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THE UNIVERSITY OF MELBOURNE
SCHOOL OF MATHEMATICS AND STATISTICS
MAST10006 Calculus 2
Lecture Notes
© School of Mathematics and Statistics, University of Melbourne, 2022.
STUDENT NAME:
These notes have been written by Christine Mangelsdorf, Anthony Morphett, TriThang Tran and Binzhou Xia. Reproduction of
any part of this work other than that authorised by Australian Copyright Law without permission of the copyright owners is
unlawful.
EMAIL:
This compilation has been made in accordance with the provisions of Part VB of the copyright act for the teaching purposes of the University.
These notes are for the use of students of the University of Melbourne enrolled in the subject MAST10006 Calculus 2.
Edition 22, July 2022.
Table of Contents
Section 0 - Notation used in MAST10006 Calculus 2
Section 0 - Notation used in MAST10006 Calculus 2
2
Section 1 - Limits, Continuity, Sequences and Series
7
Section 2 - Hyperbolic Functions
Standard Abbreviations
1. such that or given that: |
2. for all: ∀
88
Section 3 - Complex Numbers
117
3. there exists: ∃
Section 4 - Integral Calculus
142
4. equivalent to: ≡
Section 5 - First Order Ordinary Differential Equations
181
Section 6 - Second Order Ordinary Differential Equations
249
Section 7 - Functions of Two Variables
311
5. that is: i.e
6. approximate: ≈
7. much smaller than: ≪
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Standard Notation for Sets of Numbers
Standard Notation for Intervals
1. element of: ∈
so a ∈ X means “a is an element of the set X ”
1. natural numbers: N = {1, 2, 3, . . . }
2. integers: Z = {0, ±1, ±2, . . . }
2. open interval: (a, b)
so x ∈ (0, 1) means “0 < x < 1”
3. rational numbers: Q = { mn | m, n ∈ Z, n , 0}
3. closed interval: [a, b]
so x ∈ [0, 1] means “0 ≤ x ≤ 1”
4. real numbers: R (rational numbers plus irrational numbers)
5. complex numbers: C = {x + iy | x, y ∈ R, i2 = −1}
4. partial open and closed interval: (a, b] or [a, b)
so x ∈ [0, 1) means “0 ≤ x < 1”
6. R2 = {(x, y) | x, y ∈ R} (xy plane)
5. not including: \
so x ∈ R \ {0} means “x is any real number excluding 0”.
Alternatively, we could write (−∞, 0) ∪ (0, ∞) where ∪
means the ”union of the two intervals”.
7. R3 = {(x, y, z) | x, y, z ∈ R} (3 dimensional space)
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More Standard Notation
Greek Alphabet
1. natural logarithm (base e): log x
base 10 logarithm: log10 x
α
β
γ
δ
ϵ or ε
ζ
η
θ
ι
κ
λ
µ
Alternative notations for natural logarithms used in
textbooks: loge x, ln x
2. inverse trigonometric functions: arcsin x, arctan x etc
Alternative notations used in textbooks: sin−1 x, tan−1 x etc
3. implies: ⇒
so p ⇒ q means “p implies q”
4. if and only if (iff): ⇔ (means both ⇐ and ⇒)
so p ⇔ q means “p implies q” AND “q implies p”
alpha
beta
gamma
delta
epsilon
zeta
eta
theta
iota
kappa
lambda
mu
ν
ξ
o
π
ρ
σ
τ
υ
ϕ
χ
ψ
ω
nu
xi
omicron
pi
rho
sigma
tau
upsilon
phi
chi
psi
omega
5. approaches: →
so f (x) → 1 as x → 0 means “f (x) approaches 1 as x
approaches 0”
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Section 1: Limits, Continuity, Sequences, Series
Definition of limit of a function
Let f be a real-valued function.
Why do we study limits and continuity in calculus?
The limit of f (x) as x approaches a is L, written
lim f (x) = L
x→a
if f (x) gets arbitrarily close to L whenever x is close enough to a
but x , a.
Note:
If it exists, the limit L must be a unique finite real number.
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(
Example 1.1: If f (x) =
2x x , 1
, evaluate lim f (x).
4 x=1
x→1
Example 1.2: If f (x) =
1
, evaluate lim f (x).
x→0
x2
f HxL
f HxL
4
3
2
1
-3
Solution:
-2
-1
1
2
3
x
x
-1
Solution:
Note:
The limit of f as x approaches a does not depend on f (a). The
limit can exist even if f is undefined at x = a.
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(
Example 1.3: If f (x) =
We can describe this behaviour in terms of one-sided limits.
We write
1 x<0
, evaluate lim f (x).
2 x≥0
x→0
f HxL
2
1
Theorem:
x
lim f (x) = L if and only if lim− f (x) = L and lim+ f (x) = L.
Solution:
x→a
x→a
x→a
Thus the limit exists if and only if the left and right hand limits
exist and are equal.
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Limit Laws
x3 + 2x2 − 1
Example 1.4: Use the limit laws to evaluate lim
.
x→2
5 − 3x
Let f and g be real-valued functions and let c ∈ R be a constant.
If lim f (x) and lim g(x) exist, then
x→a
x→a
Solution:
1. lim [f (x) + g(x)] = lim f (x) + lim g(x).
x→a
x→a
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x→a
2. lim [cf (x)] = c lim f (x).
x→a
x→a
3. lim [f (x)g(x)] = lim f (x) · lim g(x).
x→a
x→a
# lim f (x)
f (x)
x→a
=
4. lim
x→a g(x)
lim g(x)
x→a
"
x→a
provided lim g(x) , 0.
x→a
5. lim c = c.
x→a
6. lim x = a.
x→a
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Limits as x Approaches Infinity
Example 1.5: Evaluate lim e−x .
x→∞
The limit of f (x) as x approaches positive infinity is L,
y = e-x
lim f (x) = L
x→∞
H0,1L
if f (x) gets arbitrarily close to L whenever x is sufficiently large
and positive.
The limit of f (x) as x approaches negative infinity is M,
lim f (x) = M
x
x→−∞
Solution:
if f (x) gets arbitrarily close to M whenever x is sufficiently large
and negative.
Note:
1. L and M must be finite.
2. Limit laws (1)-(5) apply to limits as x → ±∞.
3. lim f (x) = lim f (−x).
x→−∞
x→∞
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Some Standard Limits
Terminology
The following are all equivalent ways of expressing lim f (x) = L:
x→a
▶ The limit of f (x) as x approaches a is L
▶ f (x) converges to L as x approaches a
We can use the following standard limits without further proof:
▶ f (x) → L as x → a
1
(1) lim p = 0 (p > 0)
x→∞ x
These all mean the same thing.
If the limit lim f (x) exists, we say that
(2) lim rx = 0
x→∞
x→a
(0 ≤ r < 1)
f (x) converges as x approaches a.
If the limit lim f (x) does not exist, we say that
x→a
f (x) diverges as x approaches a.
We will see more standard limits later.
Similarly for limits as x → ±∞.
Note:
Diverges simply means does not converge.
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More about divergence
Example 1.6: Explain why the following limits diverge.
1. lim sin x
How do we show that a limit lim f (x) diverges?
x→a
x→∞
2. lim
x→0
1
x2
Solution:
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f (x)
∞
has indeterminate form
as x → a if
g(x)
∞
f (x) → ∞ and g(x) → ∞.
Notation and ∞
We say a function
∞ is not a number, and should not appear as a number in your
writing.
In other textbooks, you will often see the notation lim
x→0
mean that
1
x2
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3x2 − 2x + 3
.
x→∞ x2 + 4x + 4
Example 1.7: Evaluate lim
1
= ∞ to
x2
Solution:
diverges to infinity.
You should not use this notation in Calculus 2 and will lose
notation marks for this!
Why?
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Sandwich Theorem (version for x → a)
We say a function f (x) − g(x) has indeterminate form ∞ − ∞ as
x → a if f (x) → ∞ and g(x) → ∞.
Example 1.8: Evaluate lim
√
x→∞
If g(x) ≤ f (x) ≤ h(x) when x is near a but x , a, and
lim g(x) = lim h(x) = L
x2 + 1 − x .
x→a
then
x→a
lim f (x) = L.
Solution:
x→a
y
hHxL
f HxL
L
a
gHxL
x
Note: “x is near a but x , a” means that x ∈ (b, a) ∪ (a, c) for
some b < a < c.
We will finish this example later.
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Sandwich Theorem (version for x → ∞)
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1
Example 1.9: Evaluate lim x2 sin
.
x→0
x
A version of the Sandwich Theorem also works for limits as
x → ∞.
Solution:
If g(x) ≤ f (x) ≤ h(x) when x is sufficiently large, and
lim g(x) = lim h(x) = L
then
x→∞
x→∞
lim f (x) = L.
x→∞
Similarly, the theorem holds for x → −∞.
Note: “x is sufficiently large” means x ∈ (c, ∞) for some real
number c.
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1
Example 1.10: Evaluate lim x sin
.
x→0
x
Example 1.8 (continued)
lim
Solution:
x→∞
√
x2 + 1 − x =
lim √
x→∞
1
x2 + 1 + x
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Continuity
f HxL
Example 1.11: Let
(
2x x , 1
f (x) =
4 x = 1.
4
3
2
Is f continuous at x = 1?
Definition of continuity
1
-3
Let f be a real-valued function.
-2
-1
1
2
3
x
-1
The function f is continuous at x = a if
Solution:
lim f (x) = f (a).
x→a
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 2
x −4




 x−2 x,2
Example 1.12: Let f (x) = 




4 x = 2.
Theorem:
The following function types are continuous at every point in
their domains:
▶ polynomials
Is f continuous at x = 2?
▶ trigonometric functions: sin x, cos x, tan x, sec x, cosec x,
cot x, arcsin x, arccos x, arctan x
▶ exponential functions: ax for a > 0
Solution:
▶ logarithm functions: loga x for a > 0
√
▶ nth root functions: n x for n ∈ {2, 3, 4, ...}
▶ hyperbolic functions: sinh x, cosh x, tanh x, sech x, cosech x,
coth x, arcsinh x, arccosh x, arctanh x
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Example 1.13: Evaluate lim sin (e−x ) .
x→∞
Let f and g be real-valued functions and b ∈ R.
