal.com to get complete for all chapters

(e) y ′ + (sin t)y = 1 can be written as L(y) = 1 for L = D + sin t

(f) 3 yyy ′′′−+ = sin t can be written as L(y) = sin t for L = D2 3D + 1.

Linear and Nonlinear Operations

12. ( ) 2 Lyyy ′ =+

Suppose 12 , yy and y are functions of t and c is any constant. Then

Hence, L is a linear operator.

13. ( ) 2 Lyyy ′ =+

To show that ( ) 2 Lyyy ′ =+ is not linear we can pick a likely function of t and show that it does not satisfy one of the properties of linearity, equations (2) or (3). Consider the function yt = and the constant 5 c = :

Hence, L is not a linear operator.

14. ( ) 2 Lyyty ′ =+

Suppose 12 , yy and y are functions and c is any constant.

Hence, L is a linear operator. This problem illustrates the fact that the coefficients of a DE can be functions of t and the operator will still be linear.

SECTION 2.1 Linear Equations: The Nature of Their Solutions 93
()()() ()() () ()()() ()() 121212 1122 12 2 22 22 2 Lyyyyyy yyyy Lyy Lcycycycycy cyycLy ′ +=+++ ′′ =+++ =+ ′ ′ =+=+ ′ =+=
()()() ()() 2 2 22 555525 5555 Ltttt tttLt ′ =+=+ ⎛⎞ ′ ≠+=+= ⎜⎟ ⎝⎠
()()() ()() ()() ()()()() () 121212 1122 12 2 22 22 Lyyyytyy ytyyty LyLy Lcycytcycyty cLy ′ +=+++ ′′ =+++ =+ ′ ′ =+=+ =

CHAPTER 2 Linearity and Nonlinearity

15. ( ) t Lyyey ′ =−

Suppose 12 , yy and y are functions of t and c is any constant.

Hence, L is a linear operator. This problem illustrates the fact that a linear operator need not have coefficients that are linear functions of t

16.

Hence, L is a linear operator. This problem illustrates the fact that a linear operator need not have coefficients that are linear functions of t.

Hence, ( ) Ly is not a linear operator.

94
()()() ()() ()() ()()() () () 121212 1122 12 t tt tt Lyyyyeyy yeyyey LyLy Lcycyecycyey cLy ′ +=+−+ ′′ =−+− =+ ′ ′ =−=− =
()()()() () {} () {} ()() ()()()() () {} () 121212 1122 12 sin sinsin sin sin Lyyyytyy ytyyty LyLy Lcycytcy cyty cLy ′′ +=+++ ′′′′ =+++ =+ ′′ =+ ′′ =+ =
( ) ( ) sin Lyyty ′′ =+
Lyyyyy
()()() { } () () {} () 2 2 1 1 Lcycycyycy cyyyy cLy ′′ ′ =+−+ ′′′ ≠+−+ =
17. ( ) ( ) 2 1
′′′ =+−+
Pop Quiz 18. () 2 1 21 2 t yyytce ′ +=⇒=+ 19. ( ) 22 t yyytce ′ + =⇒=+ 20. ( ) 0.08 0.081001250 t yyytce ′ −=⇒=− 21. () 3 5 35 3 t yyytce ′ =⇒=−

Superposition

Adding these equations gives

and multiplying by c we get

which shows that

Second-Order Superposition Principle

25. If 1y and 2y are solutions of

we have

Multiplying these equations by 1c and 2c respectively, then adding and using properties of the derivative, we arrive at

which shows that

+ is also a solution.

SECTION 2.1 Linear Equations: The Nature of Their Solutions 95 22. 51yy ′ += , ()() 5 1 10 5 t yytce=⇒=+ , () 5 1 10 5 yce =⇒=− . Hence, () () () 51 1 1 5 t yte =− 23. 24yy ′ += , ( ) ( ) 2 012 t yytce=⇒=+ , ( ) 011yc = ⇒=− . Hence, () 2 2 t yte =−
1y and 2y are solutions of ( ) 0 ypty ′ + = , then ( ) () 11 22 0 0. ypty ypty ′ + = ′ + =
Principle 24. If
( ) ( ) 1212 0 yyptypty ′′ + ++= or ()()() 1212 0 yyptyy ′ + ++= ,
12yy +
of the given equation.
1y is
( ) 11 0 ypty ′ + =
( ) ( ) () ()()() 11 11 11 0 0 0, cypty cycpty cyptcy ′ + = ′ + = ′ + =
which shows that
is also a solution
If
a solution, we have
1cy
is also a solution of the equation.
( ) ( ) 0 yptyqty ′′′ + += ,
( ) ( ) ()() 111 222 0 0. yptyqty yptyqty ′′′ + += ′′′ + +=
()()()()() 112211221122 0 cycyptcycyqtcycy ′′′ +++++= ,
1122 cycy

CHAPTER 2 Linearity and Nonlinearity

Thus, 3333 331212 9(99)9()0 tttt yycececece ′′ −=+−+=

c2 cos 2t, then 3122cos2(2sin2) yctct ′ = +−

312(4sin2)(4cos2) yctct ′′ = −+−

Thus, 331212 4(4sin2)(4cos2)4(sin2cos2)0 yyctctctct ′′ +=−+−++= .

28. 20; yyy′′′+−=

For y1 = e t/2 , /2

ye ′ =

Substituting: 11/2/2/2 20 42 ttt eee ⎛⎞ +−=

For y2 = e t , 2 , t ye ′ =− 2 t ye ′′ =

Substituting: ( ) ( ) 2 ttt eee +−− = 0.

For c1 and c2, let y = c1e t/2 + c2e t

Substituting: ()/2/2/2 121212 11 2 42 tttttt cececececece

= 0.

96
Verifying Superposition 26. 90;yy ′′ −= 3 1 t ye = ⇒ 3 1 3 t ye ′ = ⇒ 3 1 9, t ye ′′ = so that 33 119990 tt yyee ′′ =−= 3 2 t ye = ⇒ 3 2 3 t ye ′ =− ⇒ 3 2 9, t ye ′′ = so that 33 229990 tt yyee ′′ =−= . Let y3 = c1y1 + c2y2 = c1e 3t + c2e 3t , then 333123(3)tt ycece ′ =+− 3331299tt ycece ′′ =+
y1 = sin 2t, 1 2cos2 yt ′ = ⇒ 1 4sin2,yt ′′ = so that 1144sin24sin20 yytt ′′ + =−+= .
y2 = cos 2t, 2 2sin2 yt ′ =− ⇒ 2 4cos2, yt ′′ = so that 2244cos24cos20
=−+= .
y3
27. 40;yy ′′ += For
For
yytt ′′ +
Let
= c1 sin 2t +
1 1 2 t
,
1 1 4 t
/2
ye ′′ = .
⎜⎟ ⎝⎠ .
⎛⎞⎛⎞ ⎜⎟⎜⎟++−−+ ⎝⎠⎝⎠

29. 560yyy ′′′−+=

For y1 = e 2t , 2 1 2 t ye ′ = , 2 1 4 t ye ′′ =

Substituting: 222 45(2)6()0 ttt eee−+= .

For y2 = e 3t , 3 2 3, t ye ′ = 3 2 9 t ye ′′ = .

Substituting: 333 95(3)60 ttt eee−+=

For y = c1e 2t + c2e 3t , ( ) ( ) 232323 121212 564952360 tttttt yyycececececece ′′′−+=+−+++=

30. 60yyy ′′′ −−=

Substituting: 33)3 (9)(3)6()0 ttt eee−−= For

Substituting: 222 (4)(2)60 ttt eee−−−=

For y = c1e 3t + c

e

t ( ) ( ) ( ) 323233 12112 6943260 tttttt yyycececeecece ′′′−−=+−−−+=

31. 90yy ′′ −=

For y1 = cosh 3t, 1 3sinh3 yt ′ = 1 9cosh3 yt ′′ = .

