sms 2308 - mathematical methods lecture notes
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SMS 2308 - Mathematical MethodsLecture Notes
Samsun Baharin Haji Mohamad
September 9, 2009
Chapter 1
Differential Equations
1.1 Definitions
A differential equation is an equation which involve differential coefficients ordifferentials. For example, the equations below are all differential equations.
1. exdx+ eydy = 0
2. d2xdt2
+ n2x = 0
3. y = x dydx
+ xdxdy
4.[1 +
(dydx
)2]3/2/ d
2ydx2
= c
5. dxdy− wy = a cos(pt), dy
dt+ wx = a sin(pt)
6. x∂u∂x
+ y ∂u∂y
= 2u
7. ∂2y∂t2
= c2 ∂2y∂x2
An ordinary differential equations (ODE) is differential equations whereall the differential coefficients have reference to a single independent variable.Item 1 to 5 in the list are all ODEs.
A partial differential equation (PDE) is differential equations which thereare two or more independent variables and partial differential coefficientswith respect to any of them. Item 6 and 7 are PDEs.
The ORDER of a differential equation is the order of the highest deriva-tive appearing in it.
1
The DEGREE of a differential equation is the degree of the highestderivative occuring in it, after the equation has been expressed in a form freefrom any radicals or fractions as far as the derivatives are concerned.
From the list above, we can see that
1. Item 1 is of the first order and first degree.
2. Item 2 is of the second order and first degree.
3. Item 3 written as y dydx
= x(dydx
)2+ x is clearly of the first order but of
second degree.
4. Item 4 written as[1 +
(dydx
)2]3= c2
(d2ydx2
)2is of the second order and
second degree.
1.2 Solution of Differential Equation
A solution of a differential equation is a relation between the variables whichsatisfies the given differential equation.
y = A cos(nx+ �)
is a solution of
d2y
dx2+ ny2 = 0
The general (or complete) solution of a differential equation is that inwhich the number of arbitrary constants are equal to the order of the dif-ferential equation. Thus y = A cos(nx + �) is a solution for d2y
dx2+ ny2 = 0
as the number of arbitrary constants (A,�) are the same as the order ofd2ydx2
+ ny2 = 0.A particular solution is a solution that can be obtained from general
solution by giving particular values to the arbitrary constants. For example
y = A cos(nx+ �/4)
is the particular solution of the equation d2ydx2
+ny2 = 0 as it can be derivedfrom the general solution y = A cos(nx+ �) by putting � = �/4.
A differential equation may sometimes have an additional solution whichcannot be obtained from the general solution by assigning a particular valueto the arbitrary constant. Such a solution is called a singular solution.
2
1.2.1 Linearly independent solution
Two solutions y1(x) and y2(x) of the differential equation
d2y
dx2+ P (x)
dy
dx+Q(x)y = 0
are said to be linearly independent if c1y1(x) + c2y2(x) = 0 such thatc1 = 0 and c2 = 0.
If c1 and c2 are not both zero, then the two solutions y1(x) and y2(x) aresaid to be linearly dependent.
If y1(x) and y2(x) any two solutions of d2ydx2
+ P (x) dydx
+ Q(x)y = 0, thentheir linear combination c1y1(x) + c2y2(x) where c1 and c2 are constants, is
also a solution of d2ydx2
+ P (x) dydx
+Q(x)y = 0.
1.3 First Order and First Degree ODE
Some special methods to find solutions for these ODEs will be discussed here,
1. Separation of Variables
2. Homogeneous equations
3. Linear equations
4. Exact equations.
1.3.1 Separation of Variables
If in a n equation, it is possible to collect all function of x and dx on oneside and all the functions of y and dy on the other side, then the variablesare said to be separable. Thus the general form of such equation is
f(x)dx = g(y)dy
Integrating both sides, we get∫f(x)dx =
∫g(y)dy + c
as its solution.
