SEMESTER II MATHEMATICS GENERAL INTEGRAL CALCULUS AND DIFFERENTIAL EQUATIONS

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SEMESTER II MATHEMATICS GENERAL
LECTURE NOTE
INTEGRAL CALCULUS AND DIFFERENTIAL EQUATIONS
TARUN KUMAR BANDYOPADHYAY, DEPARTMENT OF MATHEMATICS
In case you face difficulty in understanding the following material,
you may e-mail to me at tbanerjee1960@gmail.com stating
your Name and Roll No.
DOWNLOAD SITE: WWW.SXCCAL.EDU
1
SECTION I (Integral Calculus)
Text: An Introduction to Analysis: Integral Calculs— K. C. Maity,
R. K. Ghosh
CHAPTER 1: DEFINITE INTEGRALS—A REVISION
Let f be a real valued continuous function defined on a
closed and bounded interval [a,b]. Let us choose a
partition (collection of finite number of points of [a,b]
including a and b) P = {a = x0,x1,x2,…,xn=b} of [a,b] (for
example: {0,1/2,1} is a partition for [0,1].How many
partitions are there for a given interval—finite or infinite?).
Fig 1: Area under a curve is approximated by sum of areas of rectangles
2
Let 𝛿 r = xr-xr-1, r = 1,…,n and 𝛿 = max⁑{𝛿r| r = 1,2,…,n}.
Choose an arbitrary point cr∈(xr-1,xr) for all r and
consider sum of areas of rectangles ∑𝑛1 𝑓(π‘π‘Ÿ )π›Ώπ‘Ÿ . It can
be seen that this sum approaches more closely the
actual area under the curve if we make width of the
rectangles smaller , that is, if we increase number n of
points of subdivision (sum of areas of two rectangles on πœΉπ’“ gives
a better approximation to the area under the curve than area of a single
rectangle).
Definition
1.1
𝒃
⁑∫𝒂 𝒇(𝒙)𝒅𝒙 = ⁑ π₯𝐒𝐦 ∑π’πŸ 𝒇(𝒄𝒓 )πœΉπ’“
𝒏→∞
,
provided the limit exists independent of choice of
points of subdivision xi and that of ci , for all i.
It can be proved that for a continuous function f defined
𝒃
over a closed bounded interval [a,b], ∫𝒂 𝒇(𝒙)𝒅𝒙 exists in
above sense.
𝒃
Simpler equivalent expression for calculating ∫𝒂 𝒇(𝒙)𝒅𝒙:
3
We can make choices of xi and ci suitably so as to obtain
𝑏
equivalent simpler expression of ∫π‘Ž 𝑓 (π‘₯ )𝑑π‘₯.
οƒ˜ Let us choose xi’s equi-spaced, that is , 𝛿 1 = 𝛿 2 = … = 𝛿 n
𝑏
= (b-a)/n. Then∫π‘Ž 𝑓 (π‘₯ )𝑑π‘₯ = ⁑ lim
𝑏−π‘Ž
𝑛→∞ 𝑛
∑𝑛1 𝑓(π‘π‘Ÿ ).
οƒ˜ Let us choose cr = a+rh, r = 1,…,n, where h = (b-a)/n.
Then
𝑏
∫π‘Ž 𝑓 (π‘₯ )𝑑π‘₯ = ⁑ lim
𝑏−π‘Ž
𝑛→∞ 𝑛
∑𝑛1 𝑓(π‘Ž + π‘Ÿ
𝑏−π‘Ž
𝑛
=
)
lim β„Ž ∑𝑛1 𝑓(π‘Ž + π‘Ÿβ„Ž).
β„Ž→0
As
a
special
1
case, ∫0 𝑓 (π‘₯ )𝑑π‘₯⁑ = ⁑ lim
1
𝑛→∞ 𝑛
π‘Ÿ
∑𝑛1 𝑓 ( ) =
𝑛
lim β„Ž ∑𝑛1 𝑓(π‘Ÿβ„Ž)
β„Ž→0
1
Example 1.1 From definition, calculate ∫0 π‘₯ 2 𝑑π‘₯.
1
» ∫0 π‘₯ 2 𝑑π‘₯ = lim β„Ž ∑𝑛1(π‘Ÿβ„Ž)2 = lim
β„Ž→0
β„Ž→0
(π‘›β„Ž)(π‘›β„Ž+β„Ž)(2π‘›β„Ž+β„Ž)
6
= 1/3,
since nh = 1 holds, for every positive integer n and the
corresponding h.
Fundamental Theorem of Integral Calculus
4
𝑏
Theorem 1.1 If ∫π‘Ž 𝑓(π‘₯ )𝑑π‘₯⁑exists and if there exists a
function g:[a, b]→R such that g1(x) = f(x)(suffix denotes
𝑏
order of differentiation) on [a, b], then ∫π‘Ž 𝑓(π‘₯ )𝑑π‘₯⁑ =
g(b) – g(a).
NOTE: g is called a primitive of f. A function f may not
𝑏
possess a primitive on [a,b] but ∫π‘Ž 𝑓 (π‘₯ )𝑑π‘₯⁑ may exist ;
𝑏
in that case, ⁑∫π‘Ž 𝑓(π‘₯ )𝑑π‘₯⁑ can not be calculated using
fundamental theorem. Primitives of f on [a, b] are
given by the indefinite integral ∫ 𝑓(π‘₯ )𝑑π‘₯ : that is the
reason
why
we
consider
indefinite
integrals.
1
Example ∫0 π‘₯ 2 𝑑π‘₯ exists, since x2 is continuous on
π‘₯3
[0,1]. Also g(x)=∫ π‘₯ 𝑑π‘₯=
2
[0,1].
1
Hence
1
3
+c is a primitive of x2 on
Fundamental
1
∫0 π‘₯ 2 𝑑π‘₯=(3+c)-c=3.
5
Theorem
gives
1
Note ∫0 π‘₯ 2 𝑑π‘₯ ⁑ is independent of c though ∫ π‘₯ 2 𝑑π‘₯
involves c.
PROPERTIES OF DEFINITE INTEGRALS
We assume below that the definite integrals exist and
𝑏
whenever we consider ∫π‘Ž 𝑓 (π‘₯ )𝑑π‘₯⁑, a primitive g to f
over [a,b] exists, so that we can apply Fundamental
π‘Ž
𝑏
Theorem. For a<b, we define ∫𝑏 𝑓 (π‘₯ )𝑑π‘₯ = - ∫π‘Ž 𝑓 (π‘₯ )𝑑π‘₯⁑.
𝑏
𝑐
𝑏
1. ∫π‘Ž 𝑓 (π‘₯ )𝑑π‘₯⁑ = ∫π‘Ž 𝑓 (π‘₯ )𝑑π‘₯⁑ + ∫𝑐 𝑓 (π‘₯ )𝑑π‘₯⁑ (irrespective of
relative algebraic magnitude of a,b,c)
1
4
Example ∫3 π‘₯ 2 𝑑π‘₯+∫1 π‘₯ 2 𝑑π‘₯=
3
− ∫1 π‘₯ 2 𝑑π‘₯
37⁑
4
⁑∫1 π‘₯ 2 𝑑π‘₯
+
4
=∫3 π‘₯ 2 𝑑π‘₯.
7
π‘Ž
1
64
3
3
= − (9 − ) + (
π‘Ž
2. ∫0 𝑓(π‘₯ )𝑑π‘₯ = ∫0 𝑓(π‘Ž − π‘₯ )𝑑π‘₯
6
1
− )=
3
Example
πœ‹⁄
πœ‹
2 sin π‘₯⁑𝑑π‘₯ = ⁄2 cos π‘₯⁑𝑑π‘₯
∫0
∫0
π‘Ž
π‘Ž/2
3. ∫0 𝑓(π‘₯ )𝑑π‘₯ = ⁑ ∫0
π‘Ž/2
𝑓(π‘₯ )𝑑π‘₯ + ∫0
𝑓 (π‘Ž − π‘₯ )𝑑π‘₯
.
In
particular, if f(a-x) = f(x)for all x in [0,a], then
π‘Ž
π‘Ž/2
∫0 𝑓(π‘₯ )𝑑π‘₯ = 2 ∫0
𝑓 (π‘₯ )𝑑π‘₯ and if f(a-x) = - f(x) for all x
π‘Ž
in [0,a], then ∫0 𝑓(π‘₯ )𝑑π‘₯ = 0.
π‘›π‘Ž
π‘Ž
4. ∫0 𝑓 (π‘₯ )𝑑π‘₯ = 𝑛 ∫0 𝑓(π‘₯ )𝑑π‘₯ , if f(a+x) = f(x), n natural.
π‘Ž
π‘Ž
5. ∫−π‘Ž 𝑓 (π‘₯ )𝑑π‘₯ = ⁑ ∫0 {𝑓(π‘₯ ) + 𝑓(−π‘₯ )}𝑑π‘₯
π‘Ž
.
π‘Ž
If
f
is
π‘Ž
even,∫−π‘Ž 𝑓(π‘₯ )𝑑π‘₯ = 2 ∫0 𝑓(π‘₯ )𝑑π‘₯. If f is odd, ∫−π‘Ž 𝑓(π‘₯)⁑𝑑π‘₯=
0.
Example
1
∫−1 π‘₯ 3 cos 2π‘₯⁑𝑑π‘₯ =0,
1
2∫0 π‘₯ 4 cos 2π‘₯⁑𝑑π‘₯
7
1
∫−1 π‘₯ 4 cos 2π‘₯⁑𝑑π‘₯ =
PRACTICE SUMS
πœ‹
2
1. Evaluate:∫0
√sin π‘₯
𝑑π‘₯ .
√sin π‘₯+√cos π‘₯
2 π‘₯ 2 sin π‘₯
2. Evaluate:∫−2 6
𝑑π‘₯
π‘₯ +12
3. If f(x) = f(x+ kp) for all integer values of k, show that
𝑛𝑝
𝑝
∫0 𝑓(π‘₯ )𝑑π‘₯ = 𝑛 ∫0 𝑓(π‘₯ )𝑑π‘₯ .
CHAPTER 2: REDUCTION FORMULA
In this chapter, we study how to decrease complexity
of some integrals in a stepwise manner by the use of
recurrence relation that we derive generally using
integration by parts formula.
1. Let In = ∫ 𝑠𝑖𝑛𝑛 π‘₯⁑𝑑π‘₯ , n natural.
In
= ∫ 𝑠𝑖𝑛𝑛−1 π‘₯ sin π‘₯⁑𝑑π‘₯ =
sinn-1x(-cos
x)-
(n-
1) ∫ 𝑠𝑖𝑛𝑛−2 π‘₯⁑ cos π‘₯⁑(− cos π‘₯)⁑𝑑π‘₯ = sinn-1x(-cos x)+(n-
8
1)∫ 𝑠𝑖𝑛𝑛−2 π‘₯ (1 − 𝑠𝑖𝑛2 π‘₯ )𝑑π‘₯= -sinn-1x cos x+(n-1)In-2-(n1)In. hence In=−
If
we
𝑠𝑖𝑛𝑛−1 π‘₯π‘π‘œπ‘ β‘π‘₯
𝑛
denote
𝑠𝑖𝑛𝑛−1 π‘₯π‘π‘œπ‘ β‘π‘₯ πœ‹⁄2
−
|0
𝑛
+
+
𝑛−1
𝑛
πœ‹⁄
∫0 2 𝑠𝑖𝑛𝑛 π‘₯⁑𝑑π‘₯,
Jn
=
𝑛−1
Jn-2 =
𝑛
In-2.