Substituting: (9cosh3)9(cosh3)0 tt−=

For y2 = sinh 3t, 2 3cosh3, yt ′ = 2 9sinh3 yt ′′ = .

Substituting: (9sinh3)9(sinh3) tt = 0.

For y = c1 cosh 3t + c2 sinh 3t, ( ) ( )

1212 99cosh39sinh39cosh3sinh30 yyctctctct ′′ −=+−+=

SECTION 2.1 Linear Equations: The Nature of Their Solutions 97
3 1
t
3 1 9 t
′′
For y1 = e 3t ,
3,
ye ′ =
ye
=
2
2t
2 2 2, t
2 2 4 t ye ′′ =
y
= e
,
ye
=−
2
3

CHAPTER 2 Linearity and Nonlinearity

Different Results?

32. The solutions of Problem 31, cosh 3t

are linear combinations of the solutions of Problem 26 and vice-versa,

Many from One

33. Because ( ) 2 ytt = is a solution of a linear homogeneous equation, we know by equation (3) that 2 ct is also a solution for any real number c

Guessing Solutions

We can often find a particular solution of a nonhomogeneous DE by inspection (guessing). For the firstorder equations given for Problems 27–31 the general solutions come in two parts: solutions to the associated homogeneous equation (which could be found by separation of variables) plus a particular solution of the nonhomogeneous equation. For second-order linear equations as Problems 32–35 we can also sometimes find solutions by inspection.

Nonhomogeneous Principle

In these problems, the verification of p y is a straightforward substitution. To find the rest of the solution we simply add to p

all the homogeneous solutions yh , which we find by inspection or separation of variables.

98
333 2 tt e + and sinh
t = 33 2 tt ee ,
=
3
i.e., e 3t = cosh 3t + sinh 3t and e 3t = cosh 3t sinh 3t.
34.
2 ttt yyeytcee ′ +=⇒=+ 35. ( ) ttt yyeytcete ′ +=⇒=+ 36. ( ) ttt yyeytcete ′ −=⇒=+ 37. () 2 2 0 t ytyytce ′ −=⇒= 38. () 4 3 5ytytyct tt ′ +=⇒=+ 39. ( ) 2 12 0 yayytceceatat ′′ −=⇒=+ . An alternative form is ( ) ( ) ( ) 12 sinhcosh ytcatcat =+ . 40. ( ) 2 12 0sincos yayytcatcat ′′ +=⇒=+ 41. ( ) 12 0 t yyytcce ′′′+=⇒=+ 42. ( ) 12 0 yyytccet ′′′−=⇒=+
() 1
43. 3 t yye ′ −= has general solution ()3tt hp ytyycete =+=+ . 44. 210sin yyt ′ += has general solution ( ) 2 4sin2cos t hp ytyycett =+=+− . 45. 2 2 yyy t ′ −= has general solution ( ) 23 hp ytyyctt = +=+ .
y

46. 1 2 1 yy t ′ += + has general solution () 2 2 11 hp ctt ytyy tt + =+=+ + + .

Third-Order Examples

47. (a) For y1 = e t, we substitute into 0 yyyy ′′′′′′−−+= to obtain e t e t e t + e t = 0.

For y2 = tet, we obtain 2 , yteett ′ = + 2 (), ttt yteee ′′ = ++ 2 ()2, ttt yteee ′′′ =++ and substitute to verify

(tet + 3e t) (tet + 2et) (tet + e t) + tet = 0.

For y3 = e t, we obtain 333,,, ttt yeyeye ′′′′′′ =−==− and substitute to verify

()()()tttt eeee −−−+ = 0.

(b) yh = c1e t + c2tet + c3e t

(c) Given yp = 2t +

To verify:

tttt

′′′′′′−−+=−−++++

pppp

=−+

84(22)(21) 213 (d) y(t) = yh + yp = c1e t + c2tet + c3e t + 2t + 1 + e 2t

SECTION
Linear
of Their
99
2.1
Equations: The Nature
Solutions
2
2
t p ye ′ =+ 2 4 t p ye ′′ = 2 8 t p ye ′′′ =
1 + e
t :
22
2
t
2222
yyyyeeete te

(e) 2 123()22 ttttt ycecteecee ′ =++−++

123(2)4 ttttt ycecteecee ′′ =++++ y

23 233 cc cc +=−

⎫ ⎬ +=−

(a) For y1 = e t, we obtain by substitution

0 tttt yyyyeeee ′′′′′′+−−=+−−=

()()0tttt yyyyeeee ′′′′′′+−−=−+−−−=

For y = te t we obtain by substitution

(3)(2)()0 ttttttt yyyyteeteeteete ′′′′′′+−−=−++−−−+−= .

(b) yh = c1e t + c2e t + c3te t

(c) Given yp = cos t sin t 3: sincos p ytt ′ =−−

cossin p ytt ′′ =−+

sincos p ytt ′′′ =+

To verify:

(sincos)(cossin)(sincos)(cossin3) 4sin3 pppp yyyytttttttt t ′′′′′′+−−=++−+−−−−−− =+

(d) y(t) = yh + yp = c1e t + c2e t + c3te t + cos t sin t 3

100
CHAPTER 2 Linearity and Nonlinearity
(0)
c1 + c3 + 2 ⇒ c1 + c3 = 1 Equation
y ′ = 2 = c1 + c2 c3 + 4 ⇒ c1 + c2 c3 = 2 Equation (2) (0) y ′′ = 3 = c1 + 2c2 + c3 + 4 ⇒ c1 + 2c2 + c3 = 1 Equation (3)
2
= 1 =
(1) (0)
⎭ ⇒ c2 =
Add Equation (2) to (1) and (3) 12 12 c1 = 3 2 , c3 = 1 2 .
0,
Thus, y = 2 31 21. 22 ttt eete −++++ 48. 4sin3yyyyt ′′′′′′+−−=+
For y = e t, we obtain by substitution
SECTION 2.1 Linear Equations: The Nature of Their Solutions 101 (e) 123 ()sincostttt ycececteett ′ =−+−+−− 123 (2)cossintttt ycececteett ′′ =++−−+ y(0) = 1 = c1 + c2 + 1 3 ⇒ c1 + c2 = 3 Equation (1) (0) y ′ = 2 = c1 + c2 c3 1 ⇒ c1 c2 + c3 = 3 Equation (2) (0) y ′′ = 3 = c1 + c2 2c3 1 ⇒ c1 + c2 2c3 = 4 Equation (3) Add Equation (2) to (1) and (3) 13 13 26 27 cc cc += ⎫ ⎬ −= ⎭ ⇒ c1 = 13 4 , c2 = 1 , 4 c3 = 1 . 2 y(t) = 1311 cossin3 442 ttt eetett −+−− . Suggested Journal Entry 49. Student Project

2.2 Solving the First-Order Linear Differential Equation General Solutions

The solutions for Problems 1–15 can be found using either the Euler-Lagrange method or the integrating factor method. For problems where we find a particular solution by inspection (Problems 2, 6, 7) we use the Euler-Lagrange method. For the other problems we find it more convenient to use the integrating factor method, which gives both the homogeneous solutions and a particular solution in one swoop. You can use the Euler-Lagrange method to get the same results.