3
Example 1 Solvedy
dx=x(2 log x+ 1)
sin y + y cos y
We separate them into
(sin y + y cos y)dy = (x(2 log x+ 1))dx
Integrating both side, we get∫sin ydy +
∫y cos ydy = 2
∫log x ⋅ xdx+ 2
∫xdx
− cos y +
[y sin y −
∫sin y ⋅ 1dy + c
]= 2
[(log x ⋅ x
2
2−∫
1
x⋅ x
2
2dx
)+x2
2
]− cos y + y sin y + cos y + c = 2x2 log x− x2
2+x2
2
Hence the solution is2x2 log x− y sin y = c
Example 2 Solvedy
dx= e3x−2y + x2e−2y
We separate them intoe2ydy = (e3x + x2)dx
Integrating both side, we get∫e2ydy =
∫(e3x + x2)dx+ c
e2y
2=e3x
3+x3
3+ c
Hence the solution is3e2y = 2(e3x + x3) + 6c
Example 3 Solve
dy
dx= sin(x+ y) + cos(x+ y)
Setting x+ y = t so that dy/dx = dt/dx− 1. The given equation becomes
dt
dx− 1 = sin t+ cos t
dx =dt
1 + sin t+ cos t
4
Integrating both side, we get∫dx =
∫dt
1 + sin t+ cos t+ c
x =
∫2d�
1 + sin 2� + cos 2�+ c (setting t = 2�)
=
∫2d�
2 cos2 � + 2 sin � cos �c
=
∫sec2 �
1 + tan �d� + c
= log(1 + tan �) + c
Hence the solution is
x = log
[1 + tan
1
2(x+ y)
]+ c
Example 4 Solve
y
x
dy
dx+
x2 + y2 − 1
2(x2 + y2) + 1= 0
Setting x2 + y2 = t, we get
2x+ 2ydy
dx=dt
dx
ory
x
dy
dx=
1
2x
dt
dx− 1
The given equation becomes
1
2x
dt
dx− 1 +
t− 1
2t+ 1= 0
1
2x
dt
dx= 1− t− 1
2t+ 1=
t+ 2
2t+ 1
2xdx =2t+ 1
t+ 2dt
2xdx =
(2− 3
t+ 2
)dt
Integrating both side, we get∫2xdx =
∫ (2− 3
t+ 2
)dt+ c
x2 = 2t− 3 log(t+ 2) + c
Hence the solution is
x2 + 2y2 − 3 log(x2 + y2 + 2) + c = 0
5
1.3.2 Homogeneous Equations
Homogeneous equations are of the form
dy
dx=f(x, y)
g(x, y)
where f(x, y) and g(x, y) are homogeneous functions of the same degree in xand y.