𝑛−1
𝑛
then
Jn
=
Jn-2. By repeated
application of the reduction formula, it can be proved
that Jn=
𝑛−1
𝑛
𝑛−1 𝑛−3
Jn-2=…=
𝑛 𝑛−2
1
𝑛−1 𝑛−3
2
𝑛 𝑛−2
… . 𝐽0 =
𝑛−1 𝑛−3
even natural and Jn =
𝑛 𝑛−2
1 πœ‹
… . , if n is
2 2
2
𝑛−1 𝑛−3
3
𝑛 𝑛−2
… 𝐽1 =
2
… , if n is
3
odd natural.
2. Let In = ∫ π‘‘π‘Žπ‘›π‘› π‘₯⁑𝑑π‘₯ , n natural.
Then
In
=∫ π‘‘π‘Žπ‘›
Also,
3. Let
𝑛−2
=
∫ π‘‘π‘Žπ‘›π‘›−2 π‘₯. π‘‘π‘Žπ‘›2 π‘₯⁑𝑑π‘₯
π‘₯. (𝑠𝑒𝑐 π‘₯ − 1)⁑𝑑π‘₯ =
2
π‘‘π‘Žπ‘›π‘›−1 π‘₯
𝑛−1
− 𝐼𝑛−2 .
πœ‹⁄
π‘‘π‘Žπ‘›π‘›−1 π‘₯ πœ‹⁄4
1
𝑛
4
Jn = ∫0 π‘‘π‘Žπ‘› π‘₯⁑𝑑π‘₯=
|0 -Jn-2=
𝑛−1
𝑛−1
In
= ∫ 𝑠𝑒𝑐 𝑛 π‘₯⁑𝑑π‘₯ ,
∫ 𝑠𝑒𝑐 𝑛−2 π‘₯. 𝑠𝑒𝑐 2 π‘₯⁑𝑑π‘₯
n
=
natural.
secn-2x
9
− Jn-2.
Then
tanx
–
In
=
(n-
2)⁑∫ 𝑠𝑒𝑐 𝑛−2 π‘₯. (𝑠𝑒𝑐 2 π‘₯ − 1)⁑𝑑π‘₯ = secn-2x tan x – (n-2)(In𝑠𝑒𝑐 𝑛−2 π‘₯ tan π‘₯ 𝑛−2
In-2). Hence In =
4. Let
Im,n
∫(𝑠𝑖𝑛 π‘₯π‘π‘œπ‘ β‘π‘₯)β‘π‘π‘œπ‘ 
∫ π‘π‘œπ‘ 
𝑛−2
∫ π‘π‘œπ‘ 
𝑛−2
Im,n-2-
𝑛−1
π‘š+1
𝑛−1
π‘š+1
𝑛−1
π‘š+1
𝐼 .
𝑛−1 𝑛−2
=
π‘š
𝑛−1
+
𝑛−1
𝑛−1
∫ π‘ π‘–π‘›π‘š π‘₯β‘π‘π‘œπ‘  𝑛 π‘₯ 𝑑π‘₯
=
π‘₯ 𝑑π‘₯
π‘š
π‘ π‘–π‘›π‘š+1 π‘₯β‘π‘π‘œπ‘  𝑛−1 π‘₯
π‘š+1
π‘ π‘–π‘›π‘š+1 π‘₯β‘π‘π‘œπ‘  𝑛−1 π‘₯
=
2
π‘₯𝑠𝑖𝑛 π‘₯⁑𝑠𝑖𝑛 π‘₯⁑𝑑π‘₯
π‘š+1
π‘₯𝑠𝑖𝑛 π‘₯⁑(1 − π‘π‘œπ‘  π‘₯)⁑𝑑π‘₯ =
π‘š
𝐼 .
π‘š+1 π‘š,𝑛
2
π‘ π‘–π‘›π‘š+1 π‘₯β‘π‘π‘œπ‘  𝑛−1 π‘₯
π‘š+1
=
+
+
+
Transposing and simplifying, we get
a reduction formula for Im,n.
5. Let
π‘š
𝑛
π‘š
𝑛
Im,n
∫ π‘π‘œπ‘ 
π‘š−1
= ∫ π‘π‘œπ‘  π‘₯ sin 𝑛π‘₯⁑𝑑π‘₯ =
-
π‘š
π‘₯ sin π‘₯ cos 𝑛π‘₯⁑𝑑π‘₯
∫ π‘π‘œπ‘  π‘š−1 π‘₯ sin 𝑛π‘₯ cos π‘₯⁑𝑑π‘₯
=
+
-
π‘π‘œπ‘  π‘š π‘₯ cos 𝑛π‘₯
𝑛
π‘π‘œπ‘  π‘š π‘₯ cos 𝑛π‘₯
𝑛
−
−
π‘š
π‘π‘œπ‘  π‘š−1 π‘₯ sin(𝑛 −
∫
𝑛
1) π‘₯⁑𝑑π‘₯ [ since cos nx sin x = sin nx cos x – sin(n-1)x] =
-
π‘π‘œπ‘  π‘š π‘₯ cos 𝑛π‘₯
𝑛
−
π‘š
𝑛
Im,n+
π‘š
𝐼
𝑛 π‘š−1,𝑛−1
. Transposing and
simplifying, we get a reduction formula for Im,n.
10
Illustrative examples
πœ‹
2
1. 𝐼𝑛 = ∫0 π‘₯ 𝑛 sin π‘₯⁑𝑑π‘₯ and n>1, show that In+ n(n-1)In-2 =
πœ‹
n( )𝑛−1
2
πœ‹⁄
cos π‘₯ )|0 2
»β‘𝐼𝑛
=
(−π‘₯
n
𝑛−1
πœ‹⁄
sin π‘₯|0 2
[π‘₯
𝑛
+
πœ‹⁄
𝑛 ∫0 2 π‘₯ 𝑛−1 cos π‘₯⁑𝑑π‘₯
=
πœ‹⁄
− 1) ∫0 2 π‘₯ 𝑛−2 sin π‘₯⁑𝑑π‘₯ ]
− (𝑛
=
πœ‹
n( )𝑛−1 -n(n-1)𝐼𝑛−2 . Hence.
2
π‘₯ π‘š+1
2. Im,n = ∫ π‘₯ (1 − π‘₯) 𝑑π‘₯ =
π‘š
𝑛
𝑛−1
(1 − π‘₯ )](1 − π‘₯)
𝑑π‘₯ =
π‘š+1
π‘₯ π‘š+1
π‘š+1
(1 − π‘₯)𝑛 +
(1 − π‘₯)𝑛 +
𝑛
π‘₯ π‘š [1 −
∫
π‘š+1
𝑛
π‘š+1
( πΌπ‘š,𝑛−1 −
πΌπ‘š,𝑛 ). Hence Im,n can be obtained.
3. Im =
1
2
πœ‹⁄
∫0 2 π‘π‘œπ‘  π‘š π‘₯ sin π‘šπ‘₯⁑𝑑π‘₯.
πΌπ‘š−1 =
1
𝐼
.
22 π‘š−2
1
2π‘š
1
+ [
1
2 2(π‘š−1)
From 5 above, Im =
1
1
2
2π‘š
+ πΌπ‘š−2 ] =
+
1
2π‘š
1
22 (π‘š−1)
+
+
Repeating the use of the reduction formula, it
can be proved that Im =
1
2π‘š+1
[2 +
11
22
2
+
23
3
+β‹―+
2π‘š
π‘š
].
4. Get
a
reduction
formula
for
following:∫ π‘₯ π‘š (ln π‘₯)𝑛 𝑑π‘₯, ∫ 𝑒 −π‘₯ π‘₯ 𝑛 𝑑π‘₯,∫
each
sin 𝑛π‘₯
sin π‘₯
of
the
𝑑π‘₯.
CHAPTER 3: IMPROPER INTEGRAL
𝑏
When we consider the definite integral ∫π‘Ž 𝑓 (π‘₯ )𝑑π‘₯ in
earlier standards, we implicitly assume two conditions
to hold: (a) f is continuous on [a, b] or , to that matter, at
𝒃
least the limit ∫𝒂 𝒇(𝒙)𝒅𝒙 = ⁑ π₯𝐒𝐦 ∑π’πŸ 𝒇(𝒄𝒓 )πœΉπ’“ exists
𝒏→∞
independent of choice of points of subdivision xi and
that of ci, for all i and (b) the interval [a,b] is bounded.
𝑏
We want to extend the definition of ∫π‘Ž 𝑓(π‘₯ )𝑑π‘₯ when
either (a) or (b) or both are not met. This extended
definition of definite integral is referred to as
Improper Integrals. Improper integrals can be of
two types: (a) Type 1: interval of integration is
12
unbounded, (b) Type 2: integrand has a finite
number of infinite discontinuities in the interval of
integration.
Definition
of
∞
TYPE
I
𝒂
improper
∞
integral∫𝒂 𝒇(𝒙)𝒅𝒙,∫−∞ 𝒇(𝒙)𝒅𝒙 and ∫−∞ 𝒇(𝒙)𝒅𝒙
Let the function f be integrable in [a ,B], for every B>a.
𝐡
∞
If lim ∫π‘Ž 𝑓(π‘₯ )𝑑π‘₯ exist finitely, we define ∫π‘Ž 𝑓(π‘₯ )𝑑π‘₯ =
𝐡→∞
𝐡
lim ∫π‘Ž 𝑓(π‘₯ )𝑑π‘₯ and
𝐡→∞
we
∞
say ∫π‘Ž 𝑓(π‘₯ )𝑑π‘₯ exists
or
∞
converges; otherwise ∫π‘Ž 𝑓(π‘₯ )𝑑π‘₯ diverges. Similarly,
π‘Ž
∫−∞ 𝑓 (π‘₯ )𝑑π‘₯
π‘Ž
= lim ∫𝐡 𝑓 (π‘₯ )𝑑π‘₯ (provided
the
𝐡→−∞
∞
π‘Ž
limit
∞
exists) and ∫−∞ 𝑓(π‘₯ )𝑑π‘₯ = ⁑ ∫−∞ 𝑓 (π‘₯ )𝑑π‘₯ + ∫π‘Ž 𝑓(π‘₯ )𝑑π‘₯ , a
∞
π‘Ž
is any real, provided ∫π‘Ž 𝑓(π‘₯ )𝑑π‘₯ and ∫−∞ 𝑓 (π‘₯ )𝑑π‘₯ exist
separately.
13
∞ 𝑑π‘₯
Example 3.1 ∫1
π‘₯
∞ 𝑑π‘₯
2 ,⁑∫1
√π‘₯
. The range of integration of
π‘Ž 𝑑π‘₯
the integrals are unbounded. For a>1, ∫1
π‘Ž 𝑑π‘₯
and ∫1
π‘₯2
= 1-⁑⁑
1
β‘β‘π‘Ž
1
= 2(√π‘Ž-1). Since lim (1 − )= 1 exists but
π‘Ž
√π‘₯
π‘Ž→∞
lim (2(√π‘Ž − 1)) does not exist, hence the improper
π‘Ž→∞
integral
∞ 𝑑π‘₯
∫1
π‘₯2
converges
and
∞ 𝑑π‘₯
∫1
√π‘₯
diverges.(compare areas below the curves y = 1/x2
and y = 1/√π‘₯⁑ in diagram below)
Fig.2:Comparison of areas under y=1/x2 and y=1/√π‘₯ in (0,1] and [1,⁑∞)
Definition of TYPE II improper integral
14
Let f have an infinite discontinuity only at the point a
(that is, lim 𝑓 (π‘₯ ) = ±∞⁑ or ⁑lim 𝑓 (π‘₯ ) = ±∞) and is
π‘₯→π‘Ž+
π‘₯→π‘Ž−
𝑏
continuous in (a, b].Then we define ∫π‘Ž 𝑓(π‘₯ )𝑑π‘₯ =
𝑏
⁑ lim ∫π‘Ž+𝑐 𝑓 (π‘₯ )𝑑π‘₯,0<c<b-a, provided the limit exists.