1. 20yy ′ +=

By inspection we have ( ) 2 t ytce =

2. 23 t yye ′ +=

We find the homogeneous solution by inspection as 2 t h yce = . A particular solution on the nonhomogeneous equation can also be found by inspection, and we see t p ye = . Hence the general solution is ( ) 2 ytceett =+

3. 3 t yye ′ −=

We multiply each side of the equation by the integrating factor

We multiply each side of the equation by the integrating factor ( ) t te μ

102 CHAPTER 2 Linearity and Nonlinearity
() ()() 1 ptdtdt t teee μ ∫∫ === giving ( ) 3 t eyy ′ −= , or simply () 3 t d ye dt = . Integrating, we
3 t yetc =+ , or ( ) 3 tt ytcete =+ .
find
yyt
4. sin
′ +=
,
() sin tt eyyet ′ += , or, () sin tt d yeet dt = .
we
() 1 sincos 2 tt yeettc =−+ .
for
() 11 sincos 22 t ytcett =+−
=
giving
Integrating by parts,
get
Solving
y, we find

5. 1 1 t yy e ′ += +

We multiply each side of the equation by the integrating factor ( ) t te μ = , giving

Integrating, we get ( ) ln1 tt yeec =++

Hence, () ( ) ln1 ttt ytceee =++ .

6. 2 ytyt ′ +=

In this problem we see that () 1 2 p yt = is a solution of the nonhomogeneous equation (there are other single solutions, but this is the easiest to find). Hence, to find the general solution we solve the corresponding homogeneous equation, 20yty ′ + = , by separation of variables, getting

=− , which has the general solution

t yce = , where c is any constant. Adding the solutions of the homogeneous equation to the particular solution 1 2 p y = we get the general solution of the nonhomogeneous equation:

7. 22 3 ytyt ′ +=

In this problem we see that () 1 3 p yt = is a solution of the nonhomogeneous equation (there are other single solutions, but this is the easiest to find). Hence, to find the general solution, we solve the corresponding homogeneous equation, 2 30yty ′ + = , by separation of variables, getting

3 dy tdt y =− , which has the general solution () 3 t ytce = , where c is any constant. Adding the solutions of the homogeneous equation to the particular solution 1 3 p y = , we get the general solution of the nonhomogeneous equation

ytce = +

3 1 3

SECTION 2.2 Solving the First-Order Linear Differential Equation 103
() () ,
. 11 tt tt tt ede eyyye dt ee ′ +== ++
or,
2
()
t
dy tdt y
2
2 1 2
ytce = +
2
()
t

CHAPTER 2 Linearity and Nonlinearity

8. 2 11 yy t t ′ += , ( ) 0 t ≠

We multiply each side of the equation by the integrating factor () ln dtt t teet μ ∫ = == , giving () 111 , or, . d tyytyttdtt

Integrating, we find ln tytc =+

Solving for y, we get () 1 ln c ytt tt

9. 2 tyyt ′ +=

We rewrite the equation as 1 2 yy t ′ += , and multiply each side of the equation by the integrating factor () ln dtt t teet μ ∫ === , giving () 1 2, or, 2. d tyyttyt

Integrating, we find 2 tytc =+

Solving for y, we get () c ytt t =+ .

10. ( ) cossin1 tyty ′ +=

We rewrite the equation as ( ) tansec ytyt ′ += , and multiply each side of the equation by the integrating factor ()

()() 1 lncoslncos tan sec tt tdt teeet μ ∫ ==== , giving () () () () sectansec,22 or, secsec. d tytyttyt dt ′ +==

Integrating, we find ( ) sectantytc =+ . Solving for y, we get ( ) cossin ytctt =+

104
⎛⎞
⎜⎟ ⎝⎠
′ + ==
⎜⎟ ⎝⎠
⎛⎞ =+
⎛⎞ ′ ⎜⎟+== ⎝⎠
tdt

11.

We multiply each side of the equation by the integrating factor

We multiply each side of the equation by the integrating factor

We rewrite the equation as

and then multiply each side of the equation by the integrating factor

SECTION 2.2 Solving the First-Order Linear Differential Equation 105
2
−= , ( ) 0 t ≠
2 cos yytt t ′
() () 2 2 2lnln2 tdt tt teeet μ ∫ ==== , giving ()22 2 cos, or, cos. d tyyttyt tdt ⎛⎞ ′ ⎜⎟−== ⎝⎠
we
2 sin tytc =+ . Solving for y, we get ( ) 22 sin ytcttt =+ .
t ≠
Integrating,
find
12. 3 3sin t yy t t ′ += , ( ) 0
() () ( ) 3 ln 3 3ln3 t tdt t teeet μ ∫ = === , giving ()33 3 sin, or, sin. d tyyttyt tdt ⎛⎞ ′ ⎜⎟+== ⎝⎠ Integrating, we
3 cos tytc =−+ . Solving for y, we get () 33 1 cos c ytt tt =− .
find
13. ( ) 10 tt eyey ′ ++=
0 1 t t e yy e ⎛⎞ ′ + = ⎜⎟ + ⎝⎠ ,
() ( ) ( ) 1ln1 1 ttt eedte t teee μ ++ ∫ = ==+ , giving () ( ) 10 t d ey dt + =
t
() 1 t c yt e = + .
Integrating, we find ( ) 1
eyc+= . Solving for y, we have

CHAPTER 2 Linearity and Nonlinearity

14. ( ) 2 90tyty ′ ++=

We rewrite the equation as 2 0

and then multiply each side of the equation by the integrating factor

We multiply each side of the equation by the integrating factor

Initial-Value Problems

16. 1 yy ′ −= , ( ) 01 y =

By inspection, the homogeneous solutions are t h yce = . A particular solution of the nonhomogeneous can also be found by inspection to be 1 p y = . Hence, the general solution is

Substituting ( ) 01 y = gives 11 c −= or 2 c = . Hence, the solution of the IVP is

106
t
⎛⎞ ′ += ⎜⎟ + ⎝⎠
9
yy t
,
() ( ) () ( ) 22912ln9 2 9 ttdtt teet μ ++ ∫ ===+ , giving ( ) 2 90 d ty dt += Integrating, we find 2 9 tyc += . Solving for y, we find () 2 9 c yt t = + 15. 21 2 t yyt t + ⎛⎞ ′ += ⎜⎟ ⎝⎠ , ( ) 0 t ≠
() 2 211 2 t t tdtdtte tt μ + ==+= ∫∫ , giving ()222 2 tt d teyte dt = Integrating, we find 22222 1 2 tttt teyteteec =−++ Solving for y, we have () 2 1 1 2 t e ytct tt ⎛⎞ =++− ⎜⎟ ⎝⎠
1 t hp yyyce
.
= +=−
( )
t yte
21
=

17. 3 2 ytyt ′ += , ( ) 11 y =

We can solve the differential equation using either the Euler-Lagrange method or the integrating factor method to get () 2 2 11 22 t yttce =−+ .

Substituting ( ) 11 y = we find 1 1 ce = or c = e. Hence, the solution of the IVP is () 2 1121 22 t ytte =−+ .

18. 3 3 yyt t ⎛⎞ ′ −= ⎜⎟ ⎝⎠ , ( ) 14 y =

We find the integrating factor to be () () 3 3 3lnln3 tdt tt teeet μ ∫ = ===

Multiplying the DE by this, we get () 3 1 d ty dt =

Hence, 3 tytc =+ , or, 34 () ytctt = +

Substituting ( ) 14 y = gives 14 c + = or 3 c = . Hence, the solution of the IVP is ( ) 34 3 yttt = + .

19. 2 ytyt ′ += , ( ) 01 y =

We solved this differential equation in Problem 6 using the integrating factor method and found () 2 1 2 t ytce = +

Substituting ( ) 01 y = gives 1 1 2 c + = or 1 2 c = . Hence, the solution of the IVP is () 2 11 22 t yte = +

20. ( ) 10 tt eyey ′ ++= , ( ) 01 y =

We solved this DE in Problem 13 and found () 1 t c yt e = +

Substituting ( ) 01 y = gives 1 2 c = or 2 c = . Hence, the solution of the IVP is () 2 1 t yt e = +

SECTION 2.2 Solving the First-Order Linear Differential Equation 107

CHAPTER 2 Linearity and Nonlinearity

Synthesizing Facts

21. (a) () ()

(b) ( ) ( ) 1, 1 yttt=+>−

(c) The algebraic solution given in Example 1 for 1 k = is

(d) The solution passing through the origin ( ) 0, 0 asymptotically approaches the line 1 yt=+ as t →∞ , which is the solution passing through ( ) 01 y = . The entire line 1 yt=+ is not a solution of the DE, as the slope is not defined when 1 t =− . The segment of the line 1 yt=+ for 1 t >− is the solution passing through ( ) 01 y = .