Solution:
Theorem:
If lim g(x) = b and f is continuous at b then
x→a
lim f g(x) = f lim g(x) = f (b).
x→a
x→a
Note:
This theorem also holds for limits as x → ∞.
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Let f and g be real-valued functions and c ∈ R be a constant.
Theorem:
If the functions f and g are continuous at x = a, then the
following functions are continuous at x = a:
Recall that ( g ◦ f )(x) = g( f (x)).
1. f + g,
Theorem:
2. cf ,
If f is continuous at x = a and g is continuous at x = f (a), then
g ◦ f is continuous at x = a.
3. fg,
4.
f
if g(a) , 0.
g
Note:
The theorem follows from limit laws.
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Example 1.14: Let f (x) =
sin x2 + 1
log x
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.
For which values of x is f continuous?
Solution:
Note:
This set can also be written as
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 3

x − cx + 8, x ≤ 1



Example 1.15: f (x) = 


 x2 + 2cx + 2, x > 1.
For which values of c is f continuous at all x ∈ R?
Justify your answer.
Solution:
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Where does this definition come from?
Differentiability
Before seeing what is filled in from the lectures, try to come up
with a picture that explains where the definition comes from.
Definition of derivative
Let f be a real-valued function whose domain contains an open
interval around x = a. The derivative of f at x = a is defined by
f ′ (a) = lim
h→0
f (a + h) − f (a)
.
h
The function f is differentiable at x = a if this limit exists.
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Geometrically, f is differentiable at x = a if the graph y = f (x)
has a tangent line at x = a.
f HxL
Differentiability and Continuity
f HxL
Theorem:
If f is differentiable at x = a, then f is continuous at x = a.
x
a
Differentiable at x=a
x
What about the converse?
Not differentiable
at x=0
f HxL
If f is differentiable at x = a, then
f HxL
y = f (a) + f ′ (a)(x − a)
is the tangent line to the curve y = f (x) at the point x = a, and
f (x) ≃ f (a) + f ′ (a)(x − a)
x
a
Differentiable at x=a
when x is close to a.
x
Not differentiable
at x=0
That is, the tangent line is a linear approximation for the
function close to the point x = a.
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L’Hôpital’s Rule
Let f and g be differentiable functions near x = a, and
at all points x near a with x , a. If
g′ (x)
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Example 1.16: Evaluate lim
,0
x→0
sin x
.
x
Solution:
f (x)
lim
x→a g(x)
has the indeterminate form
lim
x→a
0
∞
or
then
0
∞
f (x)
f ′ (x)
= lim ′
x→a g (x)
g(x)
if the limit involving the derivatives exists.
Note:
L’Hôpital’s Rule also holds for limits as x → ∞, and for
one-sided limits x → a+ and x → a− for a ∈ R.
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3x2 − 2x + 3
Example 1.17: Evaluate lim 2
.
x→∞ x + 4x + 4
1
Example 1.18: Evaluate lim x− 3 log x .
Solution:
Solution:
x→∞
(0 · ∞)
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Aside - What is a limit really?*
Aside - What is a limit really?*
Recall our definition of limit:
Example 1.19: Using the definition, prove that
lim f (x) = L if f (x) gets arbitrarily close to L whenever x is close
lim 2x = 2
x→a
enough to a but x , a.
x→1
Solution:
What do ‘arbitrarily close’ and ‘close enough’ mean?
For an arbitrary positive real number ε,
More formally,
1
|f (x) − 2| = 2|x − 1| < ε if and only if |x − 1| < ε = δ.
2
This shows that |f (x) − 2| can be arbitrarily small whenever
|x − 1| is small enough but not equal to 0.
for any arbitrary positive real number ε, there is a positive real
number δ such that
|f (x) − L| < ϵ whenever 0 < |x − a| < δ.
In other words, f (x) can be arbitrarily close to 2 whenever x is
close enough to 1 but x , 1.
This formal definition of limit is covered in MAST20026 Real
Analysis, but as a taster we do two examples.
Therefore,
lim f (x) = 2.
x→1
* Slides 49-51 are not examinable in MAST10006.
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Aside - What is a limit really?*
Sequences
Definition of sequence
Example 1.20: Sketch a proof of the limit law
A sequence is a function f : N → R.
It can be thought of as an ordered list of real numbers
lim [f (x) + g(x)] = lim f (x) + lim g(x)
x→a
x→a
x→a
a1 , a2 , a3 , a4 , . . . , an . . .
Solution:
Suppose lim f (x) = L and lim g(x) = M.
x→a
Thus, f (n) = an .
The sequence is denoted by (an ), where an is the nth term.
x→a
For an arbitrary positive real number ε, to make
|f (x) + g(x) − (L + M)| < ε
ε
ε
we only need to make |f (x) − L| < and |g(x) − M| < .
2
2
These will be satisfied whenever x is close enough to a but
x , a since lim f (x) = L and lim g(x) = M.
x→a
Sometimes the notation {an } is also used.
Example
1 1 1 1
1, , , , , . . .
2 3 4 5
x→a
Hence f (x) + g(x) can be arbitrarily close to L + M whenever x is
close enough to a but x , a, which means that
x→a
1
n
Example
1, −1, 1, −1, 1, −1, . . .
lim [f (x) + g(x)] = L + M = lim f (x) + lim g(x).
x→a
an =
x→a
an = (−1)n−1
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Limits of Sequences
The graph of a sequence (an ) can be plotted on a set of axes
with n on the x-axis and an on the y-axis.
Example: an =
Definition of limit of sequence
Example: an = (−1)n−1
1
n
A sequence (an ) has the limit L if an can be made arbitrarily
close to L by making n sufficiently large. We write
an
an
1
1
lim an = L
n→∞
1
−1
2
3
4
5
n
1
2
3
4
5
or an → L as n → ∞.
n
If the limit exists we say that the sequence converges.
Otherwise, we say that the sequence diverges.
−1
Note:
If it exists, L must be a unique finite real number.
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Theorem (Limit Laws):
Example 1.21: Determine whether
the following sequences
1
converge or diverge: (a)
(b) (−1)n−1 (c) (n)
n
Let (an ) and (bn ) be sequences of real numbers and c ∈ R a
constant.
If lim an and lim bn exist, then
n→∞
Solution:
n→∞
1. lim [an + bn ] = lim an + lim bn .
n→∞
n→∞
n→∞
2. lim [can ] = c lim an .
n→∞
n→∞
3. lim [an bn ] = lim an · lim bn .
n→∞
n→∞
4. lim
n→∞
n→∞
lim an
an
n→∞
=
bn
lim bn
provided lim bn , 0.
n→∞
n→∞
5. lim c = c.
n→∞
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The Factorial Function
Standard Limits
The factorial function n! (n = 0, 1, 2, ...) is defined by
n! = n(n − 1)! ,
or
(1) lim
n→∞
1
=0
np
1
0! = 1
(3) lim a n = 1
n→∞
n! = n × (n − 1) × (n − 2) × ... × 3 × 2 × 1
(p > 0)
(2) lim rn = 0
(a > 0)
(4) lim n n = 1
an
= 0 (a ∈ R)
n→∞ n!
a n
(7) lim 1 +
= ea (a ∈ R)
n→∞
n
(5) lim
Therefore
1! = 1
2! = 2 × 1 = 2
3! = 3 × 2 × 1 = 6
4! = 4 × 3 × 2 × 1 = 24
(9) lim arctan(cn) =
n→∞
Example
(2n + 2)! = (2n + 2) × (2n + 1) × (2n) × (2n − 1) × ... × 3 × 2 × 1
or
n→∞
(|r| < 1)
1
n→∞
(6) lim
log n
=0
np
(8) lim
np
=0
an
n→∞
n→∞
(p > 0)
(p ∈ R, a > 1)
π
(c > 0)
2
Note:
(2n + 2)! = (2n + 2) × (2n + 1) × (2n)!
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Standard limits (1), (3), (4), (6), (7), (8), (9) also hold for limits of
real-valued functions as x → ∞ by replacing n with x.
Standard limit (2) also holds for x → ∞ when 0 ≤ r < 1.
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"
Example 1.22: Evaluate lim
n→∞
n−2
n
n
#
4n2
+ n .
3
Example 1.23: Find the limit of the sequence
an =
Solution:
3n + 2
, n ≥ 1.
4n + 2n
Solution:
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Sandwich Theorem for sequences
Let (an ), (bn ) and (cn ) be sequences of real numbers.
Note:
If an ≤ cn ≤ bn for all n > N for some N, and
The order hierarchy can be used to help identify the largest
term in an expression:
lim an = lim bn = L
log n ≪ np ≪ an ≪ n!
then
n→∞
n→∞
lim cn = L.
n→∞
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1 + sin2
Example 1.24: Evaluate lim
√
n→∞
n
nπ
3
Continuity theorem for sequences
.
Solution:
Let f (x) be a real-valued function, (an ) a sequence of real
numbers and b ∈ R.
Theorem:
If lim an = b and f is continuous at x = b then
n→∞
lim f (an ) = f lim an = f (b).
n→∞
n→∞
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The only difference between lim an = L and lim f (x) = L is
h
i
Example 1.25: Evaluate lim log(3n2 + 2) − log n2 .
n→∞
n→∞
x→∞
that n is a natural number whereas x is a real number.
Solution:
Theorem:
Let f (x)) be a real-valued function and (an ) be a sequence of
real numbers such that an = f (n).
If
lim f (x) = L then
x→∞
lim an = L.
n→∞
This means that we can use the techniques for evaluating limits
of functions to evaluate limits of sequences.
Note:
lim an = L
n→∞
=⇒
̸
lim f (x) = L.
x→∞
eg. an = sin(2πn), f (x) = sin(2πx).
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Example 1.26: Prove Standard Limit 6:
lim
n→∞
log n
=0
np
(p > 0)
Solution:
Note:
We must change from a limit of a sequence (in terms of n) to a
limit of a real-valued function (in terms of x) before applying
L’Hôpital’s rule.
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n
1
Example 1.27: Find the sum S of an =
, n ≥ 1.
2
Solution:
Adding Infinitely Many Numbers
Starting with any sequence (an ), adding the an ’s together in
order gives a sequence (sn ):
s1 = a1 ,
s2 = a1 + a2 ,
s3 = a1 + a2 + a3 ,
..