𝑐→0+
Similarly, if f has an infinite discontinuity only at the
point b and is continuous in [a, b), then we define
𝑏
𝑏−𝑐
∫π‘Ž 𝑓 (π‘₯ )𝑑π‘₯ = ⁑ lim ∫π‘Ž
𝑐→0+
𝑓 (π‘₯ )𝑑π‘₯, 0<c<b-a, provided the
limit exists. If f has an infinite discontinuity at d, a<d<b,
and is otherwise continuous in [a,b], we define
𝑏
𝑑
𝑏
∫π‘Ž 𝑓 (π‘₯ )𝑑π‘₯ = ⁑ ∫π‘Ž 𝑓 (π‘₯ )𝑑π‘₯ + ∫𝑑 𝑓 (π‘₯ )𝑑π‘₯, provided both of
𝑑
𝑏
∫π‘Ž 𝑓(π‘₯ )𝑑π‘₯ and ∫𝑑 𝑓(π‘₯ )𝑑π‘₯ exist separately.
1 𝑑π‘₯
Example 3.2 ∫0
√π‘₯
1 𝑑π‘₯
,⁑∫0
π‘₯2
. The integrands have an
1⁑ 1
infinite discontinuity at x=0. For 0<a<1, ∫π‘Ž
1 𝑑π‘₯
2(1 − √π‘Ž) and ∫π‘Ž
π‘₯2
√π‘₯
𝑑π‘₯ =
1
= − 1. Since lim 2(1 − √π‘Ž) = 2
π‘Ž
π‘Ž→0+
1 𝑑π‘₯
1
exists but lim ( − 1) does not exist, so ∫0
π‘Ž
π‘Ž→0+
15
√π‘₯
1 𝑑π‘₯
converges whereas ∫0
π‘₯2
diverges. (Compare areas
between x = a,0<a<1, and x = 1, below the curves y =
1/x2 and y = 1/√π‘₯⁑ in diagram above)
∞
Example 3.3 ∫0
»β‘The integrand
𝑑π‘₯
4+9π‘₯ 2
1
=
πœ‹
12
is continuous everywhere but
4+9π‘₯ 2
the interval of integration is unbounded. Let a>o be
π‘Ž
fixed. ∫0
π‘Ž
lim ∫0
π‘Ž→∞
𝑑π‘₯
4+9π‘₯ 2
𝑑π‘₯
4+9π‘₯
π‘Ž
1
=
∫
9 0
𝑑π‘₯
2 2
π‘₯ 2 +( )
3
1 πœ‹
πœ‹
6 2
12
3
= .
2
2 = . =
Example 3.4 ∫0
𝑑π‘₯
√9−π‘₯
=
1
6
π‘‘π‘Žπ‘›−1
3π‘Ž
2
.
Thus
.
πœ‹
2
» The integrand has an infinite discontinuity at x = 3
π‘Ž
and is continuous on [0, 3). Let 0<a<3. Then ∫0
π‘Ž
sin-1(a/3) . So lim ∫0
π‘Ž→3−
3
Hence ∫0
𝑑π‘₯
√9−π‘₯
𝑑π‘₯
√9−π‘₯ 2
πœ‹
= .
2
2
16
𝑑π‘₯
√9−π‘₯ 2
π‘Ž
πœ‹
3
2
= lim 𝑠𝑖𝑛−1 ( ) =
π‘Ž→3−
=
.
Note : we can apply standard methods of integration,
in particular method of substitution, only to a proper
integral and not directly to an improper integral. Thus
if we substitute z=1/x directly in the improper
1 𝑑π‘₯
integral ∫−1
π‘₯2
, we get a value -2 of the integral
whereas it can be checked from definition that the
improper integral diverges.
PRACTICE SUM
∞
∞
2
Verify⁑that⁑(1) ∫−∞ π‘₯𝑒 −π‘₯ 𝑑π‘₯ = 0, (2) ∫0
𝑑π‘₯
(π‘₯ 2 +π‘Ž2 )(π‘₯ 2 +𝑏2 )
πœ‹
,
2π‘Žπ‘(π‘Ž+𝑏)
∞
(3) ∫0
π‘₯𝑑π‘₯
(π‘₯ 2 +π‘Ž2 )(π‘₯ 2 +𝑏2 )
∞
1
=
π‘Ž2 −𝑏
πœ‹
1
(4) ∫0 𝑒 −π‘₯ sin π‘₯⁑𝑑π‘₯ = , (5)∫0
2
TESTS
=
FOR
π‘Ž
2 𝑙𝑛 ( )
𝑑π‘₯
4+5⁑𝑠𝑖𝑛π‘₯
𝑏
(a,b>0),
2
= ln 2.
3
CONVERGENCE
IMPROPER INTEGRALS
TYPE I INTEGRAL
17
OF
Theorem 3.1 (Comparison test) Let f and g be
integrable in [a, B], for every B>a. Let g(x)>0, for all x
𝑓(π‘₯)
≥a. If lim
π‘₯→∞ 𝑔(π‘₯)
∞
= c≠0, then the integrals ∫π‘Ž 𝑓 (π‘₯ )𝑑π‘₯ and
∞
∫π‘Ž 𝑔(π‘₯ )𝑑π‘₯ either both converge or both diverge. If c =
0
∞
and ∫π‘Ž 𝑔(π‘₯ )𝑑π‘₯ converges
,
∞
then ∫π‘Ž 𝑓 (π‘₯ )𝑑π‘₯
converges.
Theorem 3.2 (π›β‘π“πžπ¬π­) Let f be integrable in [a, B], for
∞
every B>a. Then ∫π‘Ž 𝑓(π‘₯ )𝑑π‘₯ converges if lim π‘₯ πœ‡ 𝑓(π‘₯)
π‘₯→∞
∞
exists with πœ‡>1 and ∫π‘Ž 𝑓 (π‘₯ )𝑑π‘₯ diverges if lim π‘₯ πœ‡ 𝑓(π‘₯)
π‘₯→∞
exists and ≠0 with πœ‡ ≤ 1.
Example
3.5
∞ 𝑑π‘₯
∫0
converges
𝑒 π‘₯ +1
comparison test , since 0≤
lim
𝑒π‘₯
π‘₯→∞ 𝑒 π‘₯ +1
= lim
π‘₯→∞
∞ 𝑑π‘₯
1
= 1 and ∫0
1+𝑒 −π‘₯
to prove!).
18
𝑒π‘₯
1
𝑒π‘₯
by
for all x≥0,
converges (need
∞
Example 3.6 ∫1
1
dx
converges by μ⁑Test since
x√1+x2
2
[
]
is⁑integrable⁑in⁑
1,
B
,
for⁑B
>
1,
lim
π‘₯
{
2
x√1+x
π‘₯→∞
1, πœ‡ = 2>1. Note that
1
π‘₯√1+π‘₯ 2
1
π‘₯√1+π‘₯ 2
}=
is continuous and hence
integrable in [1, B]for B>1.
Example
∞
2
3.7 ∫0 e−x dx converges
2 −π‘₯ 2
since⁑⁑lim( π‘₯ 𝑒
π‘₯→∞
by π›β‘π“πžπ¬π­
) = 0 (verify using L’Hospital’s rule)
2
,β‘πœ‡ = 2>1 and e−x is continuous, and hence integrable,
in [0,B] for B>0.
Example
3.8
3
1⁄
π‘₯ ⁄2
2
lim ( π‘₯ ( 2 ))
3π‘₯ +5
π‘₯→∞
3
∞ x ⁄2
∫0 3x2 +5 dx
diverges,
= 1/3, πœ‡ = ½<1 and
since
3
x ⁄2
3x2 +5
continuous, and hence integrable, in [0,B] for B>0.
TYPE II INTEGRAL
19
is
Theorem 3.3 (Comparison test) Let f and g be
integrable in [c, b], for every c, a<c<b. Let g(x)>0 , for
all x, a<x≤b. If lim
π‘₯→π‘Ž+
𝑏
𝑓(π‘₯)
≠0, then ∫π‘Ž 𝑓(π‘₯ )𝑑π‘₯ and
𝑔(π‘₯)
𝑏
∫π‘Ž 𝑔(π‘₯ )𝑑π‘₯ both converge or both diverge. If lim
𝑓(π‘₯)
π‘₯→π‘Ž+ 𝑔(π‘₯)
𝑏
=
𝑏
0 and ∫π‘Ž 𝑔(π‘₯ )𝑑π‘₯converges, then ∫π‘Ž 𝑓(π‘₯ )𝑑π‘₯ converges.
Theorem 3.4 (π›β‘π“πžπ¬π­) Let f be integrable in[c, b], for
every
c,
a<c<b.
𝑏
Then ∫π‘Ž 𝑓(π‘₯ )𝑑π‘₯ converges
if
𝑏
lim (π‘₯ − π‘Ž)πœ‡ f(x) exists for 0 < πœ‡ < 1 and ∫π‘Ž 𝑓(π‘₯ )𝑑π‘₯
π‘₯→π‘Ž+
diverges if lim (π‘₯ − π‘Ž)πœ‡ f(x) exists (≠0) for πœ‡≥1.
π‘₯→π‘Ž+
1
Example 3.9 ∫0
1
2
0)
1
(1+π‘₯)√π‘₯
dx
(1+x)√x
converges , since lim (π‘₯ −
π‘₯→0+
= 1, for πœ‡<1 and
1
(1+x)√x
is continuous, and
hence integrable, in [c,1]for 0<c<1.
Example
1⁄
2
lim (1 − π‘₯)
π‘₯→1−
1
dx
∫1⁄ x(1−x)
2√
3.10
1
√π‘₯(1−π‘₯)
converges,
1
1
2
√x(1−x)
= 1, for πœ‡ = < 1 and
20
since
is
continuous, and hence integrable, in [1/2, c]for
1/2<c<1.
THE GAMMA AND BETA FUNCTIONS
Definition (Gamma function) For n>0, 𝛀 (n) =
∞ −π‘₯ 𝑛−1
𝑑π‘₯.
∫0 𝑒 π‘₯
NOTE: Gamma function is an improper integral of type
I. If 0<n<1, 𝛀(n) is also an improper integral of type II.
We shall assume convergence of the gamma function
in our course of study.
Definition (Beta function) For m, n>0,⁑⁑𝛽(m,n) =
1 π‘š−1
(1
∫0 π‘₯
− π‘₯)𝑛−1 ⁑𝑑π‘₯
21
NOTE: Beta function is an improper integral of type II
if either m or n or both lies between 0 and 1 strictly;
otherwise it is a proper integral.
Properties of Gamma and Beta functions
∞
1. For any a>0, ∫0 𝑒 −π‘Žπ‘₯ π‘₯ 𝑛−1 𝑑π‘₯ = 𝛀(n)/an.
» let 0<c<d. consider the proper integral I =
𝑑
∫𝑐 𝑒 −π‘Žπ‘₯ π‘₯ 𝑛−1 𝑑π‘₯ .
