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The Laplace Transform (Sect. 4.1).
I The definition of the Laplace Transform.
I Review: Improper integrals.
I Examples of Laplace Transforms.
I A table of Laplace Transforms.
I Properties of the Laplace Transform.
I Laplace Transform and differential equations.
The Laplace Transform (Sect. 4.1).
I The definition of the Laplace Transform.
I Review: Improper integrals.
I Examples of Laplace Transforms.
I A table of Laplace Transforms.
I Properties of the Laplace Transform.
I Laplace Transform and differential equations.
The definition of the Laplace Transform.
DefinitionThe function F : DF → R is the Laplace transform of a functionf : [0,∞) → R iff for all s ∈ DF holds,
F (s) =
∫ ∞
0
e−st f (t) dt,
where DF ⊂ R is the set where the integral converges.
Remark: The domain DF of F depends on the function f .
Notation: We often denote: F (s) = L[f (t)].
I This notation L[ ] emphasizes that the Laplace transformdefines a map from a set of functions into a set of functions.
I Functions are denoted as t 7→ f (t).
I The Laplace transform is also a function: f 7→ L[f ].
The definition of the Laplace Transform.
DefinitionThe function F : DF → R is the Laplace transform of a functionf : [0,∞) → R iff for all s ∈ DF holds,
F (s) =
∫ ∞
0
e−st f (t) dt,
where DF ⊂ R is the set where the integral converges.
Remark: The domain DF of F depends on the function f .
Notation: We often denote: F (s) = L[f (t)].
I This notation L[ ] emphasizes that the Laplace transformdefines a map from a set of functions into a set of functions.
I Functions are denoted as t 7→ f (t).
I The Laplace transform is also a function: f 7→ L[f ].
The definition of the Laplace Transform.
DefinitionThe function F : DF → R is the Laplace transform of a functionf : [0,∞) → R iff for all s ∈ DF holds,
F (s) =
∫ ∞
0
e−st f (t) dt,
where DF ⊂ R is the set where the integral converges.
Remark: The domain DF of F depends on the function f .
Notation: We often denote: F (s) = L[f (t)].
I This notation L[ ] emphasizes that the Laplace transformdefines a map from a set of functions into a set of functions.
I Functions are denoted as t 7→ f (t).
I The Laplace transform is also a function: f 7→ L[f ].
The definition of the Laplace Transform.
DefinitionThe function F : DF → R is the Laplace transform of a functionf : [0,∞) → R iff for all s ∈ DF holds,
F (s) =
∫ ∞
0
e−st f (t) dt,
where DF ⊂ R is the set where the integral converges.
Remark: The domain DF of F depends on the function f .
Notation: We often denote: F (s) = L[f (t)].
I This notation L[ ] emphasizes that the Laplace transformdefines a map from a set of functions into a set of functions.
I Functions are denoted as t 7→ f (t).
I The Laplace transform is also a function: f 7→ L[f ].
The definition of the Laplace Transform.
DefinitionThe function F : DF → R is the Laplace transform of a functionf : [0,∞) → R iff for all s ∈ DF holds,
F (s) =
∫ ∞
0
e−st f (t) dt,
where DF ⊂ R is the set where the integral converges.
Remark: The domain DF of F depends on the function f .
Notation: We often denote: F (s) = L[f (t)].
I This notation L[ ] emphasizes that the Laplace transformdefines a map from a set of functions into a set of functions.
I Functions are denoted as t 7→ f (t).
I The Laplace transform is also a function: f 7→ L[f ].
The definition of the Laplace Transform.
DefinitionThe function F : DF → R is the Laplace transform of a functionf : [0,∞) → R iff for all s ∈ DF holds,
F (s) =
∫ ∞
0
e−st f (t) dt,
where DF ⊂ R is the set where the integral converges.
Remark: The domain DF of F depends on the function f .
Notation: We often denote: F (s) = L[f (t)].
I This notation L[ ] emphasizes that the Laplace transformdefines a map from a set of functions into a set of functions.
I Functions are denoted as t 7→ f (t).
I The Laplace transform is also a function: f 7→ L[f ].
The Laplace Transform (Sect. 4.1).
I The definition of the Laplace Transform.
I Review: Improper integrals.
I Examples of Laplace Transforms.
I A table of Laplace Transforms.
I Properties of the Laplace Transform.
I Laplace Transform and differential equations.
Review: Improper integrals.
Recall: Improper integral are defined as a limit.∫ ∞
t0
g(t) dt = limN→∞
∫ N
t0
g(t) dt.
I The integral converges iff the limit exists.
I The integral diverges iff the limit does not exist.