..
..
..
.
.
.
.
The sequence of partial sums (sn ) may or may not converge. If
it does converge, we call
S = lim sn = lim (a1 + a2 + . . . + an )
n→∞
n→∞
the sum of the an ’s.
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Series
A series with terms an is denoted by the sum
∞
X
an .
n=1
If the associated sequence of partial sums (sn ) converges then
∞
X
we say that the series
an converges. Otherwise we say that
n=1
the series diverges.
Example
The constant sequence with an = 2 is the sequence 2, 2, 2, 2, . . .
∞
∞
X
X
an =
2 represents the sum 2 + 2 + 2 + · · ·
The series
n=1
n=1
The sequence of terms converges, but the series diverges to
infinity.
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Application: Decimals
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Properties of Series
The decimal representation of a number is actually a series.
Let
Example
The sequence
1
10n
If
= 0.1, 0.01, 0.001, . . ..
∞
X
1
The series
= 0.1 + 0.01 + 0.001 + . . . = 0.11111111 . . .
10n
an and
n=1
∞
X
n=1
n=1
an and
n=1
2.
If
For a number x ∈ (0, 1) with decimal digits d1 , d2 , d3 , d4 , . . .
∞
X
dn
x = 0.d1 d2 d3 d4 · · · =
10n
bn be series, and c ∈ R\{0} a constant.
bn converge then
∞
X
∞
X
n=1
n=1
(an + bn ) =
an +
∞
X
bn converges.
n=1
∞
∞
X
X
(can ) = c
an converges.
n=1
In General
∞
X
n=1
∞
X
1.
1
The sequence converges to 0 while the series converges to .
9
∞
X
∞
X
n=1
an diverges then
n=1
∞
X
(can ) diverges.
n=1
Note:
n=1
These follow from the properties of the limits of sequences.
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Geometric Series
Example 1.28: What does the series
A geometric series has the form
∞
X
arn =
n=0
∞
X
∞ n
X
1
n=0
arn−1 = a + ar + ar2 + ar3 + . . .
2
=1+
2 3
1
1
1
+
+ ...
+
2
2
2
converge to?
n=1
where a ∈ R\{0} and r ∈ R.
Solution:
The series converges if |r| < 1 and diverges if |r| ≥ 1.
If |r| < 1, we have
∞
X
arn =
n=0
a
.
1−r
Note:
This follows from the fact that
n
X
ark =
k=0
a(1 − rn+1 )
for r , 1.
1−r
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Harmonic p Series
Divergence Test
If lim an , 0 then
A harmonic p series has the form
n→∞
∞
X
1
.
np
∞
X
an diverges.
n=1
Note:
n=1
lim an , 0 includes the case that the limit lim an does not exist.
n→∞
The series converges if p > 1 and diverges if p ≤ 1.
n→∞
If lim an = 0 then
n→∞
∞
X
Example
1.
an may converge or diverge.
n=1
∞
∞
X
X
1
1
converges BUT
diverges.
2
n
n
n=1
n=1
2. The Divergence Test is not applicable, so we need to use
∞
X
another test to determine if
an converges or diverges.
n=1
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Example 1.29: Does the series
∞
X
n+1
n=1
n
converge?
Solution:
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Comparison Test
Let
∞
X
Example 1.30: Does
n=1
an be a series with non-negative terms (i.e. an ≥ 0).
1. If
bn is another series such that
n=1
0 ≤ bn ≤ an for all n, then
∞
X
∞
X
3+
5
n
2n2 + n + 2
converge or diverge?
Solution:
n=1
∞
X
∞
X
bn diverges and
n=1
an also diverges.
n=1
2. If
∞
X
cn is another series such that
n=1
cn ≥ an for all n, then
∞
X
∞
X
cn converges and
n=1
an also converges.
n=1
To apply the comparison test we compare a given series to a
harmonic p series or geometric series.
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Example 1.31: Does
∞
X
n2 + 4
n=1
n3 + 5
converge or diverge?
Solution:
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Ratio Test
Let
∞
X
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Example 1.32: Does
∞
X
10n
n=1
converge or diverge?
Solution:
an be a positive term series (i.e. an > 0 for all n). Let
n=1
n!
an+1
.
n→∞ an
L = lim
1. If L < 1,
∞
X
an converges.
n=1
2. If L > 1,
∞
X
an diverges.
n=1
3. If L = 1, the ratio test is inconclusive.
The ratio test is useful if an contains an exponential or factorial
function of n.
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Example 1.33: Does
∞
X
(2n)!
n=1
n! n!
converge or diverge?
Solution:
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Section 2: Hyperbolic Functions
y = cosh(x)
y
4
Even Functions
y
y = x2
4
A function f is an even function if
We define the hyperbolic cosine
function:
3
3
2
f (−x) = f (x)
2
1 x
e + e−x , x ∈ R
cosh x =
2
1
Example
1
x
f (x) = cos x and f (x) = x2
−2
−1
1
y
x
2
−3
Odd Functions
1
2
3
Properties
4
A function f is an odd function if
−1
−1
y = x3
8
−2
x
f (−x) = −f (x)
−2
−1
1
2
−4
Example
f (x) = sin x and f (x) = x3
−8
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y
y
We define the hyperbolic
tangent function:
y = sinh(x)
4
3
We define the hyperbolic sine
function:
sinh x =
1 x
e − e−x ,
2
x∈R
tanh x =
2
=
1
x
−3
−2
−1
1
2
3
=
−1
2
sinh x
cosh x
1 x
−x
2 (e − e )
1 x
−x
2 (e + e )
ex − e−x
ex + e−x
,
y = tanh(x)
1
x
−3
−2
−1
1
2
3
−1
x ∈ R.
−2
−2
Properties
Properties
−3
−4
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Why call them hyperbolic functions?
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So (x, y) = (cosh t, sinh t) denotes a point on the hyperbola
x2 − y2 = 1. Since x ≥ 1, the right hand branch of the hyperbola
can be parametrised by x = cosh t, y = sinh t, t ∈ R.
Let x = cosh t and y = sinh t then
y
x2-y2=1
t>0
4
t
x=cosh t
y=sinh t
2
4
2
-4
-2
-2
-4
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x
t=0
t<0
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Application: Catenary
Example 2.1: If cosh x =
13
12
and x < 0 find sinh x and tanh x.
Solution:
A flexible, heavy cable of uniform mass per length ρ and
tension T at its lowest point has shape
ρgx T
y=
cosh
ρg
T
where g is the acceleration due to gravity.
y
Support
Support
x
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Addition Formulae
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sinh(x + y)
=
sinh x cosh y + cosh x sinh y
cosh(x + y)
=
cosh x cosh y + sinh x sinh y
sinh(x − y)
=
sinh x cosh y − cosh x sinh y
cosh(x − y)
=
cosh x cosh y − sinh x sinh y
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Double Angle Formulae
Example 2.2: Prove the sinh(x + y) addition formula.
Solution:
sinh(2x)
=
2 sinh x cosh x
cosh(2x)
=
cosh2 x + sinh2 x
cosh(2x)
=
2cosh2 x − 1
cosh(2x)
=
2sinh2 x + 1
These can be proved using the addition formulae.
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Reciprocal Hyperbolic Functions
Reciprocal Hyperbolic Functions
We define the three reciprocal hyperbolic functions:
coth x =
sech x =
1
, x∈R
cosh x
cosech x =
1
, x ∈ R \ {0}
sinh x
cosh x
1
=
,
tanh x
sinh x
x ∈ R \ {0}
y
y
y
3
1.0
2
0.5
1
2
y = sech(x)
x
−3
−2
−1
1
−0.5
y = coth(x)
1
2
3
−3
−2
−1
1
2
y = cosech(x)
x
3
x
−3
−2
−1
1
2
3
−1
−1
−2
−2
−3
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Basic Identities
Derivatives of Hyperbolic Functions
cosh2 x − sinh2 x
=
1
coth2 x − 1
=
cosech2 x
1 − tanh2 x
=
sech2 x
d
(cosh x)
dx
=
sinh x,
x∈R
d
(sinh x)
dx
=
cosh x,
x∈R
d
(tanh x)
dx
=
sech2 x,
x∈R
d
(sech x)
dx
=
− sech x tanh x,
d
(cosech x)
dx
=
− cosech x coth x,
d
(coth x)
dx
=
− cosech2 x,
x∈R
x ∈ R \ {0}
x ∈ R \ {0}
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Example 2.3: Prove that
d (cosh x)
= sinh x.
dx
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Example 2.4: Let y =
Solution:
p
sinh(6x), x > 0. Find
dy
.
dx
Solution:
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Inverses of Hyperbolic Functions
2. Inverse hyperbolic cosine function: arccosh x
We define three inverse hyperbolic functions.
Restrict domain of cosh x to be [0, ∞) to give a 1-1 function.
Then
1. Inverse hyperbolic sine function: arcsinh x
Since sinh x is a 1-1 function
domain arcsinh x =
domain arccosh x =
range sinh x = R.
range arcsinh x =
range arccosh x =
domain sinh x = R.
arcsinh(sinh x) = x,
x ∈ R.
sinh(arcsinh x) = x,
x ∈ R.
x ≥ 1.
arccosh(cosh x) = x,
x ≥ 0.
y
4
3
y = arcsinh(x)
2
−2
y = arccosh(x)
2
1
−3
y = cosh(x)
5
3
−4
restricted domain cosh x = [0, ∞).
cosh(arccosh x) = x,
y = sinh(x)
y
range cosh x = [1, ∞).
−1
2
1
3
4
x
1
−1
2
1
−2
3
4
5
x
−3
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3. Inverse hyperbolic tangent function: arctanh x
The inverse hyperbolic functions can be expressed in terms of
natural logarithms.
Since tanh x is a 1-1 function
domain arctanh x =
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range tanh x = (−1, 1).
range arctanh x =
domain tanh x = R.
tanh(arctanh x) = x,
−1 < x < 1.
arctanh(tanh x) = x,
x ∈ R.
y
3
arcsinh x
=
√
log x + x2 + 1 ,
x∈R
arccosh x
=
√
log x + x2 − 1 ,
x≥1
arctanh x
=
1
1+x
log
,
2
1−x
−1 < x < 1
y = arctanh(x)
2
y = tanh(x)
1
−4
−3
−2
We can also define inverse reciprocal hyperbolic functions:
• arcsech x
(0 < x ≤ 1)
−1
• arccosech x
(x , 0)
−2
• arccoth x
(x < −1 or x > 1)
−1
1
2
3
4
x
−3
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Example 2.5: Proof of arcsinh x relation.