1
Let y = ax. Then I =
π‘Žπ‘‘
−𝑦 𝑛−1
𝑒
𝑦
𝑑𝑦. Thus lim I =
∫
𝑛
π‘Ž π‘Žπ‘
π‘Žπ‘‘
∫π‘Žπ‘ 𝑒 −𝑦
𝛀(n)
π‘Žπ‘›
𝑦 𝑛−1 1
. 𝑑𝑦 =
π‘Žπ‘›−1 π‘Ž
as 𝑐 → 0 + and d→
∞.
2. 𝛀(n+1) = n⁑𝛀(n)
» Let 0<c<d. using integration by parts on the proper
integral I =
𝑑 −π‘₯ 𝑛
∫𝑐 𝑒 π‘₯ 𝑑π‘₯ ,
𝑑
𝑛 ∫𝑐 𝑒 −π‘₯ π‘₯ 𝑛−1 𝑑π‘₯
= (
𝑐𝑛
𝑑𝑛
𝑒
𝑒
𝑐 −
we get I = (−
π‘₯𝑛
𝑒
𝑑
)
|
𝑐 +
π‘₯
𝑑
−π‘₯ 𝑛−1
π‘₯
𝑑π‘₯ , which
𝑑 )+⁑𝑛 ∫𝑐 𝑒
tends to n⁑𝛀 (n) as c→ 0+ and d→ ∞ (by use of
L’Hospital’s rule). Hence the result.
3
𝛀(1) = 1 (can be verified easily)
22
4⁑⁑⁑⁑⁑𝛀(n+1) = n!, for a natural n (follows from property
2 and 3)
4 𝛽(m,n) = 𝛽(n,m) (follows using a substitution y = 1-x
after passing to a proper integral)
5 𝛽(m,n)
πœ‹⁄
=2∫0 2 𝑠𝑖𝑛2π‘š−1 πœƒβ‘π‘π‘œπ‘  2𝑛−1 πœƒβ‘π‘‘πœƒβ‘(follows
using a
substitution x = sin2 πœƒ after passing to a proper
integral)
11
6 𝛽( , )=πœ‹ (follows from definition)
22
7 𝛽(π‘š, 𝑛) = ⁑
𝛀(π‘š)𝛀(𝑛)
𝛀(π‘š+𝑛)
1
8 𝛀 ( ) = √πœ‹
2
9 For 0<m<1, 𝛀(m) 𝛀(1-m) =β‘πœ‹ cosec(mβ‘πœ‹)
∞
2
Example 3.11 ∫0 e−x dx = ⁑
√π
.
2
» The range of integration of the given integral is
unbounded
but
the
everywhere. For 0<a,
integrand
2
π‘Ž
∫0 e−x dx
23
is
=
continuous
π‘Ž2 −1 −𝑦
∫ 𝑦 2 𝑒 𝑑𝑦
2 0
1
(substituting y = x2 in the proper integral ). Thus
2
π‘Ž
lim ∫0 e−x dx
π‘Ž→∞
1
1
2
2
π‘Ž2 −1 −𝑦
1 ∞ −𝑦 1−1
lim ∫ 𝑦 2 𝑒 𝑑𝑦 = ∫0 𝑒 𝑦 2 𝑑𝑦
2 π‘Ž→∞ 0
2
1
=
= ⁑𝛀 ( ) = √πœ‹/2.
1
Example 3.12 ∫0
dx
1
6
(1−x )6
dx.
» The integrand has an infinite discontinuity at x =
1.Let 0<c<1. Substituting x3 = sinβ‘πœƒ in the proper
integral
𝑐
𝑑π‘₯
∫0
1
(1−π‘₯ 6 ) ⁄6
𝑐
𝑑π‘₯
∫0
1
(1−π‘₯ 6 ) ⁄6
,
5⁄ −1
1⁄ −1
𝑠𝑖𝑛−1 𝑐 3
3
3 πœƒβ‘π‘‘πœƒ
π‘π‘œπ‘ 
β‘πœƒβ‘π‘ π‘–π‘›
∫
3 0
1
𝑐
𝑑π‘₯
lim ∫0
1
𝑐→1−
(1−π‘₯ 6 ) ⁄6
1
9
5
1
= ⁑𝛽(5/3,1/3) =
6
1
1
3
3
27
6 𝛀(5+1)
π
πœ‹π‘π‘œπ‘ π‘’π‘( ).
3
PRACTICE SUMS
πœ‹⁄
1. ∫0 2 √tan π‘₯ 𝑑π‘₯
1
=
πœ‹
1
1 𝛀(3)𝛀(3)
3 3
1
⁑𝛀 ( ) 𝛀 (1 − ) =
.
.
√2
1
π‘š
2
2
2. ∫0 π‘₯ π‘š−1 (1 − π‘₯ 2 )𝑛−1 𝑑π‘₯ = ⁑ ⁑𝛽 ( , 𝑛)
24
=
Since
2
1
1 2 𝛀(3)𝛀(3
= .
63
1
=
1
3. ∫0 √1 − π‘₯ 4 𝑑π‘₯ = ⁑
1
4
[𝛀( )]
2
6√2πœ‹
CHAPTER 4: DOUBLE INTEGRAL
Fig. 3:Volume enclosed by the surface z=f(x,y) is
approximated by volume of parallelopipeds
Integrals over rectangles
Let f(x,y) be a bounded function of two independent
variables x and y defined over a closed rectangular
region R: a≤x≤b; c≤y≤d. we take partitions {a =
x0,x1,…,xr-1,xr,…,xn = b} of [a,b] and {c = y0,y1,…,ys1,ys,…,ym
= d}. These partitions divides the rectangle R
25
into mn number of subrectangles Rij(1≤i≤n, 1≤j≤m).
Let us choose arbitrarily ( 𝛼𝑖 , 𝛽𝑗 ) ∈ Rij⁑where⁑ 𝛼𝑖 ∈
[π‘₯𝑖−1 , π‘₯𝑖 ] and 𝛽𝑗 ∈ [𝑦𝑗−1 , 𝑦𝑗 ], 1≤i≤n, 1≤j≤m. the volume
of the parallelepiped with base Rij and altitude f(𝛼𝑖 , 𝛽𝑗 )
is f(𝛼𝑖 , 𝛽𝑗 )(xi-xi-1)(yj-yj-1). ∑𝑖,𝑗 𝑓(𝛼𝑖 , 𝛽𝑗 )(π‘₯𝑖 − π‘₯𝑖−1 )(𝑦𝑗 −
𝑦𝑗−1 ), sum of the volumes of all the parallelepipeds
erected over all of the Rij’s, gives an approximation of
the volume enclosed by the curve and the planes x =
a,x = b, y = c, y = d and z = 0. The approximation can be
improved by increasing number of subrectangles into
which
lim
π‘š→∞,𝑛→∞
R
is
divided
into.
Thus
the
limit
∑𝑖,𝑗 𝑓(𝛼𝑖 , 𝛽𝑗 )(π‘₯𝑖 − π‘₯𝑖−1 )(𝑦𝑗 − 𝑦𝑗−1 ), provided
it exists, gives the volume and is represented by
βˆ¬π‘… 𝑓(π‘₯, 𝑦)𝑑π‘₯𝑑𝑦.
NOTE: Every continuous function is integrable over
any rectangle.
26
Theorem4.1 (equivalence of double integrals with
repeated integrals) If βˆ¬π‘… 𝑓(π‘₯, 𝑦)𝑑π‘₯𝑑𝑦 exists over a
𝑏
rectangle R: a≤x≤b; c≤y≤d and ∫π‘Ž 𝑓(π‘₯, 𝑦)𝑑π‘₯ exists for
each value of y in [c,d], then the repeated integral
𝑑
𝑏
∫𝑐 𝑑𝑦 ∫π‘Ž 𝑓 (π‘₯, 𝑦)𝑑π‘₯ ⁑
exists
and
is
equal
to
βˆ¬π‘… 𝑓(π‘₯, 𝑦)𝑑π‘₯𝑑𝑦.
Example
4.1
πœ‹
πœ‹
2
2
Evaluate βˆ¬π‘… 𝑠𝑖𝑛(π‘₯ + 𝑦)𝑑π‘₯⁑𝑑𝑦 over
R:0≤x≤ , 0≤y≤ .
# sin(x+y) is continuous on R, so the double
integralβ‘βˆ¬π‘… 𝑠𝑖𝑛(π‘₯ + 𝑦)𝑑π‘₯⁑𝑑𝑦⁑⁑exists . Evaluating given
double integral in terms of repeated integrals,
βˆ¬π‘… 𝑠𝑖𝑛(π‘₯ + 𝑦)𝑑π‘₯⁑𝑑𝑦 =
πœ‹⁄
∫0 2[−cos⁑(π‘₯
πœ‹
2
πœ‹⁄
πœ‹⁄
2 𝑑π‘₯
∫0
∫0 2 sin(π‘₯
πœ‹
2
+ 𝑦)𝑑𝑦 =
+ 𝑦)|0 𝑑π‘₯ = ⁑ ∫0 (cos π‘₯ + sin π‘₯)⁑𝑑π‘₯= 2.
27
Example 4.2 Evaluate βˆ¬π‘… (π‘₯ 2 + 𝑦 2 )𝑑π‘₯⁑𝑑𝑦 over R
bounded by y = x2, x = 2, y = 1.
Fig.4:Fixing up of range of integration of independent
variables x and y
2
2)
# βˆ¬π‘… (π‘₯ + 𝑦 𝑑π‘₯⁑𝑑𝑦
2
∫1 [π‘₯ 2 𝑦
+
𝑦3
π‘₯2
]
3 1
𝑑π‘₯ =
2
π‘₯2 2
∫1 𝑑π‘₯ ∫1 (π‘₯
=
2 π‘₯6
∫1 ( 3
=
+ 𝑦 2 )𝑑𝑦
1
1006
3
105
+ π‘₯ 4 − π‘₯ 2 − ) 𝑑π‘₯ =
.
Example 4.3 Prove that βˆ¬π‘… π‘₯𝑦(π‘₯ + 𝑦)𝑑π‘₯⁑𝑑𝑦 =
,where R is the region bounded by y = x and y = x2.
CHAPTER 5: EVALUATION OF AREA
28
5
36
Cartesian co-ordinate
It has already been seen that area of the region
bounded by the curve y = f(x), lines x = a, x = b and y =
𝑏
0 is given by ∫π‘Ž 𝑓(π‘₯)𝑑π‘₯, provided it exists. Similarly
area of the region bounded by the curve x = g(y), lines
𝑑
y = c, y = d and x = 0 is given by ∫𝑐 𝑔(𝑦)𝑑𝑦, provided it
𝑑
exists. We can define F:[a,b]→ R by F(t)=∫π‘Ž 𝑓 (π‘₯ )𝑑π‘₯
,a≤t≤b.
Observe that for the function f[-2,2]→ 𝑅⁑⁑, 𝑓 (π‘₯ ) = π‘₯ 2 −
π‘₯ + 3⁑, 𝐹: [−2,2] →
𝑅⁑can⁑be⁑depicted⁑as⁑⁑⁑..\Document
s\30.gif.
29
Fig.5: Sign convention of area calculation and area
bounded by two curves
Example 5.1 find the area of the bounded region
bounded by the curve y = x(x-1)(x-2) and the xaxis...\Documents\31.gif
# y value is positive for 0<x<1 and for x>2 and is
negative for 1<x<2; the curve cuts the x-axis at points
whose
abscissa
are
0,1,2.