On the other hand, if the initial condition were ( ) 54 y =− , then the solution would be the segment of the line 1 yt = + for t less than –1. Notice in the direction field the slope element is not defined at ( ) 1, 0 .

Using Integrating Factors

In each of the following equations, we first write in the form ( ) ( ) yptyft

and then identify ( ) p

108
2 2 , 1 1 tt ytt t + =>− +
() ( ) 2 2 1 21 11 t tt yt tt + ++ == ++ .
when 1 t ≠−
yt = + . –3 3 y 3 t –3
Hence,
we have 1
+=
t 22. 20yy ′ += Here ( ) 2 pt = , therefore the integrating factor is () () 2 2 ptdtdt t teee μ ∫∫ = == Multiplying each side of the equation 20yy ′ + = by 2 t e yields () 2 0 t d ye dt = Integrating gives 2 t yec = . Solving for y gives ( ) 2 t ytce = 23. 23 t yye ′ += Here ( ) 2 pt = , therefore the integrating factor is () () 2 2 ptdtdt t teee μ ∫∫ = == Multiplying each side of the equation 23 t yye ′ += by 2 t e yields ()23 3 tt d yee dt = Integrating
23 tt yeec =+
Solving for y
( ) 2 ytceett = +
gives
.
gives

24. 3t yye ′ −=

Here ( ) 1 pt =− , therefore the integrating factor is () () ptdtdt t teee μ ∫∫ ===

Multiplying each side of the equation 3t yye ′ = by t e yields () 2 tt d yee dt = .

Integrating gives 2 1 2 tt yeec =+ . Solving for y gives () 3 1 2 ytceett =+ .

25. sin yyt ′ +=

Here ( ) 1 pt = therefore the integrating factor is () () ptdtdt t teee μ ∫∫ = == .

Multiplying each side of the equation sin yyt ′ + = by t e gives () sin tt d yeet dt =

Integrating gives () 1 sincos 2 tt yeettc =−+ . Solving for y gives () () 1 sincos 2 t ytttce =−+

26. 1 1 t yy e ′ += +

Here ( ) 1 pt = therefore the integrating factor is () () ptdtdt t teee μ ∫∫ = == .

Multiplying each side of the equation 1 1 t yy e ′ += + by t e yields () 1

t t t de ye dt e = +

Integrating gives ( ) ln1 tt yeec =++ . Solving for y gives () ( ) ln1 ttt yteece =++ .

27. 2 ytyt ′ +=

Here ( ) 2 p tt = , therefore the integrating factor is () () 2 2 ptdttdt t teee μ ∫∫ = == .

Multiplying each side of the equation 2 ytyt ′ + = by 2 t e yields ( ) 22 tt d yete dt = .

Integrating gives 22 1 2 tt yeec =+ . Solving for y gives () 2 1 2 t ytce = +

Solving
First-Order
SECTION 2.2
the
Linear Differential Equation 109

110 CHAPTER 2 Linearity and Nonlinearity

28. 22 3 ytyt ′ +=

Here () 2 3 p tt = , therefore the integrating factor is () () 2 3 3 ptdttdt t teee μ ∫∫ === .

Multiplying each side of the equation 22 3 ytyt ′ + = by 3 t e yields ( ) 33 2 tt d yete dt = .

Integrating gives 33 1 3 tt yeec =+ . Solving for y gives () 3 1 3 t ytce = + .

29. 2 11 yy t t ′ +=

Here () 1 pt t = , therefore the integrating factor is () () () 1 ln ptdttdt t teeet μ ∫∫ = ===

Multiplying each side of the equation 2 11 yy t t ′ + = by t yields

() 1 d ty dtt =

Integrating gives ln tytc =+ . Solving for y gives () 11 ln ytct tt =+

30. 2 tyyt ′ +=

Here () 1 pt t = , therefore the integrating factor is () () () 1 ln ptdttdt t teeet μ ∫∫ = ===

Multiplying each side of the equation 2 y y t ′ + = by t yields () 2 d tyt dt = .

Integrating gives 2 tytc =+ . Solving for y gives () 1 ytct t = +

Switch for Linearity 1 dy dtty = + , ( ) 10 y =

31. Flipping both sides of the equation yields the equivalent linear form dt ty dy = + , or dt ty dy −=

Solving this equation we get ( ) 1 y tycey=−−

Using the condition ( ) 10 y −= , we find 0 11 ce =− , and so 0 c = . Thus, we have 1 ty=−− and solving for y gives ( ) 1 ytt =

The Tough Made Easy 2 2 y dyy dt ety =

32. We flip both sides of the equation, getting 2 2 , y dtety dy y = or, 2 2 y dte t dyy y +=

We solve this linear DE for ( ) ty getting () 2

y ec ty y + = .

A Useful Transformation

33. (a) Letting ln zy = , we have z ye = and z dydz e dtdt =

Now the equation ln dy aybyy dt += can be rewritten as zzz dz eaebze dt += .

Dividing by z e gives the simple linear equation dz bza dt =− .

Solving yields bt a zce b =+ and using ln zy = , the solution becomes () ()abcebt yte + = .

(b) If 1 ab== , we have () ( ) 1 t ce yte + = .

Note that when 0 c = we have the constant solution ye = .

Bernoulli Equation ( ) ( ) yptyqtyα ′ += , 0

34. (a) We divide by y α to obtain 1 ()() yyptyqt αα ′ += .

Let 1 vy α = so that (1) a vyy α ′ ′ =− and 1 a v yy α

′ ′ = .

Substituting into the first equation for 1 y α and yy α ′ , we have ()() 1 v p tvqt α

′ += , a linear DE in v, which we can now rewrite into standard form as (1)()(1)() vptvqt α α ′ + −=− .

SECTION 2.2
111
Solving the First-Order Linear Differential Equation
1 α ≠
α
,

(b) 3 α = , ( ) 1 pt =− , and ( ) 1 qt = ; hence 22 dv v dt + =− , which has the general solution

( ) 2 1 t vtce =−+

Because 2 1 v y = , this yields () ( ) 12 2 1 t ytce =−+ .

Note, too, that 0 y = satisfies the given equation.

(c) When 0 α = the Bernoulli equation is

()() dy p tyqt dt += ,

which is the general first-order linear equation we solved by the integrating factor method and the Euler-Lagrange method.

When 1 α = the Bernoulli equation is

()() dy p tyqty dt += , or, ()() () 0 dy ptqty dt + −= ,

which can be solved by separation of variables.