Example
Compute the improper integral
∫ ∞
0e−at dt, with a > 0.
Solution:
∫ ∞
0
e−at dt = limN→∞
∫ N
0
e−at dt = limN→∞
−1
a
(e−aN − 1
).
Since limN→∞
e−aN = 0 for a > 0, we conclude
∫ ∞
0
e−at dt =1
a. C
Review: Improper integrals.
Recall: Improper integral are defined as a limit.∫ ∞
t0
g(t) dt = limN→∞
∫ N
t0
g(t) dt.
I The integral converges iff the limit exists.
I The integral diverges iff the limit does not exist.
Example
Compute the improper integral
∫ ∞
0e−at dt, with a > 0.
Solution:
∫ ∞
0
e−at dt = limN→∞
∫ N
0
e−at dt = limN→∞
−1
a
(e−aN − 1
).
Since limN→∞
e−aN = 0 for a > 0, we conclude
∫ ∞
0
e−at dt =1
a. C
Review: Improper integrals.
Recall: Improper integral are defined as a limit.∫ ∞
t0
g(t) dt = limN→∞
∫ N
t0
g(t) dt.
I The integral converges iff the limit exists.
I The integral diverges iff the limit does not exist.
Example
Compute the improper integral
∫ ∞
0e−at dt, with a > 0.
Solution:
∫ ∞
0
e−at dt = limN→∞
∫ N
0
e−at dt = limN→∞
−1
a
(e−aN − 1
).
Since limN→∞
e−aN = 0 for a > 0, we conclude
∫ ∞
0
e−at dt =1
a. C
Review: Improper integrals.
Recall: Improper integral are defined as a limit.∫ ∞
t0
g(t) dt = limN→∞
∫ N
t0
g(t) dt.
I The integral converges iff the limit exists.
I The integral diverges iff the limit does not exist.
Example
Compute the improper integral
∫ ∞
0e−at dt, with a > 0.
Solution:
∫ ∞
0
e−at dt = limN→∞
∫ N
0
e−at dt = limN→∞
−1
a
(e−aN − 1
).
Since limN→∞
e−aN = 0 for a > 0, we conclude
∫ ∞
0
e−at dt =1
a. C
Review: Improper integrals.
Recall: Improper integral are defined as a limit.∫ ∞
t0
g(t) dt = limN→∞
∫ N
t0
g(t) dt.
I The integral converges iff the limit exists.
I The integral diverges iff the limit does not exist.
Example
Compute the improper integral
∫ ∞
0e−at dt, with a > 0.
Solution:
∫ ∞
0
e−at dt = limN→∞
∫ N
0
e−at dt
= limN→∞
−1
a
(e−aN − 1
).
Since limN→∞
e−aN = 0 for a > 0, we conclude
∫ ∞
0
e−at dt =1
a. C
Review: Improper integrals.
Recall: Improper integral are defined as a limit.∫ ∞
t0
g(t) dt = limN→∞
∫ N
t0
g(t) dt.
I The integral converges iff the limit exists.
I The integral diverges iff the limit does not exist.
Example
Compute the improper integral
∫ ∞
0e−at dt, with a > 0.
Solution:
∫ ∞
0
e−at dt = limN→∞
∫ N
0
e−at dt = limN→∞
−1
a
(e−aN − 1
).
Since limN→∞
e−aN = 0 for a > 0, we conclude
∫ ∞
0
e−at dt =1
a. C
Review: Improper integrals.
Recall: Improper integral are defined as a limit.∫ ∞
t0
g(t) dt = limN→∞
∫ N
t0
g(t) dt.
I The integral converges iff the limit exists.
I The integral diverges iff the limit does not exist.
Example
Compute the improper integral
∫ ∞
0e−at dt, with a > 0.
Solution:
∫ ∞
0
e−at dt = limN→∞
∫ N
0
e−at dt = limN→∞
−1
a
(e−aN − 1
).
Since limN→∞
e−aN = 0 for a > 0,
we conclude
∫ ∞
0
e−at dt =1
a. C
Review: Improper integrals.
Recall: Improper integral are defined as a limit.∫ ∞
t0
g(t) dt = limN→∞
∫ N
t0
g(t) dt.
I The integral converges iff the limit exists.
I The integral diverges iff the limit does not exist.
Example
Compute the improper integral
∫ ∞
0e−at dt, with a > 0.
Solution:
∫ ∞
0
e−at dt = limN→∞
∫ N
0
e−at dt = limN→∞
−1
a
(e−aN − 1
).