Required
area
=
1
2
𝑦⁑𝑑π‘₯
+|
∫0
∫1 𝑦⁑𝑑π‘₯ |.
Example 5.2 ..\Documents\x5.mw
Example 5.2 Find the area of the bounded region
bounded by the curves y = x2 and x = y2.
# On solving the given equations of the curves, the
point of intersection of the two curves are (0,0) and
(4,4). Thus required area =
4
∫0 √4π‘₯𝑑π‘₯
30
4 π‘₯2
− ⁑ ∫0 𝑑π‘₯ .
4
Example 5.3 Find the area of the loop formed by the
curve y2 = x(x-2)2
# The abscissa of points of intersection of the curve
with the x-axis are given by y = 0, that is, x = 0,2,2. For
x<0, no real value of y satisfy the equation. Hence no
part of the curve exist corresponding to x<0.
Corresponding to each x-value satisfying 0<x<2, there
exist two values of y, equal in magnitude and opposite
in sign. Thus between x = 0 and x = 2, the curve is
symmetric about the x-axis and a loop is formed
thereby. For x>2, y→ ∞ as x→ ∞. the required area =
2
2∫0 (π‘₯ − 2)√π‘₯𝑑π‘₯ (by symmetry of the curve about xaxis).
Example 5.4 Prove that area included in a circle of
radius r unit is πœ‹r2 square unit.
# We can choose two perpendicular straight lines
passing through the centre of the circle as co-ordinate
31
axes. With reference to such a co-ordinate system,
equation of the circle is y = ±√π‘Ÿ 2 − π‘₯ 2 .Curve is
symmetric about the axes .Thus required area =
π‘Ÿ
4∫0 √π‘Ÿ 2 − π‘₯ 2 ⁑dx.
Polar co-ordinate
Fig.6:Area under a polar curve and that under a
cardioide
The area of the region bounded by the curve r = f(πœƒ) ,
1
𝛽
the radius vector πœƒ = 𝛼,πœƒ = 𝛽 is given by ∫𝛼 π‘Ÿ 2 π‘‘πœƒ.
2
Example 5.5 Find the area enclosed by the cardioide r
= a(1+ cosβ‘πœƒ)
32
πœ‹
# As πœƒβ‘varies from 0 to , r decreases continuously
2
πœ‹
from 2a to a. When πœƒβ‘further increases from to πœ‹, r
2
decreases further from a to 0. Also the curve is
symmetric about the initial line (since the equation of
the curve remains unaffected on replacing πœƒ by –β‘πœƒ).
Hence the area enclosed by the curve = 2.
π‘Ž2
πœ‹
∫ (1
2 0
+
π‘π‘œπ‘ πœƒ)2 π‘‘πœƒ.
Fig.7:Area between two cardioides
Example 5.6 Find the area enclosed by the cardioide r
= a(1+ cosβ‘πœƒ) and r = a(1- cosβ‘πœƒ)
# The vectorial angle corresponding the points of
πœ‹
πœ‹
2
2
intersection of the curves are πœƒ = and πœƒ=- . Because
of the symmetry of the curves about the initial
33
line, β‘πœƒ =
πœ‹
2
πœ‹⁄
4. ∫0 2(1
2
π‘Ž2
, β‘πœƒ =-
πœ‹
2
and πœƒ = β‘πœ‹ , required area is
− cos πœƒ)2 π‘‘πœƒ.
Notation: For the rest of our discussion ,
suffix of dependent variable or of a
function
denotes
order
of
differentiation.
CHAPTER 6: LENGTH OF ARC OF A PLANE CURVE
The length of the arc of a curve y = f(x) between two
points whose abscissae are a and b, when f1 (x) is
continuous on the interval [a,b] is given by
𝑏
∫π‘Ž √1 + {𝑓12 (π‘₯)}𝑑π‘₯ . We can define the arc length
function s:[a,b]→ R by
34
𝑑
s(t)=∫π‘Ž √1 + {𝑓12 (π‘₯)}dx ,a≤t≤b. ..\Documents\x6.mw .
Example 6.1 Find the length of circumference of a
circle of radius 5 units.
# With suitable choice of co-ordinates, equation of the
curve is x2+y2 = 25. Here 1+y12 = 25/(25-x2). Required
5
length = 4∫0
5
√25−π‘₯ 2
= 10πœ‹.
Example 6.2 Find the length of the arc of the parabola
y2 = 16 x measured from the vertex to an extremity of
the latus rectum.
Example 6.3 Let f(x)=x3+1,x∈[-2,2].In adjoining figure,
f is plotted in red, integrand in blue and the arc
35
function
π‘₯
s(x)= ⁑∫−2 √1 + {𝑓12 (𝑑)}𝑑𝑑 ,
x ∈ [-2,2],
in
green...\Documents\32.gif
Example 6.3 Find the length of the loop of the curve
3y2 = x(x-1)2.
The length of an arc of the curve r = f(πœƒ) between
points whose vectorial angles are πœƒ = ⁑𝛼 and πœƒ = 𝛽 is
given by
𝛽
∫𝛼 √π‘Ÿ 2
π‘‘π‘Ÿ 2
+ ( ) π‘‘πœƒ.
π‘‘πœƒ
Example 6.4 Find the length of the perimeter of the
cardioide r = a(1+cosπœƒ)
# As we can see from fig.7 above, using symmetry of
the curve about the initial line (justified by the
invariance of the equation on replacing πœƒ by –πœƒ), the
required
length
πœ‹⁄
[∫0 2 √π‘Ž2 (1
2x
πœ‹
− π‘π‘œπ‘ πœƒ)2 + π‘Ž2 𝑠𝑖𝑛2 πœƒ π‘‘πœƒ +
∫πœ‹⁄ √π‘Ž2 (1 − π‘π‘œπ‘ πœƒ)2 + π‘Ž2 𝑠𝑖𝑛2 πœƒ π‘‘πœƒ].
2
36
is
CHAPTER 7: SURFACE AREA AND VOLUME OF
SURFACE OF REVOLUTION
The volume generated by revolving about the x-axis an
area bounded by the curve y = f(x), the x-axis and two
ordinates x = a and x = b is given by 𝑉 =
𝑏
β‘πœ‹ ∫π‘Ž {𝑓(π‘₯)}2 𝑑π‘₯. Similarly, The volume generated by
revolving about the y-axis an area bounded by the
curve x = g(y), the y-axis and two ordinates y = c and y
𝑑
= d is given by 𝑉 = β‘πœ‹ ∫𝑐 {𝑔(𝑦)}2 𝑑𝑦. The formula for
surface area of the surface generated is given by S=
𝑏
𝑑
2πœ‹ ∫π‘Ž 𝑦√1 + 𝑦12 𝑑π‘₯ and 2πœ‹ ∫𝑐 π‘₯√1 + π‘₯12 𝑑𝑦.
37
Example 7.1 Find the volume and surface area of a
right circular cylinder of base radius r and altitude h.
Fig.8:Volume and surface area of surface of revolution
# A right circular cylinder of radius r and altitude h is
obtained by revolving y = r,z = 0 about the x-axis. Thus
β„Ž
volume = πœ‹ ∫π‘œ π‘Ÿ 2 𝑑π‘₯ = πœ‹ r2h and surface area =
β„Ž
2πœ‹ ∫0 π‘Ÿ√1 + 02 𝑑π‘₯ = 2πœ‹rh.
Example 7.2 Find the volume and surface area of a
sphere of radius r.
# A sphere of radius r is obtained by revolving
π‘Ÿ
y=√π‘Ÿ 2 − π‘₯ 2 ,-r≤x≤r, about x-axis. Thus V=β‘πœ‹ ∫−π‘Ÿ(π‘Ÿ 2 −
π‘Ÿ
π‘₯ 2 )𝑑π‘₯ and S=2πœ‹ ∫−π‘Ÿ √π‘Ÿ 2 − π‘₯ 2 ⁑
38
π‘Ÿ
√π‘Ÿ 2 −π‘₯ 2
dx=4β‘πœ‹r2.
Example 7.3 Surface area of the surface generated by
y=cos (x3) between x=0, x=2 for rotation about x-axis
and y-axis(frustum view)...\Documents\33.gif
Example 7.4 Surface area of the surface generated by
revolving y=cos x between x=0 and x=2 around x-axis:
..\Documents\x3.mw
Example 7.5 Surface area of the surface generated by
revolving y=1+ cos x between x=0 and x=2 around xaxis:..\Documents\x4.mw
SECTION II (ORDINARY DIFFERENTIAL
EQUATIONS)
NOTE: suffix denotes order of differentiation
39
TEXT : (1) Differential equations and their
applications—Zafar
Ahsan
(2)
Differential
Equations—Richard
Bronson (Schaum)
CHAPTER 1: ORDER,DEGREE AND FORMATION OF
ORDINARYDIFFERENTIAL EQUATION
Definition 1.1 An ordinary differential equation(ODE)
is an equation involving derivative(s) or differentials
w.r.t. a single independent variable.
Example: y2=a2y, 3x3y3+4x2y1 = 7x2+9, x dy – ydx+2xy
dy = 0.
Definition 1.2 the order of an ODE is the order of the
heighest ordered derivative occurring in the equation.
40
The degree of an ODE is the largest power of the
heighest ordered derivative occurring in the equation
after the ODE has been made free from the radicals
and fractions as far as the derivatives are concerned.
Example: y = x
𝑑𝑦
𝑑π‘₯
+
𝑑π‘₯
𝑑𝑦
: first order, second degree
(1+y12)3/2 = y1: first order, sixth degree.
Definition 1.3 An ODE in which the dependant
variables and all its derivatives present occur in first
degree only and no products od dependent variables
and /or derivatives occur is known as a linear ODE. An
ODE which is not linear is called nonlinear ODE. Thus
y1 = sin x+cos x is linear while y = y1+1/y1 is nonlinear.
Definition 1.4 A solution of an ODE is a relation
between the dependent and independent variables,
not involving the derivatives such that this relation
and the derivatives obtained from it satisfies the given
41
ODE. For example, y = ce2x is a solution of the ODE y1 =
2y, since y1 = 2ce2x and y = ce2x satisfy the given ODE.
Some of the solutions of the DE y2=x2-x+1 are depicted
as follows: ..\Documents\x1.mw . Some of the
solutions y=c cos x+d sin x (c varying between -20 to
10, d between -10 to 20) of y2+y=0 are shown here:
..\Documents\x2.mw
FORMATION OF ODE
GEOMETRIC PROBLEMS
Example 1.1: Let a curve under Cartesian coordinate
system satisfy the condition that the sum of x- and yintercepts of its tangents is always equal to a. Find the
ODE corresponding to the curve.
# Equation of tangent at any point (x,y) on the curve is
Y-y =
𝑑𝑦
𝑑π‘₯
(X-x). Thus the differential equation
expressing the given condition is (x-yx1)+(y – xy1) = a.
PHYSICAL PROBLEMS
42
Example 1.2: Five hundred grammes of sugar in water
are being converted into dextrose at a rate which is
proportional to the amount unconverted. Form an ODE
expressing the rate of conversion after t minutes.
# Let y denote the number of grammes converted in t
minutes. Then the ODE is
𝑑𝑦
= k(500 – y), k constant.
𝑑𝑑
Example 1.3 A person places Rs.20,000 in a savings
account
which
pays
5%
interest
per
annum,
compounded continuously. Let N(t) denotes the
balance in the account at any time t. N(t) grows by the
accumulated
interest
payments,
which
are
proportional to the amount of money in the account.
The resulting ODE is
𝑑𝑁
𝑑𝑑
=0.05 N.