112
CHAPTER 2 Linearity and Nonlinearity
Practice 35. 3 ytyty ′ += or 32 yytyt ′ +=
v = y 2 , so dv dt = 3 2 dy y dt .
in the DE gives 1 , so that 2 dv tvt dt −+= 22, dv tvt dt =− which is linear in v, with integrating factor μ = 2 2 tdt t ee ∫ =
Bernoulli
Let
Substituting
dt
222
2 1 t vce =+
back for v gives 2 2 1 , 1 t y ce = + hence 2 1 (). 1 t yt ce =± +
Thus, 222 22 ttt dv etevte
−=− , and
2,ttt evtedtec = −=+
so
. Substituting
SECTION 2.2 Solving the First-Order Linear Differential Equation 113
2 t yyey ′ −= , so that 21 t yyye ′ =
v = y 1 , so 2 dvdy y dtdt =− .
in the DE gives t dv ve dt + =− , which is linear in v with integrating factor dt t ee μ ∫ = = . Thus 2 ttt dv eeve dt +=− , and 2 2 2 t tt e evedtc = −=−+ ∫ , so 2 t t e vce =−+ . Substituting back for v gives 1 1 1 2 , or () 2 t t tt e yceyt ece =−+= −+
24 23 tytyy ′ −= or 42323ytyty ′ = , t ≠ 0
v = y 3 , so 4 3 dvdy y dtdt =− .
in the DE gives 2 1 23 3 dv ttv dt −−= , or, 2 69 dv dtt t + =− , which is linear in v, with integrating factor μ = 6 6ln6 dt t t eet ∫ = = Thus 654 69 dv ttvt dt +=− , and 645 9 9 5 tvtdttc = −=−+ ∫ , so 5 9 5 vct t =−+ . Substituting back for v gives 3 6 9 5 c y t t =−+ . Hence 6 3 5 6 15 , 9 95 5 t y c tc t t == −+ −+ so 2 3 5 1 5 () 9 ytt ct = .
22 (1)0 tytyty ′ −−−= (Assume 1 t < ) 221 (1) ytytyt ′ −−= Let v = y 1 , so 2 dvdy y dtdt =−
in the DE gives 2 (1), dv ttvt dt −−−= so that 22 , 11 dvtt v dt tt += which is linear in v, with integrating factor 2 1 t dt t e μ ∫ = 2 1 ln(1) 2 t e = = (1)21/2 t .
36.
Let
Substituting
37.
Let
Substituting
38.
Substituting

CHAPTER 2

Linearity and Nonlinearity

Thus, 21/223/223/2 (1)(1)(1) dv tttvtt

−+−=− , and

Hence v = 1 + c(1 t2)1/2 and substituting back for v gives y(t) = 1/2 1 1(1) ct+−

39. 2 yy y tt ′ += y(1) = 2 3 2 1 y yy tt ′ +=

Let v = y 3 , so 2 3.dvdy y dtdt =

Substituting in the DE gives

which is linear in v, with integrating factors

Thus, 322 33 dv ttvt dt += , and

Substituting back for v gives 33 1 yct =+ or 3 3 ()1. ytct =+

For the IVP we substitute the initial condition y(1) = 2, which gives 23 = 1 + c, so c = 7.

Thus, y 3 = 1 + 7t 3 and 3 3 ()17. ytt =+

40. 23 3210 yyyt ′ −−−=

Let v = y 3 , so 2 3 dvdy y dtdt = , and 21 dv vt dt =+ ,

which is linear in v with integrating factor

114
dt
21/2 23/23/2 1/2 1/221/2 1 (1) 2 (1) 1 1 2 2 (1) tdtdw tv tw w c wctc −==− =−+ ⎛⎞ ⎜⎟ ⎝⎠ =+=−+ ∫∫ 2 (Substitute 1 2 1 ) 2 wt dwtdt dwtdt =− =− −=
111
dv v dttt +=
or 33 dv v dttt + = ,
3
,
3/ 3ln3 tdt t eet μ ∫ = == .
3 tvtdttc ==+ ∫ , so 3 1.vct =+
323
2 2 dt t
ee μ
== .

Thus, 222 2(1) ttt dv eevte

−=+ , and 22 (1) tt evtedt =+

by parts)

Hence v = 11322 . 2424 tttt cece + −−+=−−+

Substituting

For the IVP, substituting the initial condition y(0) = 2 gives 8 =

Hence, y 3 = 2 335 244 t t e −−+ , and 2 3 335 (). 244 t t yte =−+

Equation ( ) ( ) ( ) 2 yptqtyrty ′ =++

41. (a) Suppose 1y satisfies the DE so that

Now, if we require, as suggested, that v satisfies the linear equation

then substituting in the previous equation gives

Hence, 1 1 yy v =+ satisfies the Ricatti equation as well, as long as v satisfies its given equation.

SECTION 2.2 Solving
First-Order
115
the
Linear Differential Equation
ee
dt
∫ 22 (1). (Integration
24 tt
tc =−+−+
back for v gives y 3 = 2 3 24 t t ce −−+
3
c
c
4
+ ,
= 35 4 .
Ricatti
()()() 2 1 11 dy p tqtyrty dt =++ . If
1 1 yy v = + ,
1 2 1 dy dydv dtdtdt v ⎛⎞ =− ⎜⎟ ⎝⎠
()()() 2 11 2 1 dydv ptqtyrty dtdt v ⎛⎞ =++− ⎜⎟ ⎝⎠
we define a new variable
then
Substituting for 1dy dt yields
()() () () 1 2 dv qtrtyvrt dt =−+−
()()() ( ) ( ) ( ) 1 2 11 2 2 qtrtyrt dy ptqtyrty dtvv v =+++++ ,
simplifies to ()() () ()()() 22 1 11 2 11 2 y dy p dtvvtqtyrtyptqtyrty v ⎛⎞ ⎛⎞ ⎛⎞ =+++++=++ ⎜⎟ ⎜⎟ ⎜⎟ ⎝⎠ ⎝⎠ ⎝⎠
,
which

(b) 2 12 yyy ′ =−+−

Let 1 1 y = so 1 0 y ′ = , and substitution in the DE gives 2 11 0121210 yy = −+−=−+−= .

Hence, 1y satisfies the given equation. To find v and then y, note that (

Now find v from the assumed requirement that

which reduces to 1

. This gives

(b) ( ) 2 t h ytce = , 11 24 p yt=−

The general solution is

The curves in the figure in part (a) are labeled for different values of c.

(c) The homogeneous solution yh is transient because 0 yh → as t →∞ . However, although all solutions are attracted to p y , we would not call p y a steady-state solution because it is neither constant nor periodic; p y →∞ as t →∞ .

116 CHAPTER 2 Linearity
and Nonlinearity
) 2 qt
( ) 1 rt
) 1 pt = , (
= ,
= .
()() () ()22111 dv v dt = −+−−− ,
dt
( ) vttc = + ,
() 1 11 1 yty vtc =+=+ + Computer Visuals 42. (a) 2 yyt ′ += –5 5 y 5 –5 t yx=−05025 ..
dv
=
hence
2
t hp ytyycet
()
11 24
= +=+− .

(c) There is no steady-state solution because all solutions (including both yh and p y ) go to ∞ as t →∞ . The c values are approximate: {0.5, –0.8, –1.5, –2, –2.5, –3.1} as counted from the top-most curve to the bottom-most one.

The

The curves in the figure in part (a) are labeled for different values of c.

(c) The sinusoidal steady-state solution 11 sincos 22 p ytt =−

occurs when 0 c = . Note that the other solutions approach this solution as t →∞ .

SECTION 2.2 Solving the First-Order Linear Differential Equation 117 43. (a) 3t yye ′ −= (b) ( ) t h ytce = , 3 1 2 t p ye = .
() 3 1 2 h p tt hp y y ytyycee =+=+ 3 –3 t –3 3 y c = –2
The general solution is
44. (a) sin yyt ′ += 6 –6 t –2 2 y c=-0.002 (b) ( ) t h ytce = , 11 sincos 22 p ytt =− .
sincos
ytyycett
general solution is () 11
22 t hp
=+=+− .

(b) ( ) t h ytce = , () 1 sin22cos2 5 p ytt =−

The general solution is () sin22cos2

(c) The steady-state solution is p y , which attracts all other solutions. The transient solution is yh

(b) This equation is homogeneous. The general solution is () 2 t h ytce =

(c) The equation has steady-state solution 0 y = . All solutions tend towards zero as t →∞

118
Nonlinearity 45. (a) sin2 yyt ′ += 6 –6 t –2 2 y
CHAPTER 2 Linearity and
h p
y tt
5
t y
ytce=+
46. (a)
+= –2 2 y c = –2 c = 2 c = –1 c = 1 c = 0 2 –2 t
20yty ′

The approximate c values corresponding to the curves in the center counted from top to bottom, are {1;

2; –2}

and approximately 50,000 (left curve) and –50,000 (right curve) for the side curves.