Solution:
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Derivatives
Example 2.6: Simplify cosh(arcsinh x) for x ∈ R.
Solution:
d
(arcsinh x)
dx
=
1
√
2
x +1
d
(arccosh x)
dx
=
√
d
(arctanh x)
dx
=
1
x2
1
1 − x2
−1
(x ∈ R)
(x > 1)
(−1 < x < 1)
Each formula is derived using implicit differentiation or by
differentiating the logarithm definition of each function.
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Example 2.7: Prove that
d
1
(arcsinh x) = √
.
dx
x2 + 1
Solution:
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Example 2.8: Find
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Section 3: Complex Numbers
d
(arctanh(2x) cosh(3x)).
dx
The Cartesian form of a complex number z ∈ C is
Solution:
z = x + iy where x, y ∈ R
and
• x = Re(z) is the real part of z,
• y = Im(z) is the imaginary part of z,
• i2 = −1.
ImHzL
z=x+iy
r
y
Θ
x
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ReHzL
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The Complex Exponential
The complex number can be written as
z = r(cos θ + i sin θ)
where
q
• r = |z| = x2 + y2
y
• tan θ =
x
Note:
The angle θ is not unique – only defined up to multiples of 2π.
We choose θ such that −π < θ ≤ π and call this angle the
principal argument of z.
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The Complex Exponential
Example 3.2: Write z = −1 + i in polar form.
We define the complex exponential using Euler’s formula
ImHzL
eiθ = cos θ + i sin θ
-1+i
for θ ∈ R.
2
1
Α
We can then write the polar form of a complex number as
1
z = reiθ
Θ
ReHzL
Solution:
Example 3.1: Simplify eiπ + 1.
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Properties of the Complex Exponential
Products and Division in Polar Form
1. ei0 = 1
Proof:
ei0 = cos 0 + i sin 0 = 1.
If z = r1 eiθ and w = r2 eiϕ then
2. eiθ eiϕ = ei(θ+ϕ)
Proof:
eiθ eiϕ = (cos θ + i sin θ) cos ϕ + i sin ϕ
= cos θ cos ϕ + i cos θ sin ϕ + i sin θ cos ϕ − sin θ sin ϕ
= cos θ cos ϕ − sin θ sin ϕ + i cos θ sin ϕ + sin θ cos ϕ
= cos θ + ϕ + i sin(θ + ϕ)
zw
=
r1 r2 ei(θ+ϕ)
z
w
=
r1 i(θ−ϕ)
e
r2
= ei(θ+ϕ) .
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Solution:
Example 3.3: Using the complex
exponential, simplify
√
√
√
3−i
( 3 − i)(1 + 3i) and
√ .
1 + 3i
ImHzL
1+ 3 i
2
3
Α2
1
Α1
2
ReHzL
3
1
3 -i
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De Moivre’s Theorem:
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√ 15
Example 3.4: Evaluate 1 + 3i .
Solution:
If z = reiθ and n is a positive integer then
n
zn = reiθ = rn einθ
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Exponential Form of sin θ and cos θ
Equation (1) − (2) gives
Now eiθ = cos θ + i sin θ
(1)
eiθ − e−iθ = 2i sin θ
⇒ e−iθ = cos(−θ) + i sin(−θ)
⇒ e−iθ = cos θ − i sin θ
⇒ sin θ =
1 iθ
e − e−iθ
2i
(2)
Note:
Equation (1) + (2) gives
These formulae give a connection between the hyperbolic and
trigonometric functions.
1 iθ
e + e−iθ = cos θ
cosh(iθ) =
2
eiθ + e−iθ = 2 cos θ
⇒ cos θ =
1 iθ
e + e−iθ
2
sinh(iθ) =
1 iθ
e − e−iθ = i sin θ
2
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Differentiation via the Complex Exponential
Example 3.5: Express sin5 θ in terms of the functions
sin(nθ) for integers n.
If z = x + yi where x, y ∈ R then we define
ez = ex+iy = ex eiy = ex (cos y + i sin y).
Solution:
Derivatives of functions from R to C are defined similarly as
those from R to R.
Differentiation to functions from R to C is also linear and follows
the product law.
Show that
d kt e = kekt when k = a + bi ∈ C.
dt
d h (a+bi)t i
d h at ibt i
e
=
e e
dt
dt
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=
i
d h at
e (cos(bt) + i sin(bt))
dt
= aeat [cos(bt) + i sin(bt)] + eat [−b sin(bt) + bi cos(bt)]
h
i
= aeat [cos(bt) + i sin(bt)] + eat bi2 sin(bt) + bi cos(bt)
= aeat [cos(bt) + i sin(bt)] + bieat [cos(bt) + i sin(bt)]
= (a + bi)eat [cos(bt) + i sin(bt)]
= (a + bi)eat eibt
= (a + bi)e(a+ib)t .
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d56 −t
Example 3.6: Find 56 e cos t .
dt
Solution:
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Note:
Example 3.6 also gives the answer to
d56 −t
e
sin
t
.
dt56
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Integration via the Complex Exponential
Z
Example 3.7: Evaluate
e3x sin(2x) dx.
Solution:
d kx Since
e = k ekx if k = a + bi (a, b ∈ R) , then
dx
Z
k ekx dx = ekx + C
Z
⇒
ekx dx =
1 kx
e +D
k
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Note:
Z
e3x cos(2x) dx.
Example 3.7 also gives the answer to
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Section 4: Integral Calculus
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Derivative Substitutions
Review of integration
To evaluate
Z
f [g(x)]g′ (x)dx
put u = g(x) ⇒
du
= g′ (x).
dx
Then
Z
Z
f [g(x)]g (x)dx =
′
f (u)
du
dx
dx
Z
=
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f (u) du
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Z
Example 4.1: Evaluate
Z
(6x + 10) sinh(x + 5x − 2)dx.
2
3
Example 4.2: Evaluate
Solution:
sech2 (3x)
dx.
10 + 2 tanh(3x)
Solution:
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Integration by Parts
Z
Example 4.3: Evaluate
xe5x dx.
The product rule for differentiation is
Solution:
d
du
dv
(uv) =
v+u
dx
dx
dx
Integrate
Z
d
(uv) dx =
dx
Z
⇒ uv =
Z
⇒
Z
!
dv
du
v+u
dx
dx
dx
du
v dx +
dx
Z
dv
u dx = uv −
dx
u
dv
dx
dx
Z
v
du
dx
dx
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Z
Example 4.4: Evaluate
Z
2
x log x dx
(x > 0).
log x dx
Example 4.5: Evaluate
Solution:
(x > 0).
Solution:
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Z
Example 4.6: Evaluate
e3x sin(2x) dx.
Solution:
Note:
This technique can also be used to integrate inverse
trigonometric functions and inverse hyperbolic functions.
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Trigonometric and Hyperbolic Substitutions
Integrand
√
a2 − x2 ,
√
a2 + x2 ,
√
We can use trigonometric and hyperbolic substitutions to
integrate expressions containing
√
a2 − x2 ,
√
√
a2 + x2 ,
√
x2 − a2 ,
1
a2 + x2
32
,
,
a2 + x2
− 32
,
52
a2 − x2
1
Substitution
a2 − x2
etc.
x = a sin θ
or
x = a cos θ
etc.
x = a sinh θ
etc.
x = a cosh θ
where a is a positive real number.
√
Method:
Z
Put x = g(θ).
Then
Z
f (x) dx =
f [g(θ)]g′ (θ) dθ
x2 − a2 ,
1
√
x2 − a2
1
,
a2 + x2
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x2 − a2
1
(a2
2
+ x2 )
etc.
x = a tan θ
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Z
Example 4.7: Evaluate
1
√
x2 − 25
dx using a substitution.
Solution:
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Z √
Example 4.8: Evaluate
9 − 4x2 dx if |x| ≤ 32 .
Solution:
Note:
Note the identity
√
x2 = |x|
(x ∈ R)
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Z 32
Example 4.9: Evaluate
x2 + 1 dx .
Solution:
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Powers of Hyperbolic Functions
Consider the integral:
Z
sinhm x coshn x dx
where m, n are integers (≥ 0).
• If m or n is odd, use a “derivative substitution” after rewriting
one of the odd power terms using identities if necessary.
• If m and n are even, use double angle formulae.
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Z
Example 4.10: Evaluate
cosh4 θ dθ.
Solution:
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Z
Finish Example 4.9:
Example 4.11: Evaluate
sinh5 x cosh6 x dx.
Solution:
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Z
Example 4.12: Evaluate I =
sinh5 x cosh7 x dx.
Solution:
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Partial Fractions
Let f (x) and g(x) be polynomials, then
f (x)
−→ degree n
g(x)
−→ degree d
can be written as the sum of partial fractions.
Case 1: n < d
1. Factorise g over the real numbers.
2. Write down partial fraction expansion.
3. Find unknown coefficients
A, A1 , A2 , . . . , Ar , B, B1 , B2 , . . . , Br .
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Denominator Factor
Partial Fraction Expansion
(x − a)
A
x−a
(x − a)r
A1
A2
Ar
+
+ ··· +
x − a (x − a)2
(x − a)r
(x2 + bx + c)
Ax + B
x2 + bx + c
(x2 + bx + c)r
A1 x+B1
x2 +bx+c
A2 x+B2
(x2 +bx+c)2
+
+ ··· +
Ar x+Br
(x2 +bx+c)r
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Z
Example 4.13: Evaluate
4
dx
+ 2)
x2 (x
(x , 0, −2).
Solution:
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Z
Example 4.14: Evaluate
(x2
4x
dx (x , 2).
+ 4)(x − 2)
Solution:
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Case 2: n ≥ d
Use long division, then apply case 1.
Example 4.15: Find
Z
5x4 + 13x3 + 6x2 + 4
dx
x3 + 2x2
Solution:
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(x , 0, −2).
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Section 5: First Order Differential Equations
A solution of an ODE is a function y(x) that satisfies the ODE
for all x in some interval.