Example 1.4 Five mice in a stable population of 500
are intentionally infected with a contagious disease to
test a theory of epidemic spread that postulates the
rate of change in the infected population is
43
proportional to the product of the number of mice who
have the disease with the number that are disease free.
Let N(t) denote the number of mice with the disease at
time t. resulting ODE is
𝑑𝑁
𝑑𝑑
= kN(500-N).
Example 1.5 Newton’s law of cooling states that the
time rate of change of the temperature of a body is
proportional to the temperature difference between
the body and the surrounding medium. Let T denote
the temperature of the body and let Tm denote the
temperature of the surrounding medium. Resulting
ODE is
𝑑𝑇
𝑑𝑑
= -k(T-Tm).
ELIMINATION OF ARBITRARY CONSTANTS
Suppose we are given an equation(not a differential
equation)
containing
constants).by
n
differentiating
44
parameters
the
given
(arbitrary
equation
successively n times , we get n equations more
containing
n
parameters
eliminating n parameters
and
derivatives.
By
from the above (n+1)
equations and obtaining an equation which involves
derivatives upto the n th order, we get an ODE of
order n.
Example
1.6:
Obtain
an
ODE
by
eliminating
parameters a,b from (x-a)2+(y-b)2 = c2, c constant.
(x-a)+(y-b)y1 = 0, 1+y12+(y-b)y2 = 0. Obtain values of
x-a and y-b in the given equation, obtain the ODE.
Example 1.7: Find the ODE corresponding to the
family of curves y = c(x-c)2 (2.1), where c is a
parameter.
Y1 = 2c(x-c) . so y12 = 4c2(x-c)2 (2.2). from (2.1) and
(2.2), c = y12/(4y). Substituting in (2.1), required
equation is 8y2 = 4xyy1-y12.
45
Example 1.8: Obtain the ODE corresponding to the
family of all circles each of which touches the axis of x
at the origin.
# The equation of an arbitrary circle of the family is of
the form (x-r)2+y2 = r2, that is , x2+y2 – 2rx = 0, r is a
parameter. Obtain the ODE by eliminating the
parameter r.
GENERAL,
PARTICULAR
AND
SINGULAR
SOLUTIONS
A solution which contains a number of independent
parameters equal to the order of the ODE is called the
general solution or complete integral of the ODE. A
solution obtained from the general solution by putting
particular values to at least one of the parameters
present in the general solution is called a particular
solution. A solution which is neither the general
46
solution nor is a particular solution of an ODE is called
a singular solution of the ODE.
NOTE (1) In counting the parameters in the general
solution, we must check whether they are independent
and
are not equivalent to a lesser number of
parameters. Thus a solution of the form c1 cosx+c2
sin(x+c3) appears to have three parameters but
actually they are equivalent to two; for, c1 cosx+c2
sin(x+c3) = (c1+c2 sin c3) cos x+c2 cos c3 sinx = A cos x
+B sin x.
(2) The general solution of an ODE may have more
than one form, but parameters in one form will be
related to parameters in another form. Thus y = c1
cos(x+c2)and y = c3 sin x+c4 sin x are both solutions of
y2+y = 0. Here c4 = c1 cos c2,c3 = -c1 sin c2.
47
Example 1.9 y = ln x is a solution of xy2+y1 = 0 on
(0,∞) but is not a solution on (-∞,∞) since ln x is not
defined on (-∞,0].
EXERCISES
1. Find the ODE of the family of circles whose centres are
on the y-axis and touch the x-axis.
2. Find the ODE of the family of parabolas whose axes are
parallel to the y-axis.
3. A canonical tank of height 20 cm. loses water out of an
orifice at its bottom. If the cross-sectional area of the
orifice is ¼ cm2, obtain the ODE representing the
height h of water at any time t.
48
CHAPTER 2: ODE OF FIRST ORDER AND FIRST
DEGREE
An ODE of the first order and first degree is of the form
y1 = f(x,y) which is sometimes conveniently written as
M(x,y) dx+N(x,y) dy = 0 (2.1), where M(x,y) and N(x,y)
are
either
functions
of
x,y
possessing
partial
derivatives or constants.
NOTE: First order first degree ODE whose variables
are separable or which are homogeneous or which are
reducible to homogeneous equations have been
studied earlier and will not be repeated here. Students
are advised to revise the same.
Exact equations
Definition 2.1 An ODE of the form (2.1) is called exact
if and only if there exists a function f(x,y) with
continuous partial derivatives such that (2.1) can be
written in the form df(x,y) = 0, that is, in the form fx
49
dx+fy dy = 0. In this case, f(x,y) = c will be the general
solution of given ODE.
For example, xdx+ydy = 0 is exact since the given
equation can be written in the form d(x2+y2) = 0.
Theorem2.1 (2.1) is exact iff My = Nx holds.
Example 2.1 Verify whether the differential equation
(sin x cos y+e2x) dx+(cos x sin y+tan y)dy = 0 is exact.
Also find the general solution of the equation.
# Comparing with the form Mdx+Ndy = 0, M = sin x cos
y+e2x, N = cos x sin y+tan y. so My=- sin x siny = Nx.
hence given equation is exact. Let f(x,y) = 0 be the
solution. Given equation will be identical with
fxdx+fydy = 0. Comparing, fx = sin x cosy+e2x(2.2), fy =
cos x sin y+tan y(2.3).From (2.2), f(x,y) = - cos x cos
y+1/2 e2x+g(y), where g(y) is the integration constant.
Substituting in (2.3), cos x sin y+ g1(y) = fy = cosx sin y+
tan y. Thus g1(y) = tan y so that g(y) = ln sec y. Hence
50
the general solution is f(x,y) = - cos x cos y+1/2 e2x+ln
sec y = c, c parameter.
Integrating factors
In theory, a non-exact ODE can always be made exact
by multiplying the equation by some function πœ‡(x,y) of
x and y. such a function πœ‡(x,y) is called an Integrating
factor (I.F.) of the ODE. Although there is always an
I.F. for a non-exact ODE, there is no general method of
finding the I.F. we shall now discuss methods of finding
I.F. in some particular cases .
Method 1 (by inspection) use is made of exact
differentials like
𝑦
π‘₯𝑑𝑦−𝑦𝑑π‘₯
π‘₯
π‘₯2
𝑑( ) =
π‘₯⁑𝑑𝑦−𝑦⁑𝑑π‘₯
π‘₯𝑦
𝑦
, d(xy) = x dy+y dx ,d (𝑙𝑛 ( )) =
π‘₯
𝑦
π‘₯⁑𝑑𝑦−𝑦⁑𝑑π‘₯
π‘₯
π‘₯ 2 +𝑦 2
⁑⁑, d(π‘‘π‘Žπ‘›−1 ) =
⁑.
Example 2.2: (1+xy)y dx+(1-xy)x dy = 0.
51
# d(xy)+ xy(y dx-x dy) = 0 . thus
So 𝑑 [−
1
π‘₯𝑦
𝑦
− 𝑙𝑛 ( )] =
π‘₯
0.
𝑑(π‘₯𝑦)
(π‘₯𝑦)2
General
−
π‘₯⁑𝑑𝑦−𝑦⁑𝑑π‘₯
π‘₯𝑦
solution
= 0.
is
1/(xy)+ln(y/x) = c, c parameter.
Example 2.3: x dy-y dx = a(x2+y2)dy
d(tan-1(y/x)) = a dy.
Method 2 if the ODE Mdx+Ndy = 0 is homogeneous
and Mx+Ny≠0, then 1/(Mx+Ny) is an IF.
Example 2.4: x2y dx – (x3+y3)dy = 0
# Here Mx+Ny = -y4≠0 and the given equation is
homogeneous. Thus an IF is -1/y4.
Method 3 if M = y f(xy), N =x g(xy), then 1/(Mx-Ny) is
an IF of the ODE Mdx+Ndy = 0.
Example 2.5: (xy+2x2y2) y dx+(xy – x2y2) x dy = 0.
# Here M = y[(xy)+2(xy)2] and N = x[(xy)- (xy)2]. Thus
an IF = 1/[Mx-Ny] = 1/(3x3y3).
52
Method 4 e∫ f(x)dx is an IF of Mdx+Ndy =0,if
𝑀𝑦 −𝑁π‘₯
𝑁
is a
function of x.
Example 2.6: (x2+y2)dx – 2xy dy = 0
# M = x2+y2, N = -2xy,
𝑀𝑦 −𝑁π‘₯
𝑁
=-2/x. Thus an IF =
e∫ f(x)dx =e-2 ln x = x-2.
Example 2.7 (a very useful form of ODE: linear
equation in y) y1+P(x) y = f(x), P(x), f(x) are functions
of x alone or constants. M = P(x)y-f(x), N = 1.
𝑀𝑦 −𝑁π‘₯
Thus
𝑁
Method 5
= P(x). An IF = 𝑒 ∫ 𝑃(π‘₯)𝑑π‘₯ .
e∫ f(y)dy
is an IF of Mdx+Ndy =0,if
a function of y.
Example 2.8 (xy3+y) dx+2(x2y2+x+y4) dy = 0
#⁑
𝑁π‘₯ −𝑀𝑦
𝑀
=1/y. hence an IF = 𝑒
53
1
∫𝑦𝑑𝑦
=y.
𝑁π‘₯ −𝑀𝑦
𝑀
is
Method 6 if the equation Mdx +Ndy = 0 is of the form
xayb(my dx+nx dy)+xcyd(py dx+qx dy) = 0, where
a,b,c,d,m,n,p are constants,then xhyk is an IF, where h,k
are constants and can be obtained by applying the
condition that after multiplication by xhyk the given
ODE becomes exact.
Example 2.9 (y2+2x2y)dx+(2x3-xy)dy = 0
# Let xhyk be an IF. Multiplying the given equation by
this
factor,
we
have
(xhyk+2+2xh+2yk+1)dx+(2xh+3-
xh+1yk+1)dy = 0 (2.4). Since (2.4) is to be exact, from
the condition of exactness (My=Nx), we obtain,
(k+2)xhyk+1+2(k+1)xh+2yk = -(h+1)xhyk+1+2(h+3)xh+2yk.
equating coefficients of xhyk+1and xh+2yk on both sides
and solving , we get h = -5/2, k = -1/2. Thus x-5/2y-1/2 is
an IF.
PRACTICE SUMS
1.
(x3ex-my2) dx+m xy dy = 0 (solution: 2x2ex+my2 = c.)
54
2.
(x2y – 2xy2) dx – (x3-3x2y) dy = 0.
3.
(x2y2+xy+1) y dx+(x2y2 – x+1)x dy = 0.
4.
(y+y3/3+x2/2) dx+[(x+xy2)/4] dy = 0.
5.
(xy2-x2)dx+(3x2y2+x2y – 2x3+y2) dy = 0
6.
(2y dx+3x dy)+2xy(3y dx+4x dy) = 0.
7.
(x3+xy4)dx +2y3dy = 0.
8.
(2xy4ey+2xy3+y) dx+(x2y4ey – x2y2 – 3x) dy = 0.
FIRST ORDER LINEAR DIFFERENTIAL EQUATION
A differential equation of first order is linear if the
dependent variable y and its derivatives occur only in
first degree and are not multiplied together. It is of the
form y1+Py = Q(2.5), where P and Q are either
constants or functions of x alone. As we have seen
above,𝑒 ∫ 𝑃(π‘₯)𝑑π‘₯ is an I.F. of (2.5).
Example 2.10 (1+x)y1 – xy = 1-x.