To solve a homogeneous equation,
1. Set y = ux, then dydx
= u+ xdudx
2. Separate the variables u and x, and integrate.
Example 1 Solve(x2 − y2)dx− xydy = 0
Rearrange the equation, we get
dy
dx=x2 − y2
xy
Setting y = ux, then dydx
= u+ xdudx
, the equation becomes,
u+ xdu
dx=
1− u2
u
xdu
dx=
1− 2u2
u
Separating the variables, we get
u
1− 2u2du =
dx
x
Integrating both sides, we get∫u
1− 2u2du =
∫dx
x+ c
−1
4
∫−4u
1− 2u2du =
∫dx
x+ c
−1
4log(1− 2u2) = log x+ c
4 log x+ log(1− 2u2) = −4c
log x4(1− 2u2) = −4c
x4(
1− 2y2
x2
)= e−4c = c′ (Set u = y/x)
6
Hence the solution isx2(x2 − 2y2) = c′
Example 2 Solve(x tan
y
x− y sec2
y
x
)dx+
(x sec2
y
x
)dy = 0
The equation can be rearrange into homogeneous equation
dy
dx=(yx
sec2y
x− tan
y
x
)cos2
y
x
Setting y = ux, then dydx
= u+ xdudx
, the equation becomes,
u+ xdu
dx= (u sec2 u− tanu) cos2 u
xdu
dx= u− tanu cos2 u− u
Separating the variables, we get
sec2 u
tanudu = −dx
x
Integrating both side, we get∫sec2 u
tanudu = −
∫dx
x
log tanu = − log x+ log c
x tanu = c
Hence the solution isx tan
y
x= c
Example 3 Solve
(1 + ex/y)dx+ ex/y(
1− x
y
)dy = 0
Rewrite the equation into its homogeneous form, we get
dx
dy= −
ex/y(
1− xy
)(1 + ex/y)
7
Setting x = uy, then dxdy
= u+ y dudy
, the equation becomes
u+ ydu
dy= −e
u(1− u)
(1 + eu)
ydu
dy= −e
u(1− u)
(1 + eu)− u = − u+ eu
(1 + eu)
Separating the variables, we get
−dyy
=1 + eu
u+ eudu =
d(u+ eu)
u+ eu
Integrating both side, we get
−∫dy
y=
∫d(u+ eu)
u+ eu
− log y = log(u+ eu) + c
y(u+ eu) = e−c = c′
Hence the solution isx+ yex/y = c′
1.3.3 Equations Reducible to Homogeneous Form
The equation of the form
dy
dx=
ax+ by + c
a′x+ b′y + c′
can be reduced to the homogeneous form as follows:Case I. When a
a′∕= b
b′
Settingx = X + ℎ, y = Y + k, (ℎ, k are constants)
anddx = dX, dy = dY
the equation becomes
dY
dX=
aX + bY + (aℎ+ bk + c)
a′X + b′Y + (a′ℎ+ b′k + c′)
we choose ℎ and k so that dYdX
become homogeneous equation.
8
Set aℎ+ bk + c = 0 and a′ℎ+ b′k + c′ = 0 so that
ℎ
bc′ − b′c=
k
ca′ − c′a=
1
ab′ − ba′
or
ℎ =bc′ − b′cab′ − b′a
, and k =ca′ − c′aab′ − ba′
Thus when ab′ − ba′ ∕= 0, dYdX
becomes
dY
dX=
aX + bY
a′X + b′Y
which is homogeneous in X, Y and be solved by setting Y = uX.Example Solve
dy
dx=y + x− 2
y − x− 4
Settingx = X + ℎ, y = Y + k, (ℎ, k are constants)
anddx = dX, dy = dY
the equation becomes
dy
dx=y + x+ (k + ℎ− 2)
y − x+ (k − ℎ− 4)
Letting k + ℎ − 2 = 0 and k − ℎ − 4 = 0, then ℎ = −1 and k = 3 then theequation will be dY
dX= Y+X
Y−X which is homogeneous in X and Y .
Setting Y = uX, then dYdX
= u+X dudX
, the equation becomes,
u+Xdu
dX=u+ 1
u− 1
Xdu
dX=
1 + 2u− u2
u− 1u− 1
1 + 2u− u2du =
dX
X
9
Integrating both sides, we get
−1
2
∫2− 2u
1 + 2u− u2du =
∫dX
X
−1
2log(1 + 2u− u2) = logX + c
log
(1 +
2Y
X2− Y 2
X2
)+ logX2 = −2c
log(X2 + 2XY − Y 2) = −2c
X2 + 2XY − Y 2 = e−2c = c′
Setting X = x− ℎ = x+ 1 and Y = y− k = y− 3, the previous equationbecomes
(x+ 1)2 + 2(x+ 1)(y − 3)− (y − 3)2 = c′
x2 + 2xy − y2 − 4x+ 8y − 14 = c′
which is the required solution.Case II. When a
a′= b
b′
When ab′− ba′ = 0, the above method fails as ℎ and k become infinite orundetermined.