Ordinary Differential Equations
Example 5.2: Verify by substitution that y(x) = x2 +
An ordinary differential equation (ODE) is an equation of the
form
!
dy d2 y
dn y
f x, y, , 2 , . . . , n = 0
dx dx
dx
solution of
dy y
+ = 3x for all x ∈ R \ {0}.
dx x
2
is a
x
Solution:
The order of an ODE is the order of the highest derivative
occurring in the ODE.
dy
d4 y
Example 5.1: What order is 3 4 =
dx
dx
!2
+ 2x2 y?
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First Order ODEs
Sketch of the family of solutions of
dy
The general form of a first order ODE is
= f (x, y).
dx
Example 5.3: Solve
dy
= x3
dx
y
dy
= x3 .
dx
6
Solution:
4
2
c=4
c=2
c=0
-4
A solution like this which contains an arbitrary constant c ∈ R is
called a general solution.
-2
2
-2
x
c=-2
-4
The general solution represents a family of solutions, where
each value of c corresponds to a different solution of the ODE.
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Initial value problem for a first order ODE
Solve
Separable ODEs
A separable first order ODE has the form:
dy
= f (x, y) subject to the condition y(x0 ) = y0 .
dx
dy
= M(x)N(y),
dx
dy
Example 5.4: Solve
= x3 given y(0) = 2.
dx
To solve, use separation of variables
dy
dx
Solution:
1 dy
N(y) dx
⇒
Z
Z
⇒
dy
y
=
dx 1 + x
= M(x)N(y)
= M(x)
1 dy
dx =
N(y) dx
⇒
Example 5.5: Solve
(M(x) , 0, N(y) , 0)
1
dy
N(y)
(N(y) , 0)
Z
M(x)dx
Z
=
M(x) dx
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(x , −1).
Solution:
Family of solutions
y
c=2
6
c=1
4
H-1,0L
-6
-4
2
-2
2
x
4
-2
-4
c=-1
-6
Example 5.6: Solve
dy −x
=
dx
y
c=-2
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(y , 0)
if y(0) = 3.
Solution:
Family of solutions
Linear First Order ODEs
y
5
Example 5.7: Solve x
4
Solution:
d = 16
3
2
1
dy
+ y = ex .
dx
d=9
d=4
d=1
x
-4
-3
-2
-1
0
1
2
3
4
5
-1 d = 1
-2
-3
d= 4
d=9
d = 16
-4
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A linear first order ODE has the form:
Aim:
dy
+ P(x)y = Q(x)
dx
Find an integrating factor I so the left side will be the derivative
of yI. Then
To solve:
dy
d
yI ≡ I + PIy
dx
dx
dy
dy
dI
⇒
I+y
= I + PIy
dx
dx
dx
Multiply ODE by I(x)
I(x)
dy
+ P(x)I(x)y = Q(x)I(x)
dx
If the left side can be written as the derivative of y(x)I(x), then
⇒ y
dI
= PIy
dx
⇒
dI
= PI
dx
To solve for all y
d y(x)I(x) = Q(x)I(x)
dx
which can be solved by integrating with respect to x.
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(separable)
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⇒
Z
⇒
1 dI
I dx
= P
1
dI =
I
Z
So one integrating factor is
Pdx
I(x) = e
Z
⇒ log |I| =
P dx + c
⇒ |I| = e
R
= e
R
⇒I =
R
Pdx
Note:
Pdx+c
Pdx
Since we only need one integrating factor I, we can neglect
the ‘+c’ and modulus signs when calculating I.
· ec
±ec ·e
|{z}
R
Pdx
constant
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Example 5.8: Find the general solution of
dy y
+ = sin x
dx x
(x , 0).
Solution:
Example 5.9: Solve
1 dy
− xy = x
2 dx
if y(0) = −3.
Solution:
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Note:
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Other First Order ODEs
Example 5.10: Solve the homogeneous type differential
equation
y
dy y
y
= + cos2
− π2 < x < π2
dx x
x
Sometimes it is possible to make a substitution to reduce a
general first order ODE to a separable or linear ODE.
y
by substituting u = .
x
• A homogeneous type ODE has the form
y
dy
=f
dx
x
Solution:
y
Substituting u = reduces the ODE to a separable ODE.
x
• Bernoulli’s equation has the form
Substituting u = y1−n
dy
+ P(x)y = Q(x)yn
dx
reduces the ODE to a linear ODE.
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Example 5.11: Solve the Bernoulli equation
dy
+ y = e3x y4
dx
(y , 0)
by substituting u = y−3 .
Solution:
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Population Models
Malthus (Doomsday) model
Note:
The Doomsday model predicts:
Rate of growth is proportional to the population p at time t.
dp
dt
dp
⇒
dt
• k > 0 : unbounded exponential growth
∝ p
= kp
• k < 0 : population dies out
(separable/linear)
where k is a constant of proportionality representing net births
per unit population per unit time.
• k = 0 : population stays constant
If the initial population is p(0) = p0 , then the solution is
Unbounded exponential growth is unrealistic in the long term.
p(t) = p0 ekt
You should check that you can derive this on your own!
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Equilibrium Solutions
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Example 5.12: Find all equilibrium solutions of the ODE
Definition
An equilibrium is a constant solution of an ODE.
Solution:
dx
= 3x − 2.
dt
Note:
For the ODE
dx
= f (x, t), this means
dt
▶ x(t) = C where C is a constant
▶
dx
=0
dt
Terminology
The plural form of equilibrium is equilibria.
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Phase plots
A phase plot is a plot of
Example 5.13: For the ODE
dx
= 3x − 2,
dt
dx
as a function of x.
dt
A phase plot will give
▶ the equilibria
(a) Draw a phase plot
(b) Sketch the family of solutions of the ODE, including
any equilibria.
▶ the behaviour of solutions close to the equilibria
(c) Describe the long-term behaviour of solutions with
initial conditions
1
i. x(0) =
2
Note:
Phase plots are only useful for ODEs of the form
dx
= f (x)
dt
ii. x(0) = 1
i.e., when the right-hand side has no explicit dependence on t.
ODEs of this form are called autonomous.
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(b).
Solution:
(a). The phase plot is
dx
dt
Family of solutions:
x
dx >0
dt
23
-2
1-
x
2/3-
dx <0
dt
equilibrium
x(t) = 2/3
1/2-
t
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(c) From the phase plot and family of solutions, we can see that
Stability of equilibria
An equilibrium is stable if solutions that start nearby move
closer to the equilibrium as t increases.
x
Note:
x0
Stable
We do not need to solve the ODE analytically to determine the
qualitative behaviour of the solutions.
t
When drawing a family of solutions, we include at least one
example of a solution with each possible qualitative behaviour
(unless stated otherwise in the question).
On a phase plot:
Two solutions have the same qualitative behaviour if their
shape and long-term behaviour are the same. Otherwise they
are qualitatively different.
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Stability of equilibria
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Stability of equilibria
An equilibrium is semistable if on one side of the equilibrium,
solutions that start nearby move closer as t increases, whereas
on the other side, solutions move further away as t increases.
An equilibrium is unstable if solutions that start nearby move
further away as t increases.
x
x
x
x0
Unstable
x0
Semistable
x0
t
t
Semistable
t
On a phase plot:
On a phase plot:
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Example 5.13 (continued):
(d) Determine the stability of the equilibrium.
Solution:
Doomsday model with harvesting.
Remove some of the population at a constant rate.
dp
= kp − h, h > 0.
dt
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Solution:
From Example 5.13 we know
Example 5.14: A pharmaceutical company grows
engineered yeast to produce a drug. The yeast is
continuously harvested to collect the drug.
The population p (in millions of yeast cells) at time t days
is described by
dp
= 3p − 2
dt
•
the equilibrium is
•
the phase plot is
dp
dt
dp
>0
dt
(p ≥ 0, t ≥ 0)
23
For what initial population sizes p(0) will the yeast
population eventually die out?
-2
p
dp
<0
dt
dies out!
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•
Logistic model.
the family of solutions is
p
Include “competition” term in Malthus’ model since
overcrowding, disease, lack of food and natural resources will
2/3-
Unstable
cause more deaths.
dp
k
= kp − p2 =
dt
a
t
dies out!
↗
The population will die out if
p
kp 1 −
a
↖
z }| {
z }| {
net birth rate
competition term
where a > 0 is the carrying capacity.
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• Phase plot
Example 5.15: Find the equilibrium solutions and their
stability for the ODE
dp
p
=p 1−
dt
4
dp
dt
(k = 1, a = 4)
1
Solution:
dp
>0
dt
• Equilibrium solutions
0
2
4
p
dp
<0
dt
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• Family of solutions:
p
Note:
The logistic model accurately describes
pH0L=4
• population in a limited space (e.g. bacteria culture).
• population of USA from 1790-1950.
pH0L=0
t
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Solution:
Logistic model with harvesting.
Remove some of the population at constant rate:
p
dp
= kp 1 −
− h, h > 0, a > 0
dt
a
Example 5.16: For the logistic model with harvesting
dp
p 3
3
= p 1−
−
a = 4, k = 1, h =
dt
4
4
4
determine the long-term consequences for the population
predicted by the model.
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•
•
Stability and family of solutions:
Phase plot:
1dp
dt
dp
>0
dt
1
4
1
3
4
dp
<0
dt
3
p
p
dp
<0
dt
pH0L=3
pH0L=1
t
dies out!
dies out!
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•
Interpretation:
Example 5.16 (continued): Find the time taken until the
1
population dies out if p(0) = .
2
Solve analytically for p(t) and set p(t) = 0.
dp
1
(separable - use
= − (p − 3)(p − 1)
separation
of variables)
dt
4
Note:
Case (2) is unrealistic in practice, as even a small deviation
from p(0) = 1 will result in the solution following case (1) or (3).
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Mixing Problems
Example 5.17: Effluent (pollutant concentration 2g/m3 )
flows into a pond (volume 1000m3 , initially 100g pollutant)
at a rate of 10m3 /min. The pollutant mixes quickly and
uniformly with pond water and flows out of pond at a rate
of 10m3 /min.
Find the concentration of pollutant in the pond at any time,
and interpret the long-term behaviour of the system.