55
Y1 Q=
π‘₯
1+π‘₯
1−π‘₯
1+π‘₯
1−π‘₯
y =
1+π‘₯
. Comparing with (2.5), P =-
. an I.F. = 𝑒
1
∫(1+π‘₯−1)𝑑π‘₯
π‘₯
1+π‘₯
and
= 𝑒 ln(1+π‘₯)−⁑π‘₯ . Multiplying
given equation by the I.F., we get y(1+x)e-x =
1−π‘₯
∫ 1+π‘₯ (1 + π‘₯ )𝑒 −π‘₯ 𝑑π‘₯ = xe-x+c.
Example 2.11 (1+y2) dx = (tan-1y – x) dy
𝑑π‘₯
𝑑𝑦
+
exp
x𝑒
π‘₯
1+𝑦 2
[∫
π‘‘π‘Žπ‘›−1 𝑦
=
π‘‘π‘Žπ‘›−1 𝑦
1−𝑦 2
𝑑𝑦
1+𝑦
=∫
, which is linear in x. an I.F. =
=
2]
π‘‘π‘Žπ‘›−1 𝑦
1−𝑦 2
solution is x𝑒 π‘‘π‘Žπ‘›
𝑒 π‘‘π‘Žπ‘›
𝑒 π‘‘π‘Žπ‘›
−1 𝑦
−1 𝑦
−1 𝑦
.
Solution
is
𝑑𝑦 . Put t = tan-1y. The
= 𝑒 π‘‘π‘Žπ‘›
−1 𝑦
(π‘‘π‘Žπ‘›−1 𝑦 − 1) + 𝑐.
Example 2.12 (x+2y3) y1 = y
1
The equation can be put as : x1 – .x = 2y2 (2.6), which
𝑦
is linear in x. An I.F. = 𝑒
−∫
1
𝑑𝑦
𝑦
= 1/y. Multiplying (2.6)
by the I.F.,x/y = ∫ 2𝑦 2 𝑑𝑦 + 𝑐. Thus x = y3+cy.
𝑦
56
PRACTICE SUMS
1. x cos xy1+y(x sin x+cos x) = 1.
1
2. Y2+(π‘₯ − )y1 = 0.
𝑦
BERNOULLI’S EQUATION: D.E. REDUCIBLE TO
LINEAR FORM
An equation of the form y1+Py = Qyn (2.7) where P and
Q are constants or functions of x alone and n is
constant except 0 and 1, is called a Bernoulli’s
equation. Dividing (2.7) by yn and putting v = y-n+1, the
equation reduces to v1+(1-n)pv = (1-n)Q , which is
linear in v.
Example 2.13 (1-x2)y1+xy = xy2.
Given equation can be written as y-2y1+
π‘₯
1−π‘₯
−1
=
2𝑦
π‘₯
1−π‘₯ 2
.
Let y-1 = v, so that v1 = -y-2y1 and the given equation
reduces to v1-
π‘₯
1−π‘₯
2v = -
π‘₯
1−π‘₯ 2
, which is linear in v. an I.F.
57
= exp[− ∫
π‘₯
1−π‘₯ 2
𝑑π‘₯]= (1-x2)1/2.. Multiplying by I.F. and
integrating, v(1-x2)1/2 = (1-x2)1/2+c. thus (1-y)√1 − π‘₯ 2
= cy.
Practice sums
1. y1+x sin2y = x3cos2y.
2. xy- y1 = y3𝑒 −π‘₯
2
3. (x2y3+2xy) dy = dx
4. Y(2xy+ex) dx – ex dy = 0.
CHAPTER 3: DIFFERENTIAL EQUATIONS OF FIRST
ORDER AND OF DEGREE HIGHER THAN ONE
An ODE of order one and degree higher than one has
the general form
Pn+P1(x,y)pn-1+P2(x,y)pn-2+…+Pn-1p+Pn = 0 (3.1) ,where
p= dy/dx. In our course of study we will consider
solutions of three particular cases of (3.1).
58
Case 1 Equations solvable for p
Let us consider the special case when (3.1) is of the
form [p-f1(x,y)] [p-f2(x,y)]…[p-fn(x,y)] = 0 (3.2).
Equating each factor to zero, we get n number of first
order and first degree ODEs. Let their general
solutions be f1(x,y,c1) = 0, f2(x,y,c2) = 0,…,fn(x,y,cn) = 0,
where c1,c2,…,cn are arbitrary parameters. We observe
that f1(x,y,c). f2(x,y,c)…fn(x,y,c) = 0(3.3) is a solution of
the first order ODE(3.2) and contains one parameter .
Thus (3.3) is the general solution of (3.2).
Example 3.1 x2 p2+xyp-6y2 = 0.
# Given ODE is solvable for p: (p-2y/x)(p+3y/x) = 0.
General solution of p-2y/x = 0 is y = c1x2 and that of
p+3y/x = 0 is xy3 = c2. Hence the general solution of
given ODE is (y – cx2)(xy3 – c) = 0, c parameter.
Case 2 Equations solvable for y
59
Let us suppose the given ODE (3.1) is expressible in
the form y = f(x,p) (3.4). Differentiating w.r.t. x, we get
p = g(x,p,dp/dx)(3.5). Solving (3.5), we obtain F(x,p,c)
= 0(3.6). Finally, we eliminate p between (3.4) and
(3.6). The p-eliminant gives the general solution of
(3.4). When the elimination of p cannot be carried out
easily, we just leave after remarking that the peliminant of (3.4) and (3.6) gives the general solution
of (3.4).
Example 3.2 y+px = x4p2
# Differentiating w.r.t. x yields , after simplification,
dp/p +2dx/x = 0, which on integration gives p = c/x2 .
Substituting this value of p in the given equation , we
obtain the general solution xy+c = c2x of the given ODE.
Case 3 Equations solvable for x
Let us suppose the given ODE (3.1) is expressible in
the form x = f(y,p) (3.7). Differentiating w.r.t. y, we get
60
1/p = g(y,p,dp/dy)(3.8). Solving (3.8), we obtain
F(y,p,c) = 0(3.9). Finally, we eliminate p between (3.7)
and (3.9). The p-eliminant gives the general solution of
(3.7). When the elimination of p cannot be carried out
easily, we just leave after remarking that the peliminant of (3.7) and (3.9) gives the general solution
of (3.7).
Example 3.3 y2 ln y = xy p+p2
# Given equation is x = y ln y/p-p/y, which is in
solvable for x form. Differentiating w.r.t. y, after
simplification we get dp/p = dy/y, which on
integration gives p = cy. Eliminating p , the general
solution is ln y = cx+c2.
PRACTICE SUMS
1. (p-xy)(p-x2)(p-y2) = 0 [ solution: (lny – x2/2-c)(y-x3/3c)(x+1/y+c) =0]
61
2. (p+x+y)(xp+y+x)(p+2x)=0
x)(2xy+x2-c)(y+x2-c)
[
solution(1-x-y-ce-
= 0]
3. p2+2py cot x = y2[solution: [y(1-cos x)-c][y(1+cos x)-c]
= 0]
4. y = yp2+2px[solution:2x√1 + 𝑐π‘₯+cxy = 0]
5. xp3 = a+bp[solution:p-eliminant of given equation and
y = 3a/(2p2)+2b/p+c]
A USEFUL SPECIAL CASE: CLAIRAUT’S EQUATION
Clairaut’s equation is of the form y = px+f(p)(3.10).
Differentiating w.r.t. x, we get [x+f/(p)] dp/dx = 0. If
dp/dx = 0,then p=c (constant). Eliminating p between
this and (3.10), the general solution of (3.10) is y =
cx+f(c), c parameter. If we eliminate p between x+f/(p)
= 0 and (3.10), we get a solution of (3.10) which does
not contain any parameter and gives a singular
solution of (3.10).
Example 3.4 (y-px)(p-1) = p
62
# y = xp+p/(p-1), in Clairaut’s form. Differentiating
w.r.t. x, dp/dx[x-1/(p-1)2] = 0. dp/dx = 0 gives p = c .
Thus general solution is y = xc+c/(c-1). From [x-1/(p1)2] = 0, p =
1
√π‘₯
+1. Substituting in given equation, the
1
1
1
√π‘₯
√π‘₯
√π‘₯
singular solution is [y-( +1)x].⁑ =( +1).
PRACTICE SUMS
1. p = ln(px-y) [ general solution:c = ln(cx-y)]
2. y = px+√π‘Ž2 𝑝2 + 𝑏 2 [ singular solution: y2a2(a2-x2) =
b2(x2+a2)]
CHAPTER 4: APPLICATIONS OF FIRST ORDER ODE
Example 4.1 A culture initially has N0 number of
bacteria. At t = 1 hour the number of bacteria is
measured to be 3N0/2. If the rate of growth be
proportional to the number of bacteria present,
determine the time necessary for the number of
bacteria to triple.
63
# The corresponding ODE is dN/dt = k N subject to
N(0) = N0. Separating and integrating, N = N(t) = cekt.
At t = 0,N0 = ce0 =c. thus N = N0ekt. At t = 1, 3N0/2 =
N0ek, so that ek = 3/2. Hence k = ln(3/2) = .4055. So N =
N0e.4055t.to find the time when bacteria had tripled, 3N0
= N0e.4055t. Calculating, t = 2.71 hour...\Documents\5.gif
Example 4.2 It is found that 0.5 per cent of radium
disappears in 12 years.(a) What per cent will
disappear in 1000 years? (b) What is the half-life of
radium?
# Let A be the quantity of radium in grammes, present
after t years. Then dA/dt represents the rate of
disintegration of radium. According to the law of
radioactive decay, dA/dt varies as A, that is dA/dt = kA(since A is decreasing with time). Let A0 be the
amount in grammes present initially. Then 0.005A0 g.
disappears in 12 years, so that .995 g remains. Thus A
= A0 at t = 0, and A = .995A0 g. at t=12(years) . Solution
64
of the ODE is A = ce-kt. Since A = A0 at t = 0, c = A0. So A
= A0e-kt. Also at t = 12, A = -995A0, thus -995A0 = A0e-12k,
or e-k = (-995)1/12,or k = .000418. Hence A = A0e-.000418t.
(a)Now, when t = 1000, A = .658A0, so that 34.2% will
disappear in 1000 years. (b) For half-life, A0/2 = A0 e.000418t
or, t = 1672.1770 years. ..\Documents\6.gif
Example 4.3 A body whose temperature T is initially
200 0C is immersed in a liquid whose temperature is
constantly 1000C. If the temperature of the body is
1500C at t = 1 minute, what is the temperature at t = 2
minutes?
# According to Newton’s law of cooling, dT/dt = k(T100). Solving, ln(T-100) = kt+c. when t = 0,T = 200. So
c = ln 100. Also , at t = 1,T = 150. So ln 50 = k+ln 100.
Hence k = - ln 2. Substituting values of k,c, we get T =
100[1+2-t].
Thus
,
at
1250C...\Documents\7.gif
65
t
=
2
min,
T
=
Example 4.4 A tank contains 100 litres brine in which
10 kg of salt is dissolved. Brine containing 2kg per litre
flows into the tank at 5litre/minute. If the well-stirred
mixture is drawn off at 4 litre/ minute, find(a) the
amount of salt in the tank at time t minute.
# Let P(t) denote the number of kg of salt in the tank
and G(t), the number of litres of brine at time t. then
G(t) = 100+t. P(0) = 10 and G(0) = 100. Since 5(2) = 10
kg of salt is added to the tank per minute and
[P/(100+t)]4 kg salt per minute is extracted from the
tank, P then satisfies the ODE dP/dt = 10- 4P/(100+t),
which is a linear differential equation in P. solving, P(t)
= 2(100+t)-190(100)4(100+t)-4.