Since limN→∞
e−aN = 0 for a > 0, we conclude
∫ ∞
0
e−at dt =1
a. C
The Laplace Transform (Sect. 4.1).
I The definition of the Laplace Transform.
I Review: Improper integrals.
I Examples of Laplace Transforms.
I A table of Laplace Transforms.
I Properties of the Laplace Transform.
I Laplace Transform and differential equations.
Examples of Laplace Transforms.
Example
Compute L[1].
Solution: We have to find the Laplace Transform of f (t) = 1.Following the definition we obtain,
L[1] =
∫ ∞
0
e−st 1 dt =
∫ ∞
0
e−st dt
But
∫ ∞
0
e−at dt =1
afor a > 0, and diverges for a 6 0.
Therefore L[1] =1
s, for s > 0, and L[1] does not exists for s 6 0.
In other words, F (s) = L[1] is the function F : DF → R given by
f (t) = 1, F (s) =1
s, DF = (0,∞). C
Examples of Laplace Transforms.
Example
Compute L[1].
Solution: We have to find the Laplace Transform of f (t) = 1.
Following the definition we obtain,
L[1] =
∫ ∞
0
e−st 1 dt =
∫ ∞
0
e−st dt
But
∫ ∞
0
e−at dt =1
afor a > 0, and diverges for a 6 0.
Therefore L[1] =1
s, for s > 0, and L[1] does not exists for s 6 0.
In other words, F (s) = L[1] is the function F : DF → R given by
f (t) = 1, F (s) =1
s, DF = (0,∞). C
Examples of Laplace Transforms.
Example
Compute L[1].
Solution: We have to find the Laplace Transform of f (t) = 1.Following the definition we obtain,
L[1] =
∫ ∞
0
e−st 1 dt
=
∫ ∞
0
e−st dt
But
∫ ∞
0
e−at dt =1
afor a > 0, and diverges for a 6 0.
Therefore L[1] =1
s, for s > 0, and L[1] does not exists for s 6 0.
In other words, F (s) = L[1] is the function F : DF → R given by
f (t) = 1, F (s) =1
s, DF = (0,∞). C
Examples of Laplace Transforms.
Example
Compute L[1].
Solution: We have to find the Laplace Transform of f (t) = 1.Following the definition we obtain,
L[1] =
∫ ∞
0
e−st 1 dt =
∫ ∞
0
e−st dt
But
∫ ∞
0
e−at dt =1
afor a > 0, and diverges for a 6 0.
Therefore L[1] =1
s, for s > 0, and L[1] does not exists for s 6 0.
In other words, F (s) = L[1] is the function F : DF → R given by
f (t) = 1, F (s) =1
s, DF = (0,∞). C
Examples of Laplace Transforms.
Example
Compute L[1].
Solution: We have to find the Laplace Transform of f (t) = 1.Following the definition we obtain,
L[1] =
∫ ∞
0
e−st 1 dt =
∫ ∞
0
e−st dt
But
∫ ∞
0
e−at dt =1
afor a > 0,
and diverges for a 6 0.
Therefore L[1] =1
s, for s > 0, and L[1] does not exists for s 6 0.
In other words, F (s) = L[1] is the function F : DF → R given by
f (t) = 1, F (s) =1
s, DF = (0,∞). C
Examples of Laplace Transforms.
Example
Compute L[1].
Solution: We have to find the Laplace Transform of f (t) = 1.Following the definition we obtain,
L[1] =
∫ ∞
0
e−st 1 dt =
∫ ∞
0
e−st dt
But
∫ ∞
0
e−at dt =1
afor a > 0, and diverges for a 6 0.
Therefore L[1] =1
s, for s > 0, and L[1] does not exists for s 6 0.
In other words, F (s) = L[1] is the function F : DF → R given by
f (t) = 1, F (s) =1
s, DF = (0,∞). C
Examples of Laplace Transforms.
Example
Compute L[1].
Solution: We have to find the Laplace Transform of f (t) = 1.Following the definition we obtain,
L[1] =
∫ ∞
0
e−st 1 dt =
∫ ∞
0
e−st dt
But
∫ ∞
0
e−at dt =1
afor a > 0, and diverges for a 6 0.
Therefore L[1] =1
s, for s > 0,
and L[1] does not exists for s 6 0.
In other words, F (s) = L[1] is the function F : DF → R given by
f (t) = 1, F (s) =1
s, DF = (0,∞). C
Examples of Laplace Transforms.
Example
Compute L[1].
Solution: We have to find the Laplace Transform of f (t) = 1.Following the definition we obtain,
L[1] =
∫ ∞
0
e−st 1 dt =
∫ ∞
0
e−st dt
But
∫ ∞
0
e−at dt =1
afor a > 0, and diverges for a 6 0.