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Derive the ODE:
Let x be the amount (grams) of pollutant in pond at time t
x
minutes. Then C =
is the concentration of pollutant in pond
V
(grams/m3 ), where V is the volume of the pond (m3 ) at time t.
dx
= rate pollutant flows in - rate pollutant flows out
dt
Solve analytically:
Interpret:
x
dx
+
= 20
dt 100
(Linear/Separable)
General solution is
conc. Hgm3L
−t
x(t) = 2000 + ce 100
(working omitted).
Initial condition is x(0) = 100
⇒
2
c = −1900
−t
⇒ x(t) = 2000 − 1900e 100
Find concentration:
0.1
tHminL
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Example 5.18: Derive an ODE describing the amount x
(g) of pollutant in the lake at time t (minutes), if the input
flow rate is decreased to 5m3 /min.
Definitions
1. Transient terms: terms decaying to 0 as t → ∞.
2. Steady state terms: terms NOT decaying to 0 as t → ∞.
The solution for the concentration can be classified as follows.
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Section 6: Second Order Differential Equations
Let V be the volume in pond (m3 ) at time t minutes.
A second order ODE has the form
!
dy d2 y
F x, y, , 2 = 0
dx dx
The general form of a linear second order ODE is
dy
d2 y
+ P(x) + Q(x)y = R(x)
2
dx
dx
• If R(x) = 0, the ODE is homogeneous (H).
• If R(x) , 0, the ODE is inhomogeneous (IH).
Note:
A homogeneous linear ODE is different to a homogeneous type
first order ODE.
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Homogeneous 2nd Order Linear ODEs
The general solution of a second order ODE typically has two
arbitrary constants.
Theorem:
Initial value problem for a second order ODE
The general solution of
Solve
d2 y
dy
+ P(x) + Q(x)y = R(x)
2
dx
dx
y” + P(x)y′ + Q(x)y = 0
is the function y given by
subject to the conditions y(x0 ) = y0 and y′ (x0 ) = y1 .
y(x) = c1 y1 (x) + c2 y2 (x)
where
Boundary value problem for a second order ODE
Solve
• y1 , y2 are two linearly independent solutions of the
homogeneous ODE,
d2 y
dy
+ P(x) + Q(x)y = R(x)
2
dx
dx
• c1 , c2 ∈ R are arbitrary constants.
subject to the conditions y(a) = y0 and y(b) = y1 .
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Aside - A connection with Linear Algebra*
Definition:
Why are these ODEs called linear?
Two functions y1 and y2 are linearly independent if
Because they can be written in terms of a linear transformation.
The ODE
c1 y1 (x) + c2 y2 (x) = 0 ⇒ c1 = c2 = 0
d2 y
dy
+ P(x) + Q(x)y = R(x)
2
dx
dx
or equivalently, if neither function is a non-zero constant
multiple of the other function.
Example 6.1:
(a) Are y1 (x) = x2 , y2 (x) = 2x2 linearly independent?
can be written as
T(y) = R(x)
where
T(y) =
(b) Are y1 (x) = e2x , y2 (x) = xe2x linearly independent?
d2 y
dy
+ P(x) + Q(x)y
2
dx
dx
is a linear transformation on a vector space of functions.
These concepts are covered in MAST10007 Linear Algebra.
* This slide is not examinable in MAST10006.
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Homogeneous 2nd Order Linear ODEs with Constant Coefficients
General form:
ay” + by′ + cy = 0
where a, b, c are constants.
To solve for y(x):
Try y(x) = eλx .
Then y′ (x) = λeλx and y′′ (x) = λ2 eλx .
Substitute into the ODE:
ay′′ + by′ + cy = aλ2 eλx + bλeλx + ceλx = 0
aλ2 + bλ + c eλx = 0
|{z}
,0
⇒ aλ2 + bλ + c = 0
Characteristic Equation
√
−b ± b2 − 4ac
⇒λ=
2a
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Example 6.2: Solve y” + 7y′ + 12y = 0 for y(x).
Solution:
Case 1: b2 − 4ac > 0
• 2 distinct real values λ1 , λ2
• 2 linearly independent solutions
eλ1 x ,
eλ2 x
• General Solution:
y(x) = Aeλ1 x + Beλ2 x
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Case 2: b2 − 4ac = 0
• 1 real value λ =
−b
2a
• 1 solution is eλx
• 2nd linearly independent solution is xeλx (found using variation
of parameters — not in syllabus).
• General Solution:
y(x) = Aeλx + Bxeλx
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We now verify that xeλx is a solution:
Example 6.3: Solve y” + 2y′ + y = 0 for y(x).
If y(x) = xeλx , then
Solution:
λx
y (x) = (λx + 1) e ,
′
y”(x) =
λ2 x + 2λ eλx .
So ay” + by′ + cy
= a λ2 x + 2λ eλx + b (λx + 1) eλx + cxeλx
= xeλx aλ2 + bλ + c + (2λa + b) eλx
|
{z
} | {z }
= 0
=0
=0
So y(x) = xeλx is a solution.
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Case 3: b2 − 4ac < 0
• 2 complex conjugate values
λ1 = α + iβ,
λ2 = α − iβ
• 2 complex linearly independent solutions
e(α+iβ)x ,
e(α−iβ)x
• General Solution:
y(x) = C1 e(α+iβ)x + C2 e(α−iβ)x
where C1 , C2 ∈ C
= C1 eαx cos(βx) + i sin(βx) + C2 eαx cos(βx) − i sin(βx)
= (C1 + C2 ) eαx cos(βx) + (C1 i − C2 i) eαx sin(βx)
| {z }
| {z }
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A
B
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Example 6.4: Solve y” − 4y′ + 13y = 0 for y(x) if y(0) = 1
and y′ (0) = 6.
Put A = C1 + C2 and B = (C1 − C2 )i. If C1 = C2 , then A, B ∈ R.
Solution:
Note:
Imposing real conditions on the ODE will always lead to real
coefficients A and B.
• 2 real linearly independent solutions
eαx cos(βx),
eαx sin(βx)
Real General Solution:
y(x) = Aeαx cos(βx) + Beαx sin(βx)
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This solution has the form y(x) = e2x (a cos θ + b sin θ).
Hence we can rewrite the solution from Example 6.4 as
In general, for a, b > 0,
!
√
a
b
2
2
a cos θ + b sin θ = a + b √
cos θ + √
sin θ
a2 + b2
a2 + b2
=
√
a2 + b2 cos ϕ cos θ + sin ϕ sin θ
=
√
a2 + b2 cos(θ − ϕ).
This form is sometimes preferable for graphing or further
manipulation.
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Inhomogeneous 2nd Order Linear ODEs with Constant
Coefficients
Inhomogeneous 2nd Order Linear ODEs
Theorem:
General form:
The general solution of
ay” + by′ + cy = R(x)
where a, b, c are constants.
y” + P(x)y′ + Q(x)y = R(x)
is the function y given by
Example 6.5: Solve y” + 2y′ − 8y = R(x) where
y(x) = yH (x) + yP (x)
where
(a) R(x) = 1 − 8x2
• yH (x) = c1 y1 (x) + c2 y2 (x) is the general solution of the
homogeneous ODE (called the homogeneous solution, GS(H)),
(b) R(x) = e3x
• yP (x) is a solution of the inhomogeneous ODE (called a
particular solution, PS(IH)),
(c) R(x) = 85 cos x
(d) R(x) = 3 − 24x2 + 7e3x .
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Solution:
Step 2: Find a particular solution of y” + 2y′ − 8y = R(x).
Step 1: Find the general solution of y” + 2y′ − 8y = 0.
(a) R(x) = 1 − 8x2 :
y” + 2y′ − 8y = 1 − 8x2
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(b) R(x) = e3x :
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y” + 2y′ − 8y = e3x
e3x is NOT part of GS(H)
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(c) R(x) = 85 cos x :
y” + 2y′ − 8y = 85 cos x
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Superposition of Particular Solutions
Theorem:
A particular solution of
ay” + by′ + cy = α R1 (x) + β R2 (x)
is
yP (x) = αy1 (x) + βy2 (x)
where
• y1 (x) is a particular solution of ay” + by′ + cy = R1 (x),
• y2 (x) is a particular solution of ay” + by′ + cy = R2 (x),
• a, b, c, α, β are constants.
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Example 6.6: Solve y” − y = ex .
Example 6.5 (d): R(x) = 3 − 24x2 + 7e3x .
Solution:
Solution:
GS(H) : yH (x) = Aex + Be−x
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Example 6.7: Solve y” + 2y′ + y = e−x .
Solution:
GS(H) : yH (x) = (A + Bx) e−x
Example 6.8: Solve y” + 49y = 28 sin(7t).
Solution:
GS(H) : yH (t) = A cos(7t) + B sin(7t)
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The forces are:
Springs - Free Vibrations
Consider an object (of mass m kg) attached to a spring hanging
from a fixed support.
• gravitational force, given by the gravitational law:
W = mg
Suppose that the natural length of the spring when unloaded is
L m, and that when the object is attached, it causes the spring
to stretch by s m downwards at equilibrium.
(g = 9.8m/s2 on Earth)
• restoring force in spring, given by Hooke’s Law:
T = −k · extension
(k > 0)
0
spring constant
Note:
The negative sign in Hooke’s law is because the direction of the
force T is opposite to the direction of extension:
▶ if the spring is stretched downwards, then it pulls up
▶ if the spring is compressed upwards, then it pushes down.
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Suppose the object is set in motion.
Let y(t) be the displacement of the object below the equilibrium
position (y = 0) at time t seconds.
At equilibrium, the net force is zero, so
Note:
Since displacement y is measured below the equilibrium
position, downwards is the positive direction.
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Derive the equation of motion
Newton’s Law states that
When the object is moving, there is an extra force acting:
net force = mass · acceleration
• damping force is proportional to velocity
R = −βẏ
Fnet =
m
·
ÿ
(β ≥ 0)
Apply Newton’s Law to the object:
0
damping constant
Note:
The negative sign is because the direction of the damping force
is opposite the direction of motion.
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To solve, try y(t) = eλt
⇒ mλ2 + βλ + k = 0
⇒ λ=
• If β = 0 :
λ = ±ib
√
• If 0 < β < 2 mk :
−β ±
β2 − 4mk
2m
p
simple harmonic motion
λ = a ± ib
underdamped, weak damping
√
• If β = 2 mk :
λ = a, a
critical damping
√
• If β > 2 mk :
λ = a, b
overdamped, strong damping
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Example 6.9: A 40
kg mass stretches a spring hanging
49
from a fixed support by 0.2m. The mass is released from
the equilibrium position with a downward velocity of 3m/s.