(c) The steady-state solution is ( ) 0 yt = , which is not equal to p y . Both yh and p y are transient, but as t →∞ , all solutions approach 0.

Computer Numerics

48. 2 yyt ′ += , ( ) 01 y =

(a) Using step size 0.1 h = and 0.01 h = and Euler’s method, we compute the following values. In the latter case we print only selected values.

119 47. (a) 21yty ′ += –4 4 y 4 –4 t
SECTION 2.2 Solving the First-Order Linear Differential Equation
–1;
() 2 t h ytce = , 22tt p yeedt = ∫ The general solution is () 222 h p ttt y y ytceeedt =+ ∫ .
(b)
Euler’s Method t ( ) = 0.1 yh ( ) = 0.01 yh T ( ) = 0.1 yh ( ) = 0.01 yh 0 1 1.0000 0.6 0.3777 0.4219 0.1 0.8 0.8213 0.7 0.3621 0.4039 0.2 0.65 0.6845 0.8 0.3597 0.3983 0.3 0.540 0.5819 0.9 0.3678 0.4029 0.4 0.4620 0.5071 1 0.3842 0.4158 0.5 0.4096 0.4552 By Runge-Kutta (RK4) we obtain ( ) 10.4192 y ≈
step size 0.1 h = .
for

CHAPTER 2 Linearity and Nonlinearity

(b) From Problem 42, we found the general solution of DE to be () 2 11 24 t ytcet = +−

Using IC ( ) 01 y = yields 5 4 c = . The solution of the IVP is ()

511 424 t ytet = +− , and to 4 places, we have

(c) The error for ( )1 y using step size 0.1 h = in Euler’s approximation is ERROR0.41920.38420.035 = −= Using step size 0.01 h = , Euler’s method gives ERROR0.41920.41580.0034 = −= , which is much smaller. For step size 0.1 h = , Runge-Kutta gives ( ) 10.4158 y = and zero error to four decimal places.

(d) The accuracy of Euler’s method can be greatly improved by using a smaller step size. The Runge-Kutta method is more accurate for a given step size in most cases.

(a) ( ) 19.5944 y ≈ by Euler’s method for step size 0.1 h = , ( ) 111.401909375 y ≈ by Runge-Kutta for step size 0.1 (correct to six decimal places).

(b) From Problem 24, we found the general solution of the DE to be

(c) The accuracy of Euler’s method can be greatly improved by using a smaller step size; but it still is not correct to even one decimal place for step size 0.01.

( ) 111.20206 y ≈ for step size 0.01 h =

(d) MORAL: Euler’s method converges ever so slowly to the exact answer—clearly a far smaller step would be necessary to approach the accuracy of the Runge-Kutta method.

120
2 511 10.4192
ye=+−≈
2
()
424
49. Sample analysis: 3t yye ′ −= , ( ) 01 y = , ( )1 y Exact solution is 3 0.50.5tt yee =+
( ) 111.4019090461656
, so
y = to thirteen decimal places.
3 1 2 tt ycee
=+

(a) Using step size 0.1 h = and 0.01 h = and Euler’s method, we compute the following values.

method using step size

places).

(b) From Problem 47, we found the general solution of DE to be () 222 ttt ytceeedt =+

Using IC ( ) 01 y = , yields 1 c = . The solution of the IVP is () 22 0 (1) t tu yteedu =+

and so to 10 places, we have ( ) 10.9059589485 y =

(c) The error for ( )1 y using step size 0.1 h = in Euler’s approximation is ERROR0.95170.90590.0458 = −= .

Using step size 0.01 h = , Euler’s method gives ERROR0.91020.90600.0043 = −= , which is much smaller. Using step size 0.1 h = in Runge-Kutta method gives ERROR less then 0.000001.

(d) The accuracy of Euler’s method can be greatly improved by using a smaller step size, but the Runge-Kutta method has much better performance because of higher degree of accuracy.

SECTION 2.2 Solving the First-Order Linear Differential Equation 121 50. 21yty ′ += , ( ) 01 y =
Euler’s Method t ( ) = 0.1 yh ( ) = 0.01 yh T ( ) = 0.1 yh ( ) = 0.01 yh 0 1 1.0000 0.6 1.2308 1.1780 0.1 1.1 1.0905 0.7 1.1831 1.1288 0.2 1.178 1.1578 0.8 1.1175 1.0648 0.3 1.2309 1.1999 0.9 1.0387 0.9905 0.4 1.2570 1.2165 1 0.9517 0.9102 0.5 1.2564 1.2084 ( ) 10.905958 y ≈ by
0.1 h = (correct
Runge-Kutta
to six decimal

CHAPTER 2 Linearity and Nonlinearity

Direction Field Detective

51. (a) (A) is linear homogeneous, (B) is linear nonhomogeneous, (C) is nonlinear.

(b) If 1y and 2y are solutions of a linear homogeneous equation,

ypty ′ + = , then (

11 0 ypty ′ += , and ( ) 22 0 ypty ′ + = . We can add these equations, to get

Because this equation can be written in the equivalent form

, then 12yy + is also a solution of the given equation.

(c) The sum of any two solutions follows the direction field only in (A). For the linear homogeneous equation (A) you plot any two solutions 1y and 2y by simply following curves in the direction field, and then add these curves, you will see that the sum 12yy + also follows the direction field. However, in equation (B) you can observe a straight line solution, which is 1 11 24yt =

If you add this to itself you get 111 1 2 2 yyyt + ==− , which clearly does not follow the direction field and hence is not a solution. In equation (C) 1 1 y = is a solution but if you add it to itself you can see from the direction field that 12 2 yy + = is not a solution.

Recognizing Linear Homogeneous DEs from Direction Fields

52. For (A) and (D): The direction fields appear to represent linear homogeneous DEs because the sum of any two solutions is a solution and a constant times a solution is also a solution. (Just follow the direction elements.)

For (B) , (C) , and (E): These direction fields cannot represent linear homogeneous DEs because the zero function is a solution of linear homogeneous equations, and these direction fields do not indicate that the zero function is a solution. (B) seems to represent a nonlinear DE with more than one equilibrium, while (C) and (E) represent linear but nonhomogeneous DEs.

Note: It may be helpful to look at textbook Figures 2.1.1 and 2.2.2.

Suggested Journal Entry

53. Student Project

122
( ) 0
( ) ( ) ( ) ( ) 1122 0 yptyypty ′′ + ++=
)
( ) () ( ) 1212 0 yyyy pt ′ + ++=

2.3 Growth and Decay Phenomena

1. (a) The half-life h t is the time required for the solution to reach

2. For doubling time d t , we solve 00 2 ktd yey = , which yields

3. If we examine the value of the decay curve

SECTION 2.3 Growth and Decay Phenomena 123
Half-Life
0 1 2 y . Hence, 00 1 2 kt yey =
1 ln2 h t k =−
( ) 0 kt ytye
1tt
( ) 1 10 kt ytyeB = = . Then
1 h ttt =+
() () () () 1 11 ln2ln12 ln2 1000 1 2 h h ktt kk kt ktkt h yttyeyeeyeeBeBeB + +======
Solving for h t , yields ln2 h kt = , or
(b) The solution to yky ′ = is
= so at time
= , we have
at
we have
Doubling Time
1 ln2 d t k = . Interpretation of 1 k
( ) 0 kt ytye
we find () () 1 1 000 0 1 0.3678794 . 3 kk yyeyey k y ⎛⎞ === ⎜⎟ ⎝⎠ ≈ … Hence, 1 k 0 y t 4 0.2 0.4 0.6 0.8 1 1 2 yye kt = 0 k = Š1 1/e 0 t ye falls from 0y to roughly 0 3 y when 1 t k =−
=

is a crude approximation of the third-life of a decay curve. In other words, if a substance decays and has a decay constant 0.02 k =− , and time is measured in years, then the third-life of the substance is roughly 1 50 0.02 = years. That is, every 50 years the substance decays by 2 3 . Note that the curve in the figure falls to 1 3 of its value in approximately 1 t = unit of time.