Seta
a′=b
b′=
1
mor
a′ = am, b′ = bm
then dydx
becomesdy
dx=
(ax+ by) + c
m(ax+ by) + c′
Setting ax+by = t, so that a+b dydx
= dtdx
or dydx
= 1b
(dtdx− a), then the previous
equation becomes
1
b
(dt
dx− a)
=t+ c
mt+ c′
dt
dx= a+
bt+ bc
mt+ c′
=(am+ b)t+ ac′ + bc
mt+ c′
so the variables are separable. In the solution, setting t = ax + by, we getthe required solution of dy
dx
10
Example Solve
(3y + 2x+ 4)dx− (4x+ 6y + 5)dy = 0
The equation can be rearrange as
dy
dx=
(2x+ 3y) + 4
2(2x+ 3y) + 5
Setting 2x+ 3y = t, then 2 + 3 dydx
= dtdx
The equation becomes,
1
3
(dt
dx− 2
)=
t+ 4
2t+ 5
dt
dx=
7t+ 22
2t+ 52t+ 5
7t+ 22dt = dx
Integrating both sides, ∫2t+ 5
7t+ 22dt =
∫dx∫ (
2
7− 9
7⋅ 1
7t+ 22
)= x+ c
2
7t− 9
49log(7t+ 22) = x+ c
Setting t = 2x+ 3y, we have
14(2x+ 3y)− 9 log(14x+ 21y + 22) = 49x+ 49c
21x− 42y + 9 log(14x+ 21y + 22) = c′
which is the required solution.
1.3.4 Linear First-order Equations
A differential equation is said to be linear if the dependent variable andits differential coefficients occur only in the first degree and not multipliedtogether.
Thus the standard form of a linear equation of the first order is,
dy
dx+ Py = Q
11
where P Q are the functions of x.To solve the equation, we multiply both sides by e
∫Pdx, so we get
dy
dx⋅ e
∫Pdx + y
(e∫PdxP
)= Qe
∫Pdx
d
dx
(ye
∫Pdx)
= Qe∫Pdx
Integrating both side, we get
ye∫Pdx =
∫Qe
∫Pdx + c
as the required solution.Example 1 Solve
(x+ 1)dy
dx− y = e3x(x+ 1)2
Divide the equation with (x+ 1), we get
dy
dx− y
x+ 1= e3x(x+ 1)
Here P = − 1x+1
and∫Pdx = −
∫dx
x+ 1= − log(x+ 1) = log(x+ 1)−1
The integrating factor is
e∫Pdx = elog(x+1)−1
=1
x+ 1
Thus the solution for the equation is
y
x+ 1=
∫[e3x(x+ 1)]
1
x+ 1dx+ c
=
∫e3xdx+ c
=1
3e3x + c
So the solution is
y =
(1
3e3x + c
)(x+ 1)
12
Example 2 Solve (e−2√x
√x
)dx
dy= 1
Rewrite the equation into
dy
dx+
y√x
=e−2√x
√x
where P = 1√x
and ∫Pdx =
∫1√x
= 2√x
then the integrating factor becomes e∫Pdx = e2
√x
The solution for the equations is
y ⋅ e2√x =
∫e−2√x
√x⋅ e2√xdx+ c
=
∫1√xdx+ c
So the solution isy ⋅ e2
√x = 2
√x+ c
Example 3 Solve
3x(1− x2)y2 dydx
+ (2x2 − 1)y3 = ax3
Setting z = y3 and 3y2 dydx
= dzdx
, the equation becomes
x(1− x2)dzdx
= (2x2 − 1)z = ax3
dz
dx+
2x2 − 1
x− x3z =
ax3
x− x3
Here P = 2x2−1x−x3 and∫
Pdx =
∫2x2 − 1
x− x3dx
=
∫ (−1
x− 1
2
1
1 + x+
1
2
1
1− x
)dx
= − log x− 1
2log(1 + x)− 1
2log(1− x)
= − log[x√
1− x2]
13
The integrating factor is
exp
(∫2x2 − 1
x− x3dx
)= e− log[x
√1−x2] =
[x√
1− x2]−1
So the solution is
z[x√
1− x2] = a
∫x3
x(1− x2)⋅ 1
x√
1− x2dx+ c
= a
∫x(1− x2)−3/2dx+ c
= −a2
∫(−2x)(1− x2)−3/2dx+ c
z[x√
1− x2] = a(1− x2)−1/2 + c
Inserting z = y3, we get
y3 = ax+ cx√
1− x2
1.3.5 Bernoulli’s Equation
The equationdy
dx+ Py = Qyn
where P, Q are function of x is reducible to linear equation of the first order.This is a Bernoulli’s equation.