Find the position of the mass y below equilibrium at any
time t, if the damping constant β is:
(a) 0
(b)
160
49
(c)
80
7
(d)
2000
49
Solution:
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(a) β = 0 :
ÿ + 49y = 0
y
3
7
Equil.
t
Π
7
-
2Π
7
3Π
7
3
7
Simple harmonic motion
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(b) β =
160
49
:
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ÿ + 4ẏ + 49y = 0
y
1
5
Equil.
t
1
-
1
2
Weak damping
5
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(c) β =
80
7
ÿ + 14ẏ + 49y = 0
:
y
0.15
0.1
critical damping
0.05
Equil.
t
0.5
1
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(d) β =
2000
49
:
ÿ + 50ẏ + 49y = 0
y
0.06
0.03
strong damping
Equil.
t
2
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4
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Springs - Forced Vibrations
Example 6.10: Apply an external downwards force
f (t) =
If an external downwards force f is applied to the spring-mass
system at time t, the forces acting on the mass are:
160
7
sin(7t) in Example 6.9.
Solution:
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(a) β =
GS(IH) :
80
7
:
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ÿ + 14ẏ + 49y = 28 sin(7t)
y(t) = (A + Bt) e−7t − 72 cos(7t)
y
0.4
GSHHL contributes
Equil.
1
-0.4
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2
3
t
4
oscillatory motion due to PSHIHL
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(b)
β=0:
GS(IH) :
ÿ + 49y = 28 sin(7t)
y
10
y(t) = A cos(7t) + B sin(7t) − 2t cos(7t)
5
Equil.
2
4
6
t
-5
Resonance
-10
Definition
Resonance: Resonance occurs when the external force f has
the same form as one of the terms in the GS(H).
If β = 0, then the PS(IH) will grow without bound as t → ∞.
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RLC series electric circuit
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RLC series electric circuit
The circuit components are
An RLC series electric circuit is an electric circuit with 4
components connected sequentially in a loop:
Circuits such as this are common in radio communications.
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RLC series electric circuit
Let q(t) be the charge on the capacitor (measured in Coulomb)
at time t seconds.
The charge satisfies the second-order ODE
L
d2 q
dq q
+R + =V
2
dt C
dt
This equation has the same form as the equation of motion for
a spring with external driving force, and can exhibit all the same
solution types as the spring system.
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Section 7: Functions of Two Variables
We can represent the function f by its graph in R3 . The graph
of f is:
n
o
(x, y, z) ∈ R3 : (x, y) ∈ D and z = f (x, y) .
Example
The temperature T at a point on the Earth’s surface at a given
time depends on the latitude x and the longitude y. We think of
T being a function of the variables x, y and write T = f (x, y).
This is a surface lying directly above the domain D. The x and y
axes lie in the horizontal plane and the z axis is vertical.
In general
A function of two variables is a mapping f that assigns a unique
real number z = f (x, y) to each pair of real numbers (x, y) in
some subset D of the xy plane R2 . We also write
f :D→R
where D is called the domain of f .
Example
If f (x, y) = x2 + y3 then f (2, 1) = 4 + 1 = 5.
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Equations of a Plane
The Cartesian equation of a plane has the form
ax + by + cz = d
where a, b, c, d are real constants.
n = ai + bj + ck is a normal vector to the plane.
In fact, the plane passing through a point (x0 , y0 , z0 ) with a
normal vector (a, b, c) consists of the points (x, y, z) such that
(a, b, c) is perpendicular to (x − x0 , y − y0 , z − z0 ) and thus has
equation
a(x − x0 ) + b(y − y0 ) + c(z − z0 ) = 0,
that is,
ax + by + cz = ax0 + by0 + cz0 .
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Example 7.1: Sketch the plane 4x + 3y + z = 2.
Solution:
Level Curves
Sketching Functions of Two Variables
The key steps in drawing a graph of a function of two variables
z = f (x, y) are:
A curve on the surface z = f (x, y) for which z is a constant is a
contour.
1. Draw the x, y, z axes.
For right handed axes: the positive x axis is towards you,
the positive y axis points to the right, and the positive z axis
points upward.
The same curve drawn in the xy plane is a level curve.
So a level curve of f has the form
2. Draw the y − z cross section.
{(x, y) : f (x, y) = c}
3. Draw some level curves and their contours.
4. Draw the x − z cross section.
where c ∈ R is a constant.
5. Label any x, y, z intercepts and key points.
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Example 7.2: Find the level curves,
and cross sections in
p
2
the x-z and y-z planes of z = 1 − x − y2 . Hence sketch
the surface and identify it.
Solution:
y
H0,1L
H-1,0L
c=1
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c=0
Level curves
H1,0L
x
H0,-1L
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Consider cross sections (slices) to help sketch graph.
z
z
H0,1L
H-1,0L
Surface is a hemisphere radius 1, centre at (0, 0, 0) for z ≥ 0.
H0,1L
H1,0L
H-1,0L
x
H1,0L
y
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Example 7.3: Sketch the graph of z = 4x2 + y2 .
Consider cross sections (slices) to help sketch graph.
Solution:
y
H0,2L
c=4
z
4
Level curves
H-1,0L
H1,0L
z
4
z=4x2
x
z=y2
c=0
-1
1
x
-1
1
y
H0,-2L
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Example 7.4: Sketch the graph of z =
The surface is an elliptic paraboloid (parabolic bowl).
p
4x2 + y2 .
Solution:
y
H0,2L
c=2
Level curves
H-1,0L
H1,0L
x
c=0
H0,-2L
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Cross sections
The surface is an elliptic cone.
z
z
2
-1
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2
x
1
z=2ÈxÈ
-1
y
1
z=ÈyÈ
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Limits
Continuity
Let f : D → R be a real-valued function, where D ⊆ R2 .
We say f has the limit L as (x, y) approaches (x0 , y0 )
lim
(x,y)→(x0 ,y0 )
Let f : R2 → R be a real-valued function.
f (x, y) = L
f is continuous at (x, y) = (x0 , y0 ) if
if when (x, y) approaches (x0 , y0 ) along ANY path in the domain,
f (x, y) gets arbitrarily close to L.
lim
(x,y)→(x0 ,y0 )
f (x, y) = f (x0 , y0 )
Note:
Note:
The continuity theorems for functions of one variable can be
generalised to functions of two variables.
1 L must be finite.
2 The limit can exist if f is undefined at (x0 , y0 ).
3 The usual limit laws apply.
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Example 7.5: Let f (x, y) = x2 + y2 . For which values of x
and y is f continuous?
Example 7.6: Evaluate
lim
(x,y)→(2,1)
log(1 + 2x2 + 3y2 ).
Solution:
Solution:
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First Order Partial Derivatives
Geometric Interpretation of
Let f : R2 → R be a real-valued function. The first order partial
derivatives of f with respect to the variables x and y are defined
by the limits:
fx =
∂f
f (x + h, y) − f (x, y)
= lim
h
∂x
h→0
fy =
∂f
f (x, y + h) − f (x, y)
= lim
h
∂y
h→0
∂f
∂f
and
∂x
∂y
Note:
•
•
∂f
measures the rate of change of f with respect to x
∂x
when y is held constant.
∂f
measures the rate of change of f with respect to y
∂y
when x is held constant.
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Example 7.7: Let f (x, y) = xy2 . Find
∂f
from first
∂y
principles.
Let C1 be the curve where the vertical plane y = y0 intersects
∂f
the surface. Then
gives the slope of the tangent to C1
∂x (x0 ,y0 )
at (x0 , y0 , z0 ).
Solution:
Let C2 be the curve where the vertical plane x = x0 intersects
∂f
the surface. The
gives the slope of the tangent to C2 at
∂y (x0 ,y0 )
(x0 , y0 , z0 ).
•
T1 and T2 are the tangent lines to C1 and C2 .
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Example 7.8: Let f (x, y) = 3x3 y2 + 3xy4 . Find
Example 7.9: Let f (x, y) = y log x + x tanh(3y). Find fx , fy at
(1, 0).
∂f
∂f
and
.
∂x
∂y
Solution:
Solution:
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The tangent line T1 has equation (y = y0 fixed):
Tangent Planes and Differentiability
Let f : R2 → R be a real-valued function. We say that f is
differentiable at (x0 , y0 ) if the tangent lines to all curves on the
surface z = f (x, y) passing through (x0 , y0 , z0 ) form a plane,
called the tangent plane.
z − z0 =
∂f
∂x
(x0 ,y0 )
(x − x0 )
The tangent line T2 has equation (x = x0 fixed):
z − z0 =
This holds if fx and fy exist and are continuous near (x0 , y0 ).
∂f
∂y
(x0 ,y0 )
(y − y0 )
Since a plane passing through (x0 , y0 , z0 ) has the form
z − z0 = α(x − x0 ) + β(y − y0 )
the tangent plane has equation
z − z0 =
∂f
∂x
(x0 ,y0 )
∂f
∂x
(x0 ,y0 )
(x − x0 ) +
∂f
∂y
(x0 ,y0 )
(x − x0 ) +
∂f
∂y
(x0 ,y0 )
(y − y0 )
or equivalently,
z = z0 +
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(y − y0 ).
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Linear Approximations
Example 7.10: Find the equation of the tangent plane to
the surface z = f (x, y) = 2x2 + y2 at (1, 1, 3).
Solution:
If f is differentiable at (x0 , y0 ), we can approximate z = f (x, y) by
its tangent plane at (x0 , y0 , z0 ), when (x, y) is close to (x0 , y0 ).
That is:
f (x, y) ≈ z0 +
∂f
∂x
(x0 ,y0 )
|
(x − x0 ) +
∂f
∂y
(x0 ,y0 )
{z
(y − y0 )
}
equation of tangent plane
when (x, y) is close to (x0 , y0 ).
This is called the linear approximation to f near (x0 , y0 ).
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Example 7.11: Find the linear approximation of
f (x, y) = xexy at (1, 0). Hence, approximate f (1.1, −0.1).
Solution:
Note:
The actual value is
(1.1)e−0.11 ≈ 0.98542
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Approximate Change
Example 7.12: Let z = f (x, y) = x2 + 3xy − y2 . If x changes
from 2 to 2.05 and y changes from 3 to 2.96, estimate the
change in z.