Radioactive Decay

4. dQ kQ dt = has the general solution

Initial condition ( ) 0100 Q = gives ( ) 100 kt Qte = where Q is measured in grams. We also have the initial condition ( ) 5075 Q = , from which we find

Determining Decay from Half-Life

5. dQ kQ dt = has the general solution ( ) kt Qtce = . With half-life 5 h t = hours, the decay constant has the value 1 ln20.14 5 k =−≈− . Hence,

Calling tt the time it takes to decay to 1 10 the original amount, we have

which we can solve for tt getting

124
CHAPTER 2 Linearity and Nonlinearity
( ) kt Qtce = .
13ln0.0058 504 k =≈− . The
( ) 0.0058 100 t Qte ≈
ln2 120 0.0058 h t =≈ years.
solution is
where t is measured in years. The half-life is
( ) 0.14 0 t QtQe =
0.14 00 1 10 tt QQe = ,
5ln10 16.6 ln2 tt =≈ hours.

Thorium-234

6. (a) The general decay curve is ( ) kt Qtce = . With the initial condition ( ) 01 Q = , we have ( ) kt Qte = . We also are given ( ) 10.8 Q = so 0.8 k e = , or ( ) ln0.80.22 k =≈− . Hence, we have

where Q is measured in grams and t is measured in weeks.

Dating Sneferu’s Tomb

7. The half-life for Carbon-14 is 5600 h t = years, so

Let tc be the time the wood has been aging, and 0y be the original amount of carbon. Fifty-five percent of the original amount is 0 0.55 y . The length of time the wood has aged satisfies the equation

Newspaper Announcement

8. For Carbon-14,

. If 0y is the initial amount, then the final amount of Carbon-14 present after 5000 years will be

= .

In other words, 54% of the original carbon was still present.

Radium Decay

9. 6400 years is 4 half-lives, so that 4 1 6.25% 2 ≈ will be present.

SECTION 2.3 Growth and Decay Phenomena 125
( ) 0.22 t Qte =
ln2ln2
0.22 h t
=−=≈
(c) () (
0.2210 100.107
(b)
3.1
k
weeks
)
Qe
grams
1ln2 ln20.000124 5600 h k t =−=−≈−
0.000124 00 0.55 te yey =
5600ln0.55 4830 ln2 tc =−≈ years.
. Solving for tc gives
ln2ln2 0.000124 5600 h
==≈−
50000.000124 00 0.54 yey
k t
( )

10.

General Half-Life Equation

Bombarding Plutonium

126
CHAPTER 2 Linearity and Nonlinearity
We are given the two equations 1 2 10 20 kt kt QQe QQe = = If we divide, we get () 12 1 2 ktt Q e Q = or () 1 12 2 ln Q ktt Q −= or 1 2 12 ln Q Q k tt =
in 1 ln2 h t k =− yields the general half-life of ( ) ( ) 11 22 1221ln2ln2 lnln h QQ QQ tttt t =−= . Nuclear Waste
We have ln2ln2 0.00268 258 h k t =−=−≈− and solve for t in 0.00268 00 0.05 t yey = . Thus 258ln20 1,115 ln2 t =≈ years.
Substituting
11.
We are given ln2 4.6209812 0.15 k =−≈− . The differential equation for the amount present is 0.00002 dA kA dt =+ , ( ) 00 A = . Solving this initial-value problem we get the particular solution () 0.00002 kt Atce k =−
12.

Blood Alcohol Levels

13. (a) First, because the initial blood-alcohol level is 0.2%, we have

= . After one hour, the level reduces by 10%, therefore, we have

From the decay equation we have

= , hence we have the equation

from which we find

k = ≈− . Thus our decay equation is

(b) The person can legally drive as soon as

and solving for t, yields

14. The measured blood-alcohol level was 0.06%, which had been dropping at a rate of 0.015 percentage points per hour for nine hours. This being the case, the captain’s initial blood-alcohol level was

.

The captain definitely could be liable.

Sodium Pentathol Elimination

15. The half-life is 10 hours. The decay constant is

SECTION 2.3 Growth and Decay Phenomena 127 where 0.00002 0.000004 c k =≈− . Plugging in these values gives the total amount ( ) ( ) 4.6 0.0000041 t Ate ≈−
in micrograms.
measured
()00.2
( ) ( ) ( ) 10.900.90.2PP== .
P
( )
k Pe
( ) 0.20.90.2 k e =
10.2
ln0.90.105
() ( ) ln0.9 0.105 0.20.2 t t Ptee =≈
( ) 0.1 Pt < . Setting ( ) 0.105 0.20.1 t Pte==
ln2 6.6 0.105 t =−≈ hours.
Exxon Valdez Problem
( ) 0.0690.0150.195%
+=
ln2 0.069 10 k =−≈− . Ed needs ( ) ( ) 50 mgkg100 kg5000 mg =

of pentathal to be anesthetized. This is the minimal amount that can be presented in his bloodstream after three hours. Hence,

Solving for 0A yields 0 6,155.7 A = milligrams or an initial dose of 6.16 grams.

Moonlight at High Noon

16. Let the initial brightness be 0 I . At a depth of 25 d = feet, we have that 15% of the light is lost, and so we have ( ) 0 250.85 II = . Assuming exponential decay, ( ) 0 kd IdIe = , we have the equation

from which we can find

To find d, we use the equation

from which we determine the depth to be

17. Here

k = . We can find the tripling time by solving for t in the equation

Extrapolating the Past

18. If 0P is the initial number of bacteria present (in millions), then we are given

Dividing one equation by the other we obtain

, from which we find

and

128
CHAPTER 2 Linearity and Nonlinearity
=≈=
() ( ) 0.0693 00 30.8135000 AAeA
( ) 25 250.8500 k IIeI ==
ln0.85 0.0065 25 k =≈− .
0.0065 00 1 300,000 d IeI = ,
() 1
0.0065 d
Tripling Time
ln300,0001940
=≈ feet.
ln2 10
( ) ln210 00 3 t yey ⎡⎤ ⎣⎦ = , giving ln2 ln3 10 t ⎛⎞ = ⎜⎟ ⎝⎠ or 10ln3 15.85 ln2 t =≈ hours.
6 0 5 k Pe
9 0 8 k Pe = .
3 8 5 k e =
8 5 ln 3 k = .
=

Substituting this value into the first equation gives (

0 5 Pe = , in which we can solve for

Unrestricted Yeast Growth

19. From Problem 2, we are given

with the initial population of 0 5 P = million. The population at time t will be

5

million, so at 4 t = hours, the population will be

Unrestricted Bacterial Growth

20. From Problem 2, we are given ln2 12 k = so the population equation is

In order to have five times the starting value, we require

5 t PeP = , from which we can find

Growth of Tuberculosis Bacteria

21. We are given the initial number of cells present is 0 100 P = , and that ( ) 1150 P = (1.5 times larger), then 100 ( )1 150 k e = , which yields

= . Therefore, the population ( ) Pt at any time t is

Cat and Mouse Problem

22. (a) For the first 10 years, the mouse population simply had exponential growth

Because the mouse population doubled to 50,000 in 10 years, the initial population must have been 25,000, hence ln2 10 k = . For the first 10 years, the mouse population (in thousands) was

= .