To solve it, we divide both sides with yn so that
y−ndy
dx+ Py1−n = Q
Setting y1−n = z so that
(1− n)y−ndy
dx=dz
dx
Then, the equation becomes
1
1− ndz
dx+ Pz = Q
dz
dx+ P (1− n)z = Q(1− n)
14
which is a linear equation of the first order and can be solved easily.Example Solve
xdy
dx+ y = x3y6
.Divide both sides with xy6, we get
y−6dy
dx+y−5
x= x2
Setting y−5 = z and
−5y−6dy
dx=dz
dx
The equation becomes
−1
5
dz
dx+z
x= x2
dz
dx− 5
xz = −5x2
which is the same as dydx
+ Py = Q pattern. So we can use the integratingfactor.
Integrating factor is
e∫Pdx = e−
∫(5/x)dx
= e−5 log x
= elog x−5
= x−5
The solution is
z ⋅ x−5 =
∫(−5x2) ⋅ x−5dx+ c
y−5x−5 = −5 ⋅ x−2
−2+ c
Divide both side with y−5x−5, we get
1 = (2.5 + cx2)x3y5
which is the required solution.
15
1.3.6 Exact Differential Equations
A differential equation of the form
M(x, y)dx+N(x, y)dy = 0
is said to be exact if its left hand side member is the exact differential ofsome function u(x, y) which is
du ≡Mdx+Ndy = 0
The solution is thereforeu(x, y) = c
From calculus, we see that the partial derivatives of u(x, y) is
du =∂u
∂xdx+
∂u
∂ydy
Comparing with du ≡Mdx+Ndy, then we see that
∂u
∂x= M
∂u
∂y= N
If we differentiate M with respect to y and N with respect to x, we get
∂M
∂y=
∂2u
∂y∂x
∂N
∂x=
∂2u
∂x∂y
or∂M
∂y=∂N
∂x
We integrate ∂u∂x
= M with respect to x, we get
u =
∫Mdx+ k(y) k(y) is a constant
To determine k(y), we derive ∂u∂y
from this equation, and use ∂u∂y
= N to get
dk/dy, and integrate dk/dy to get k.Example Solve
cos(x+ y)dx+ (3x2 + 2y + cos(x+ y))dy = 0
16
Test for exactness
M = cos(x+ y)
N = (3x2 + 2y + cos(x+ y))
Thus
∂M
∂y= − sin(x+ y)
∂N
∂x= − sin(x+ y)
So the equation is exact.Implicit general solution
u =
∫Mdx+ k(y)
=
∫cos(x+ y)dx+ k(y)
= sin(x+ y) + k(y)
To find k(y), we differentiate u = sin(x+ y) + k(y) with respect to y, weget
∂u
∂y= cos(x+ y) +
dk
dy
N = 3y2 + 2y + cos(x+ y)
So, dkdy
is
dk
dy= 3y2 + 2y
By integration k(y) isk(y) = y3 + y2 + c∗
Inserting k(y) into u = sin(x+ y) + k(y), we obtain the answer
u(x, y) = sin(x+ y) + y3 + y2 = c
1.3.7 Reduction to Exact Form, Integrating Factor
We can transform a non-exact equation,
P (x, y)dx+Q(x, y)dy = 0
17
by multiplying it with a function F (x, y) producing an exact equation