Rearranging the linear approximation equation, we get
f (x, y) − f (x0 , y0 ) ≃
∂f
∂x
(x0 ,y0 )
(x − x0 ) +
∂f
∂y
Solution:
(x0 ,y0 )
(y − y0 ).
Let ∆x = x − x0 , ∆y = y − y0 , ∆f = z − z0 = f (x, y) − f (x0 , y0 ).
The approximate change in f near (x0 , y0 ), for small changes ∆x
and ∆y in x and y, is:
∆f ≈
∂f
∆x
∂x (x ,y )
0 0
+
∂f
∆y
∂y (x ,y )
0 0
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Second Order Partial Derivatives
Let f : R2 → R be a real-valued function. The second order
partial derivatives of f with respect to x and y are defined by:
• fxx
Note:
• fyy
The actual change in f is
∆f
• fxy
= f (2.05, 2.96) − f (2, 3)
= 13.6449 − 13
= 0.6449
• fyx
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!
∂2 f
∂ ∂f
= fx =
= 2
x
∂x ∂x
∂x
!
∂2 f
∂ ∂f
= 2
= fy =
y
∂y ∂y
∂y
!
∂2 f
∂ ∂f
= fx =
=
y
∂y ∂x
∂y∂x
!
∂2 f
∂ ∂f
= fy =
=
x
∂x ∂y
∂x∂y
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Example 7.13: Find the second order partial derivatives of
f : R2 → R given by f (x, y) = x sin(x + 2y).
Solution:
Theorem:
If the second order partial derivatives of f exist and are
continuous then fxy = fyx .
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Chain Rule
1. If z = f (x, y) and x = g(t), y = h(t) are differentiable
functions, then z = f (g(t), h(t)) is a function of t, and
dz ∂z dx ∂z dy
=
+
dt ∂x dt ∂y dt
Note:
fxy = fyx as expected since trigonometric functions and
polynomials are continuous for all (x, y) ∈ R2 .
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dz
Example 7.14: If z = x2 − y2 , x = sin t, y = cos t. Find
at
dt
π
t= .
6
Solution:
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Example 7.15: If z = ex sinh y, x = st2 , y = s2 t.
∂z
Find .
∂s
2. If z = f (x, y) and x = g(s, t), y = h(s, t) are differentiable
functions, then z is a function of s and t with
∂z ∂z ∂x ∂z ∂y
=
+
∂s ∂x ∂s ∂y ∂s
Solution:
∂z ∂z ∂x ∂z ∂y
=
+
∂t ∂x ∂t ∂y ∂t
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Directional Derivatives
The straight line starting at P0 = (x0 , y0 ) with velocity û = (u1 , u2 )
has parametric equations:
Let û = (u1 , u2 ) be a unit vector in the xy-plane (so + = 1).
The rate of change of f at P0 = (x0 , y0 ) in the direction û is the
directional derivative Dû f P .
u21
u22
x = x0 + tu1 , y = y0 + tu2 .
Hence,
0
Geometrically this represents the slope of the surface z = f (x, y)
above the point P0 in the direction û.
Dû f
= rate of change of f along the straight line at t = 0
P0
= value of
d
f (x0 + tu1 , y0 + tu2 ) at t = 0
dt
= fx (x0 , y0 )x′ (0) + fy (x0 , y0 )y′ (0)
by the chain rule
= fx (x0 , y0 ) u1 + fy (x0 , y0 ) u2 .
We can also write this as a dot product
!
∂f
∂f
Dû f P =
,
· (u1 , u2 ).
0
∂x P0 ∂y P0
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Gradient Vectors
Example 7.16: Find the directional derivative of f (x, y) = xey
1
at (2, 0) in the direction from (2, 0) towards , 2 .
2
If f : R2 → R is a differentiable function, we can define the
gradient of f to be the vector
∂f
∂f ∂f
∂f
i+ j=
,
grad f = ∇f =
∂x
∂y
∂x ∂y
Solution:
•
!
direction û
Then the directional derivative of f at the point P0 in the
direction û is the dot product
Dû f
P0
= ∇f
P0
· û
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Example 7.17: Find
! the directional derivative of
x
π
f (x, y) = arcsin
at (1, 2) in the direction anticlockwise
y
4
from the positive x axis.
Solution:
•
direction û
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Properties of ∇f and Dû f
So for fixed ∇f :
•
Dû f is maximum when cos θ = 1 so θ = 0
The directional derivative of f is
Dû f
= ∇f · û
= |∇f | |û| cos θ
⇒ f increases most rapidly along ∇f .
= |∇f | cos θ
•
Dû f is minimum when cos θ = −1 so θ = π
where θ is the angle between ∇f and û, and |v| denotes the
length of a vector v.
⇒ f decreases most rapidly along −∇f .
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•
Dû f = 0 when cos θ = 0 so θ =
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Example 7.18: Let f (x, y) = 4x2 + y2 .
(a) Find ∇f at (1, 0) and (0, 2).
(b) Show that ∇f is perpendicular to the level curves, by
sketching ∇f at these points and the level curves of f .
π
and ∇f ⊥ û.
2
Solution:
But Dû f = 0, whenever û is tangent to a level curve of f (where
f = constant).
⇒ ∇f ⊥ level curves of f
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Example 7.19: In what direction does f (x, y) = xey
(b)
(a) increase
y
(b) decrease
most rapidly at (2, 0)? Express direction as a unit vector.
4j
Solution:
0,2
From Example 7.16
Level curves of f x,y
1,0
8i
∇f (2, 0) = i + 2j
x
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Stationary Points
A stationary point of f is a point (x0 , y0 ) at which
∇f = 0
So
∂f
∂f
= 0 and
= 0 simultaneously at (x0 , y0 ).
∂x
∂y
Geometrically, this means that the tangent plane to the graph
z = f (x, y) at (x0 , y0 ) is horizontal, i.e. parallel to the xy-plane.
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Three important types of stationary points are
A function f has a
1. local maximum at (x0 , y0 ) if f (x, y) ≤ f (x0 , y0 ) for all (x, y) in
some disk centred at (x0 , y0 ),
2. local minimum at (x0 , y0 ) if f (x, y) ≥ f (x0 , y0 ) for all (x, y) in
some disk centred at (x0 , y0 ),
3. saddle point at (x0 , y0 ) if (x0 , y0 ) is a stationary point, and
there are points near (x0 , y0 ) with f (x, y) > f (x0 , y0 ) and
other points near (x0 , y0 ) with f (x, y) < f (x0 , y0 ).
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Second Derivative Test
Any local maximum or minimum of f will occur at a critical point
(x0 , y0 ) such that
1. ∇f (x0 , y0 ) = 0
2.
If ∇f (x0 , y0 ) = 0 and the second partial derivatives of f are
or
continuous on an open disk centred at (x0 , y0 ), consider the
Hessian function
∂f
∂f
and/or
do not exist at (x0 , y0 ).
∂x
∂y
evaluated at (x0 , y0 ).
H(x, y) = fxx fyy − (fxy )2
Then (x0 , y0 ) is a
1. local minimum if H(x0 , y0 ) > 0 and fxx (x0 , y0 ) > 0.
2. local maximum if H(x0 , y0 ) > 0 and fxx (x0 , y0 ) < 0.
3. saddle point if H(x0 , y0 ) < 0.
q
z = x2 + y2 . Minimum at (0, 0) BUT ∇f does not exist at (0, 0).
Note: Test is inconclusive if H(x0 , y0 ) = 0.
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Example 7.20: Find and classify the stationary points of
f : R2 → R given by f (x, y) = x3 + y3 + 3x2 − 3y2 − 8.
Solution:
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Example 7.21: Find and classify the stationary points of
f : R2 → R given by f (x, y) = y sin x.
Solution:
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Partial Integration
Let f : R2 → R be a continuous function over a domain D in R2 .
The partial indefinite integrals of f with respect to the first and
second variables (say x and y) are denoted by:
Z
Z
f (x, y) dx and
f (x, y) dy.
Z
f (x, y) dx is evaluated by holding y fixed and integrating
•
with respect to x.
Z
•
f (x, y) dy is evaluated by holding x fixed and integrating
with respect to y.
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Z
Example 7.22: Evaluate
Z
(3x2 y + 12y2 x3 ) dx.
1
(3x2 y + 12y2 x3 ) dy.
Example 7.23: Evaluate
0
Solution:
Solution:
Note:
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Double Integrals
Let f : R2 → R be a continuous function over a domain D in R2 .
We can evaluate the double integral:
"
"
f (x, y) dx dy
f (x, y) dA =
Δx
D
D
"
Δy
f (x, y) dA is the volume under the surface z = f (x, y) that
D
lies above the domain D in the xy plane, if f (x, y) ≥ 0 in D.
Volume of thin rod = (Area base) · (height)
| {z } | {z }
∥
∆x∆y
∥
f (x, y)
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Double Integrals Over Rectangular Domains
The double integral is defined as the limit of sums of the
volumes of the rods:
"
Definitions
1. R = [a, b] × [c, d] is a rectangular domain defined by
a ≤ x ≤ b, c ≤ y ≤ d.
"
f (x, y) dA =
D
f (x, y) dx dy
D
=
lim lim
∆x→0 ∆y→0
n
X
f (x, y)∆x∆y i
i=1
Note:
If f (x, y) = 1 then
"
"
dA =
D
dx dy
D
2.
gives the area of the domain D.
R dR b
c
a
f (x, y) dx dy =
R d R b
c
a
f (x, y) dx dy means integrate
with respect to x first and then integrate with respect to y.
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"
Fubini’s Theorem
(x2 + y2 ) dx dy if
Example 7.24: Evaluate
R = [−1, 1] × [0, 1].
Solution:
Let f : R2 → R be a continuous function over the domain
R = [a, b] × [c, d]. Then
"
Z dZ b
f (x, y)dA =
f (x, y) dx dy
R
c
a
d
bZ
Z
R
=
f (x, y) dy dx
a
c
So order of integration is not important.
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Note:
As expected, the order of integration is not important since
polynomials are continuous for all (x, y) ∈ R2 .
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Example 7.25: Using double integrals, find the volume of
the wedge shown below.
Solution:
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