SECTION 2.3 Growth and Decay Phenomena 129
) 2ln85
( ) 2ln85 0 51.95Pe=≈
million bacteria.
ln2 ln2 1 k ==
) ln2
4ln2 551680 e = ⋅=
(
t e
million.
() ( ) ln212 0 t PtPe =
( ) ln212 00
ln5 1227.9 ln2 t =≈ hours.
3 ln 2 k
() ( ) ln32 0.405 100100 t t Ptee =≈ cells.
( ) 0 kt M tMe =
() ( ) ln210 25 t Mte

CHAPTER 2 Linearity and Nonlinearity

Over the next 10 years, the differential equation was 6 dM kM dt = , where ( ) 050 M = ; t now measures the number of years after the arrival of the cats. Solving this differential equation yields

Using the initial condition ( ) 050 M = , we find 6 50 c k = . The number of mice (in thousands) t years after the arrival of the cats is

where the constant k is given by ln2 0.069 10 k =≈ . We obtain

(b) () ( ) 0.06910 10873713.2Me=−≈ thousand mice.

(c) From part (a), we obtain the value of k for the population growth without harvest, i.e., ln2 0.0693 10 k =≈ . We obtain the new rate of change M ′ of the mouse population:

After 10 years the mouse population will be 18393 (give or take a mouse or two).

Banker’s View of e

23. The amount of money in a bank account that collects compound interest with continuous compounding is given by

where 0A is the initial amount and r is an annual interest rate. If 0 $1 A = is initially deposited, and if the annual interest rate is 0.10 r = , then after 10 years the account value will be

( ) 0.1010 10$1$2.72Ae=⋅≈

130
()
+
6 kt Mtce k =
.
()
kt Mte kk ⎛⎞ = ⎜⎟−+ ⎝⎠
66 50
(
) 0.069 3787 t Mte = −+ .
0.0307 ln2 0.100.0307 10 25000 t M MMM Me ′ =−≈− =
( )
AtAe =
0 rt
()

Rule of 70

24. The doubling time is given in Problem 2 by

25.

where 100r is an annual interest rate (expressed as a percentage). The rule of 70 makes sense. Power

Credit Card Debt

26. If Meena borrows 0 $5000 A = at an annual interest rate of 0.1995 r = (i.e., 19.95%), compounded continuously, then the total amount she owes (initial principle plus interest) after t years is

Compound

SECTION 2.3 Growth and Decay Phenomena 131
ln20.7070 100 d t rrr =≈=
Compounding
of Continuous
The
( ) 0 rt A tAe = , If 0 $0.50 A = , 0.06 r = and 160 t = , then the value of the account after 160 years will be () ( ) ( ) 0.06160 1600.5$7,382.39Ae=≈ .
future value of the account will be
( ) 0.1995 0 $5,000 AtAeertt == After 4 t = years, she owes () ( ) 0.19954 4$5,000$11,105.47Ae=≈ . Hence, she pays $11,105.47$5000$6,105.74 = interest for borrowing this money.
The growth rate is () 0 rt AtAe = . In this case 0 3 A = , 0.08 r = , and 320 t = . Thus, the total bottles of whiskey will be () ( ) ( ) 0.08320 3203393,600,000,000Ae=≈ That’s 393.6 billion bottles of whiskey! It Ain’t Like It Use to Be
The growth rate is () 0 rt AtAe = ,
0 1 A = , 50 t = , and ( ) 5018 A = (using thousands of dol-
50 18 r e = ,
ln18 0.0578 50 r =≈ ,
5.78%.
Interest Thwarts Hollywood Stunt 27.
28.
where
lars). Hence, we have
from which we can find
or

CHAPTER 2 Linearity and Nonlinearity

How to Become a Millionaire

29. (a) From Equation (11) we see that the equation for the amount of money is

(c) () () 40 2500 40$1,000,0001 r Ae r ==− . To solve this equation for r we require a computer. Using Maple, we find the interest rates 0.090374 r = ( ) 9.04% ≈ . You can confirm this result using direct substitution.

Living Off Your Money

Notice that when 0drA = this equation is undefined, as we have division by 0; if 0drA < , this equation is undefined because we have a negative logarithm. For the physical translation of these facts, you must return to the equation for ( ) At . If 0drA = , you are only withdrawing the interest, and the amount of money in the bank remains constant. If 0drA < , then you aren’t even withdrawing the interest, and the amount in the bank increases and ( ) At never equals zero.

How Sweet It Is

31. From equation (11), we have

the time that the money will last.

132
() () 0 1 rtrt d AtAee r
+− .
() () 0.08 1000 1 0.08 t Ate =
() ( ) 0.0840 40$1,000,0001 0.08 d Ae==− . Solving for d
we
=
In this case, 0 0 A = , 0.08 r = , and $1,000 d = . The solution becomes
(b) ()
,
get that the required annual deposit $3,399.55 d =
() 0 1
d
r =−−
0
0 1 ln d t rdrA ⎛⎞ = ⎜⎟ ⎝⎠
30. ()
rtrt
AtAee
. Setting ( )
At = and solving for t gives
() ()0.080.08 100,000 $1,000,0001 0.08 Ateett =−− . Setting ( ) 0 At = , and
ln5 20.1 0.08 t =≈ years,
solving for t, we have

The Real Value of the Lottery

32. Following the hint, we let

Solving this equation with initial condition

33. (a) After one year compounded continuously the value of the account will be

With 0.08 r = (8%) interest rate, we have the value

This is equivalent to a single annual compounding at a rate 8.329 reff = %.

(b) If we set the annual yield from a single compounding with interest effr , ( ) 0eff 1 Sr + equal to the annual yield from continuous compounding with interest r, 0 r Se , we have

(i.e., 8.328%) effective annual interest rate, which is extremely close to that achieved by continuous compounding as shown in part (a). Good

34. Student Project. Your Financial Future

35. We can write the savings equation (10) as '0.085000AA = + , (0)0A =

The exact solution by (11) is

SECTION 2.3 Growth and Decay Phenomena 133
0.1050,000AA
=
0 0 AA
( ) ( ) 0.10 0 500,000500,000 t AtAe=−+ . Setting ( ) 200 A =
for 0A we get ( ) 2 0 2 500,0001 $432,332 e A e =≈
( )
= yields
and solving
Continuous Compounding
( ) 0 1 r SSe =
( ) 0.08 1$1.08328700 SSeS =≈
( ) 0eff0 1 r SrSe += Solving for effr yields eff 1 r re = . (c) 365 daily 0.08 110.0832775 365 r ⎛⎞ =+−= ⎜⎟ ⎝⎠
Test
for
Equation
Computer or Calculator
0.08 5000 (1) 0.08 t Ae = .

CHAPTER 2 Linearity and Nonlinearity

We list the amounts, rounded to the nearest dollar, for each of the first 20 years.

After 20 years at 8%, contributions deposited have totalled 20$5,000$100,000 × = while $147,064 has accumulated in interest, for a total account value of $247,064.

Experiment will show that the interest is the more important parameter over 20 years. This answer can be seen in the solution of the annuity equation

The interest rate occurs in the exponent and the annual deposit simply occurs as a multiplier.

Mortgaging a House

(a)

Since the bank earns 1% monthly interest on the outstanding principle of the loan, and Kelly’s group make monthly payments of $2500 to the bank, the amount of money A(t) still owed the bank at time t, where t is measured in months starting from when the loan was made, is given by the savings equation (10) with a = 2500.

Thus, we have 0.012500, (0)$200,000. dA AA dt =−=

134
Year Amount Year Amount 1 5,205 11 88,181 2 10,844 12 100,731 3 16,953 13 114,326 4 23,570 14 129,053 5 30,739 15 145,007 6 38,505 16 162,290 7 46,917 17 181,012 8 56,030 18 201,293 9 65,902 19 223,264 10 76,596 20 247,065
() 0.08 5000 1 0.08 t Ae = .
36.

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