FPdx+ FQdy = 0
which can be solve by using the method from the previous section. F (x, y)is called Integrating Factor.How to find Integrating factor
For Mdx + Ndy = 0, the exactness condition is ∂M/∂y = ∂N/∂x. ForF (x) and FPdx+ FQdy = 0, the exactness condition is
∂(FP )/∂y = ∂(FQ)/∂x
By product rule, we getFPy = F ′Q+ FQx
Dividing by FQ and rearrange, we get
1
F
dF
dx= R where R =
1
Q
(∂P
∂y− ∂Q
∂x
)If we integrate the equation with respect to x and taking the exponent
on both side, we get the integrating factor which is
F (x) = exp
∫R(x)dx
and if our initial is F (y), we get
F (y) = exp
∫R(y)dy where R(y) =
1
P
(∂Q
∂x− ∂P
∂y
)Example Find an integrating factor and solve the initial value problem
of(ex+y + yey)dx+ (xey − 1)dy = 0, y(0) = 1
Test for exactness
∂P
∂y= ex+y + ey + yey
∂Q
∂x= ey
Since ∂P∂y∕= ∂Q
∂x, so we have to find the integrating factor to make it an exact
equation.
18
R(x) fail, since it on both x and y, so we have to use R(y), which is
R(y) =1
P
(∂Q
∂x− ∂P
∂y
)=
1
ex+y + yey(ey − (ex+y + ey + yey))
= −1
Hence the integrating factor is F (y) = exp∫−1dy = e−1. Multiplying the
integrating factor to the original equation, we get
(ex + y)dx+ (x− e−y)dy = 0
which is an exact equation and be solve using the previous method.
u =
∫(ex + y)
= ex + xy + k(y)
∂u
∂y= x+
dk
dy= N = x− e−y
dk
dy= −e−y
k = e−y + c∗
Hence, the general solution is
u(x, y) = ex + xy + e−y = c
The particular solution is
u(0, 1) = e0 + 0 ⋅ 1 + e−1 = 3.72
ex + xy + e−y = 3.72
1.4 Second Order Linear Differential Equa-
tion
1.4.1 Homogeneous Linear ODEs with Constant Coef-ficients
A second-order homogeneous linear ODEs with constant coefficient is
y′′
+ ay′+ by = 0
19
The solution is
y = e�x
y′= �e�x
y′′
= �2e�x
If we put the equation, we will get
(�2 + a�+ b)e�x = 0
Hence � is a solution of the important characteristic equation
�2 + a�+ b = 0
The roots for this quadratic equation is
�1 =1
2(−a+
√a2 − 4b) �2 =
1
2(−a−
√a2 − 4b)
then the functiony1 = e�1x y2 = e�2x
are solutions for second-order homogeneous linear ODEs with constant coef-ficient.
From algebra, we know that the quadratic equation might have threedifferent kind of roots, depending on the sign of the discriminant a2 − 4b,which are