Orthogonal Trajectories
Two families F1 and F2 of curves are mutually
orthogonal if each curve of any one family intersects
each member of the other family at right angles. We
66
say either family forms a set of orthogonal
trajectories of the other family.
Fig.9:Orthogonal Trajectories
As an example, consider the family of all circles having
their centres at the origin. The orthogonal trajectories
for this family of circles would be members of the
family of straight lines passing through the origin.
Similarly, the family of elipses and the family members
of which are drawn in yellow form orthogonal
trajectories of each other. As a physical example, the
family of lines of force around a bar magnet and the
family of equipotential lines form orthogonal family of
each other.
67
To find the orthogonal trajectories of a given family of
curves, we first find the differential equation of the
family . In the differential equation we replace dy/dx
by -1/dy/dx and solve the resulting differential
equation.
Example 4.5 Find the orthogonal trajectories to x2+y2
= cx.
# c = (x2+y2)/x. So y1 = (y2-x2)/(2xy). The family of
orthogonal trajectories thus have the differential
equation y1 = 2xy/(x2 – y2). Solving, the equation of
orthogonal trajectories is x2+y2 = c1y. Thus the given
family of curves is self-orthogonal.
Example 4.6 Find orthogonal trajectories of the family
of rectangular hyperbolas xy = c.
# The ODE of the family is y1 = -y/x. The ODE of the
family of orthogonal trajectories is y1= x/y. Solving y2x2 = c.
68
CHAPTER 5: LINEAR DIFFERENTIAL EQUATIONS OF
SECOND ORDER
A linear ODE of order n is an equation of the form
an(x)yn+an-1(x)yn-1+…+a1(x)y1+a0(x)y = Q(x)(5.1)
where a0,a1,…,an,Q are continuous real functions on an
interval I and a0(x)≠0 on I.
Notation: ai standing for i th function of x whereas yi
standing for ith derivative of y.
If Q(x) is identically zero on I, then (5.1) reduces to
an(x)yn+an-1(x)yn-1+…+a1(x)y1+a0(x)y =0 (5.2) and is
69
referred to as homogeneous ODE of order n. If all the
coefficients ai of (5.2) are constants, it is called linear
homogeneous equation with constant coefficients. The
general solution of (5.2) is called complementary
function(C.F.) of (5.1).
Solution of the homogeneous linear differential
equations with constant coefficients
Consider the differential equation (DE) anyn+an-1yn1+…+a1y1+a0y
= 0(5.3), where a0,a1,…,an are all
constants and an≠0.
Let y = emx be a solution of (5.3), where m is a suitable
constant to be determined suitably. Calculating y1,…,yn,
substituting in the equation and noting that emx≠0, we
obtain the characteristic equation(CE) or auxiliary
equation anmn+an-1mn-1+…+a1m+a0 = 0. While solving
the CE, following three cases may arise:
ο‚· all the roots are real and distinct
70
ο‚· all roots are real but some are multiple roots
ο‚· some roots are real and some are conjugate complex
ο‚· all roots are imaginary.
We next explain through examples how to find general
solution of (5.3) under different possible cases.
Example 5.1 y3+6y2+11y1+6y =0
Roots of auxiliary equation are -1,-2,-3. (Show
calculations!). Thus y = e-x, y = e-2x and y = e-3x are
solutions of given DE . Solutions are also linearly
independent since the wronskian
𝑒 −π‘₯
=|−𝑒 −π‘₯
𝑒 −π‘₯
𝑒 −2π‘₯
−2𝑒 −2π‘₯
4𝑒 −2π‘₯
𝑒 −3π‘₯
−3𝑒 −3π‘₯ | ≠0 for all x(calculate and
9𝑒 −3π‘₯
verify). Hence the general solution is y = c1e-x+c2e2x+c
-3x
3e ,
c1,c2,c3 are independent parameters.
Example 5.2 y3-3y1+2y = 0.
71
Roots of auxiliary equation are 1,1,-2. y = ex, y = xex and
y = e-2x are linearly independent solutions. General
solution is y = (c1+c2x)ex+c3e-2x.
Example 5.3 y3+y = 0.
Roots of auxiliary equation are -1, 1/2 ± √3/2 i.
General solution is y = c1e-x+ex/2(c2 cos√3x/2+c3 sin
√3x/2).
Solution of the nonhomogeneous linear differential
equations with constant coefficients by means of
polynomial operator
The general solution of (5.1) is given by y = yc+yp,
where yc is the complementary function( that is, the
general solution of the corresponding homogeneous
equation) and y = yp(x) is a particular integral(P.I., that
is, a particular solution) of (5.1). above we have
already seen how to find out yc for a constant
coefficient homogeneous linear DE. Below we explain
72
how to find PI using D-operator method. We use the
notation:
Dy
=
y 1,
D2y
=
y2,…,P(D)
=
a0+a1D+a2D2+…+anDn. Using this notation, the linear
nonhomogeneous constant coefficients DE of order n:
anyn+an-1yn-1+…+a1y1+a0y = Q(x) can be written as
P(D)y = Q(x). The operator P(D) has the following
properties:
Property 1 If f(x) is an n th order differentiable
function of x, then P(D)(eaxf) = eaxP(D+a)f, where a is a
constant.
Property 2 Let P(D)y = Q(x). The inverse operator of
P(D), written as P-1(D) or 1/P(D), is then defined as an
operator which, when operating on Q(x), will give the
P.I. yp of P(D)y = Q(x) that contains no constant
multiples of a term in CF: P-1(D)Q(x) = yp, or,
yp=(1/P(D))Q(x).
73
Property 3 If P(D)y = eax, then yp =
1
eax = eax/P(a),
𝑃(𝐷)
P(a)≠0.
Property 4 If P(D)y = sin(ax) or cos(ax), then yp
1
=
sin (ax) or
𝑃(𝐷2 )
1
⁑cos(ax).
𝑃(𝐷2 )
Property 5 If P(D)y =eaxV(x), then yp =
1
1
eaxV =
𝑃(𝐷)
V.
𝑃(𝐷+π‘Ž)
Property 6 If P(D)y =xV(x), then yp =
1
1
𝑃(𝐷)
(xV) = x
𝑃1 (𝐷)
.
[𝑃(𝐷)]2
V-
𝑃(𝐷)
Example 5.4 (D2-4)y = x2, y = 0 and 𝑦1 = 1 when x = 0.
# C.F. yc = ae2x+be-2x
P.I. yp =
1
𝑃(𝐷)
1
𝐷2
4
4
− (1 +
x2
=
1
x2
𝐷2 −4
1
=-
x2
𝐷2
4(1− )
4
1
1
4
2
+ β‹― )x2= - (π‘₯ 2 + ).
74
1
= - (1 −
4
𝐷2 -1 2
) x =
4
Thus the general solution is y = yc+yp = ae2x+be-2x1
4
1
(π‘₯ 2 + ).
2
π‘₯
Hence y1 = 2ae2x – 2be-2x - . Using the given conditions,
2
1
1
8
2
a+b = and a – b = . Hence a = 5/16 and b = -3/16.
Thus the PI satisfying the given condition is y = 5/16
1
1
4
2
e2x-3/16 e-2x- (π‘₯ 2 + ).
Example 5.5 (D2-2D+5)y = e-x
# C.F. e-x(c1cos 2x+ c2 sin 2x)
P.I. yp=
1
𝐷2 −2𝐷+5
e-x =
1
-x
e
2
(−1) −2(−1)+5
= e-x/8.
General solution is y = e-x(c1cos 2x+ c2 sin 2x)+ e-x/8.
Example 5.6 (D2-3D+2)y = 3 sin 2x
# C.F. aex+be2x
75
P.I. yp =
1
3
1
(D2 −3D+2)
sin 2x = -3
3𝐷+2
3
20
1
3 sin 2x = 3
3𝐷−2
sin 2x =-
−22 −3𝐷+2
sin 2x =
9𝐷2 −4
−3
(3𝐷
9(−22 )−4
− 2)sin 2x =
(3 cos 2π‘₯ − sin 2π‘₯).
Example 5.7 (D2-2D+1)y = exx2.
# C.F. (a+bx)ex.
P.I. yp=
1
𝐷2 −2𝐷+1
exx2 = ex
1
2
x
2
(𝐷+1) −2(𝐷+1)+1
= ex
1
𝐷2
x2 =
exD-2x2 = (exx4)/12.
Example 5.8 (D2+6D+9)y = 2e-3x.
# We can not use property 3 , since P(-3) = 0. Instead
we apply property 5.
Yp =
3x
1
𝐷2
1
𝐷2 +6𝐷+9
(2e-3x) = 2e-3x
1
(1)
(𝐷−3)2 +6(𝐷−3)+9
(1) = 2e-3x.x2/2 = x2e-3x.
Example 5.9 (D2+2D+1)y = x cos x
76
= 2e-
# P.I. yp =
1
1
(x cos x) = x
𝐷2 +2𝐷+1
cos x -
𝐷2 +2𝐷+1
π‘₯
1
2
2𝐷2
cos x = 𝐷 −1 cos π‘₯ −
2𝐷+2
𝐷2 +2𝐷+1
(𝐷 + 1)cos x = xsin x/2- ½
D2(-sin x+cos x) = x sin x/2 – ½(sin x – cos x).
Example 5.10 (D2+4)y = cos (2x)
# Let y =
1
1
cos(2x), z =
𝐷2 +4
(cos 2x+i sin 2x)=
𝐷2 +4
=
e2ix
1
𝐷2 +4𝑖𝐷
(1) =
e2ix
1
4𝑖𝐷
1
1
𝐷2 +4
sin(2x). then y+iz =
e2ix = e2ix
𝐷2 +4
1
(1)
(𝐷+2𝑖)2 +4
𝐷 −1
(1 − 𝑖 ) (1) = (cos 2x+i sin
4
2x)x/4i = x sin(2x)/4-i x cos(2x)/4. Equating real part,
y = xsin(2x)/4.
PRACTICE SUMS
1. y2 – 4y1 = x2.
2. Y2 – y1 – 2y = x2ex
3. Y2 = x2
4. Y3+3y2 – 4y = xe-2x.
CAUCHY-EULER EQUATION
77
An
equation
1+…+a1xy1+a0y
of
the
form
anxnyn+an-1xn-1yn-
= Q(x) (5.4) , where ai’s are constants ,
is called a Cauchy-Euler equation of order n. by
undertaking a transformation x = et of independent
variable, (5.4) can be transformed to a constant
coefficient linear ODE.
Example 5.11 x2y2+xy1-4y = x2.
# Putting x = et, or ln x = t and D1 = d/dt, the given ODE
can be written as [D1(D1-1)+D1-4]y = e2t, or (D12-4)y =
e2t. C.F. is yc = ae2t+be-2t = ax2+bx-2.
P.I. yp=
1
e2t
𝐷12 −4
=
e2t
1
(1)=
(𝐷1 +2)2 −4
e2t
1
4𝐷1
(1 +
𝐷1 −1
4
) (1) =
¼ e2tt = ¼ x2ln x.
Hence the general solution of given equation is y =
yc+yp = ax2+bx-2+1/4 x2 ln x.
PRACTICE SUMS
1. x2y2+3xy1+y =
1
(1−π‘₯)2
78
2. x2y2+y = 3x2.
3. x2y2+5xy1+3y = e-x.
79
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