1. Two real roots if a2 − 4b > 0.
2. A real double root if a2 − 4b = 0.
3. Complex conjugate roots if a2 − 4b < 0
Case I: Two Distinct Real Root �1 and �2In this case, the basic solution is
y1 = e�1x and y2 = e�2x
and the general solution is
y = c1e�1x + c2e
�2x
Example Solve the initial value problem
y′′
+ y′ − 2y = 0, y(0) = 4, y
′(0) = −5
20
The characteristics equation is
�2 + �− 2 = 0
Its roots are,�1 = 1 and �2 = −2
So the general equation is
y = c1ex + c2e
−2x
For finding particular solution, we differentiate once
y′= c1e
x − 2c2e−2x
and using the initial condition, we get
y = ex + 3e−2x
Case II: Real Double Root � = −a/2When a2 − 4b = 0 we only get one root, � = �1 = �2 = −a/2, hence the
only solution isy1 = e−(a/2)x
To obtain the second independent solution y2, we set y2 = uy1. Substitutethis and its derivative y
′2 and y
′′2 , we get
(u′′y1 + 2u′y′ + uy′′
1 ) + (a(u′y1 + uy′
1) + buy1 = 0
Collecting term
u′′y1 + u′(2y′
1 + ay1) + u(y′′
1 + ay′
1 + by1) = 0
The second and third expression is zero, so we are left with
u′′y1 = 0
By two integrations, we get
u = c1x+ c2
we choose c1 = 1 and c2 = 0 then u = x, so y2 = xy1, so the general solutionis
y = (c1 + c2x)e−(a/2)x
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Example Solve the initial value problem
y′′ + y′ + 0.25y = 0 y(0) = 3.0, y′(0) = −3.5
The characteristic equation is
�2 + �+ 0.25 = (�+ 0.5)2 = 0
It has double root � = −0.5, this give the general solution as
y = (c1 + c2x)e−0.5x
Taking the derivative and find c1 and c2, so we get the particular solution as
y = (3− 2x)e−0.5x
Case III: Complex Roots −1
2+ i! and −1
2− i!
The discriminant is a2 − 4b < 0, two complex roots, or we can obtain areal solution by using
y1 = e−ax/2 cos!x and y2 = e−ax/2 sin!x
where ! = b− 1
4a2. The real general solution for Case III is
y = e−ax/2(A cos!x+B sin!x)
where A, B are arbitrary constants.Example Solve the initial value problem
y′′ + 0.4y′ + 9.04y = 0, y(0) = 0, y′(0) = 3
The characteristic equation is
�2 + 0.4�+ 9.04 = 0
so the roots are �1 = −0.2 + 3i and �1 = −0.2 − 3i. Hence ! = 3. Thegeneral solution is
y = e−0.2x(A cos 3x+B sin 3x)
Differentiate the general solution and using the initial value, we get the par-ticular solution as
y = e−0.2x sin 3x
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1.4.2 Non-homogeneous ODEs
A general solution for a non-homogeneous ODEs
y′′ + p(x)y′ + q(x)y = r(x), r(x) ∕= 0
on aopen interval I is a solution of the form
y(x) = yℎ(x) + yp(x)
here, yℎ = c1y1 + c2y2 is a general solution from homogeneous ODE and ypis any solution of non-homogenous ODE containing no arbitrary constant.
Method of Undetermined Coefficients
Method of undetermined coefficients is suitable for linear ODEs with constantcoefficients a and b,
y′′ + ay′ + by = r(x)
when r(x) is an exponential function, a power of x, a cosine or sine, or sumsor products of such functions. These functions have derivative similar tor(x) itself. So, we choose a form for yp similar to r(x), but with unknowncoefficients to be determined by substituting yp and its derivatives into theODE. Table below shows the choice for yp for important form of r(x).
Term in r(x) Choice for ypke x Ce x
kxn (n = 0, 1, ⋅ ⋅ ⋅ ) Knxn +Kn−1x
n−1 + ⋅ ⋅ ⋅+K1x+K0
k cos!x K cos!x+M sin!xk cos!x K cos!x+M sin!xke�x cos!x e�x(K cos!x+M sin!x)ke�x sin!x e�x(K cos!x+M sin!x)
And the choice of rules for the method of undetermined coefficients are
1. Basic Rule If r(x) is one of the functions in the first column from thetable, choose yp from the same line and determine the coefficients bysubstituting yp and its derivatives into the equation
2. Modification rule If a term in our choice for yp happens to be asolution of the homogeneous ODE corresponding to the equation, wemultiply the choice of yp by x or x2 etc.
3. Sum Rule If r(x) is a sum of functions in the first column of the table;we choose yp by summing up the functions in the corresponding line.
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Example 1: Rule 1 Solve the initial value problem
y′′ + y = 0.001x2, y(0) = 0, y′(0) = 1.5
The general solution for homogeneous ODE y′′ + y = 0 is
yℎ(x) = A cosx+B sinx
Solution for non-homogeneous ODE, setting yp = Kx2, then y′′p = 2K.
Substitute into the equation, we get
2K +Kx2 = 0.001x2
Comparing both sides, we see that
2K = 0, K = 0.001
which the value of K contradict each other, so yp = Kx2 is not the solutionfor this equation.
Looking from the table, the choice of yp for the term r(x) = Kxn isyp = K2x
2 +K1x+K0, then
y′′
p + yp = 2K2 + 2K2x2 +K1x+K0 = 0.001x2
Comaparing both sides, we get
K2 = 0.001, K1 = 0, K0 = −0.002
This givesyp = 0.001x2 − 0.002
and the general solution becomes,
y = yℎ + yp = A cosx+B sinx+ 0.001x2 − 0.002
To find the value for A and B, we use the initial condition
y(0) = A cos 0 +B sin 0 + 0.001(0)2 − 0.002
= A− 0.002 = 0
So, A = 0.002. To find B, we diffentiate the general solution once and putthe initial condition
y′ = y′
ℎ + y′
p
= −A sinx+B cosx+ 0.002x
y′(0) = −A sin 0 +B cos 0 + 0.002(0)
= B = 1.5
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So, B = 1.5. This gives the answer as
y = 0.002 cosx+ 1.5 sinx+ 0.001x2 − 0.002
Example 2: Rule 2 Solve the initial value problem
y′′ + 3y′ + 2.25y = −10e−1.5x, y(0) = 1, y′(0) = 0
The general solution for the homogeneous ODE,
y′′ + 3y′ + 2.25y = 0
where �2 + 3�+ 2.25 = (�+ 1.5)2 = 0 is
yℎ = (c1 + c2x)e−1.5x
The solution of non-homogeneous ODE cannot be taken as yp = Ce−1.5x
since this a solution for homogeneous ODE. So, by using rule number 2, wemodify our choice function by x2. That is, we use
yp = Cx2e−1.5x
y′
p = C(2x− 1.5x2)e−1.5x
y′′
p = C(2− 3x− 3x+ 2.25x2)e−1.5x
Substitute these equations into the main equation, by ignoring the e−1.5x, weget
C(2− 6x+ 2.25x2) + 3C(2x− 1.5x2) + 2.25Cx2e−1.5x = −10
Comparing both sides, we get 2C = −10, so C = −5 and the solution is
yp = −5x2e−1.5x
Hence the general equation becomes
y = yℎ + yp = (c1 + c2x)e−1.5x − 5x2e−1.5x
Using the initial condition to find c1 and c2, we get
c1 = 1, and c2 = 1.5
This give the answer which is
y = (1 + 1.5x)e−1.5x − 5x2e−1.5x
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Example 3: Rule 3 Solve the initial value problem
y′′+ 2y′+ 5y = e0.5x + 40 cos 10x− 190 sin 10x, y(0) = 0.16, y′(0) = 40.08
The general solution for homogeneous ODE y′′ + 2y′ + 5y = 0 from thecharacteristics equation
�2 + 2�5 = (�+ 1 + 2i)(�+ 1− 2i) = 0
isyℎ = e−x(A cos 2x+B sin 2x)
The solution for non-homogeneous ODE, we choose our yp as summationof two function from the table, that is
yp = Ce0.5x +K cos 10x+M sin 10x
Substitute into the equation and comparing both side, we get
C = 0.16, K = 0, M = 2
Hence the solution is
y = yℎ + yp = e−x(A cos 2x+B sin 2x) + 0.16e0.5x + 2 sin 10x
From the initial condition, we found that A = 0 and B = 10, hence thecomplete solution is
y = 10e−x sin 2x+ 0.16e0.5x + 2 sin 10x
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