Therefore L[1] =1
s, for s > 0, and L[1] does not exists for s 6 0.
In other words, F (s) = L[1] is the function F : DF → R given by
f (t) = 1, F (s) =1
s, DF = (0,∞). C
Examples of Laplace Transforms.
Example
Compute L[1].
Solution: We have to find the Laplace Transform of f (t) = 1.Following the definition we obtain,
L[1] =
∫ ∞
0
e−st 1 dt =
∫ ∞
0
e−st dt
But
∫ ∞
0
e−at dt =1
afor a > 0, and diverges for a 6 0.
Therefore L[1] =1
s, for s > 0, and L[1] does not exists for s 6 0.
In other words, F (s) = L[1] is the function F : DF → R given by
f (t) = 1, F (s) =1
s, DF = (0,∞). C
Examples of Laplace Transforms.
Example
Compute L[eat ], where a ∈ R.
Solution: Following the definition of Laplace Transform,
L[eat ] =
∫ ∞
0
e−steat dt =
∫ ∞
0
e−(s−a)t dt.
We have seen that the improper integral is given by∫ ∞
0e−(s−a)t dt =
1
(s − a)for (s − a) > 0.
We conclude that L[eat ] =1
s − afor s > a. In other words,
f (t) = eat , F (s) =1
(s − a), s > a. C
Examples of Laplace Transforms.
Example
Compute L[eat ], where a ∈ R.
Solution: Following the definition of Laplace Transform,
L[eat ] =
∫ ∞
0
e−steat dt
=
∫ ∞
0
e−(s−a)t dt.
We have seen that the improper integral is given by∫ ∞
0e−(s−a)t dt =
1
(s − a)for (s − a) > 0.
We conclude that L[eat ] =1
s − afor s > a. In other words,
f (t) = eat , F (s) =1
(s − a), s > a. C
Examples of Laplace Transforms.
Example
Compute L[eat ], where a ∈ R.
Solution: Following the definition of Laplace Transform,
L[eat ] =
∫ ∞
0
e−steat dt =
∫ ∞
0
e−(s−a)t dt.
We have seen that the improper integral is given by∫ ∞
0e−(s−a)t dt =
1
(s − a)for (s − a) > 0.
We conclude that L[eat ] =1
s − afor s > a. In other words,
f (t) = eat , F (s) =1
(s − a), s > a. C
Examples of Laplace Transforms.
Example
Compute L[eat ], where a ∈ R.
Solution: Following the definition of Laplace Transform,
L[eat ] =
∫ ∞
0
e−steat dt =
∫ ∞
0
e−(s−a)t dt.
We have seen that the improper integral is given by∫ ∞
0e−(s−a)t dt =
1
(s − a)for (s − a) > 0.
We conclude that L[eat ] =1
s − afor s > a. In other words,
f (t) = eat , F (s) =1
(s − a), s > a. C
Examples of Laplace Transforms.
Example
Compute L[eat ], where a ∈ R.
Solution: Following the definition of Laplace Transform,
L[eat ] =
∫ ∞
0
e−steat dt =
∫ ∞
0
e−(s−a)t dt.
We have seen that the improper integral is given by∫ ∞
0e−(s−a)t dt =
1
(s − a)for (s − a) > 0.
We conclude that L[eat ] =1
s − afor s > a.
In other words,
f (t) = eat , F (s) =1
(s − a), s > a. C
Examples of Laplace Transforms.
Example
Compute L[eat ], where a ∈ R.
Solution: Following the definition of Laplace Transform,
L[eat ] =
∫ ∞
0
e−steat dt =
∫ ∞
0
e−(s−a)t dt.
We have seen that the improper integral is given by∫ ∞
0e−(s−a)t dt =
1
(s − a)for (s − a) > 0.
We conclude that L[eat ] =1
s − afor s > a. In other words,
f (t) = eat , F (s) =1
(s − a), s > a. C
Examples of Laplace Transforms.Example
Compute L[sin(at)], where a ∈ R.
Solution: In this case we need to compute
L[sin(at)] = limN→∞
∫ N
0
e−st sin(at) dt.
Integrating by parts twice it is not difficult to obtain:∫ N
0
e−st sin(at) dt =
−1
s
[e−st sin(at)
]∣∣∣N0
− a
s2
[e−st cos(at)
]∣∣∣N0
− a2
s2
∫ N
0
e−st sin(at) dt.
This identity implies(1 +
a2
s2
) ∫ N
0
e−st sin(at) dt = −1
s
[e−st sin(at)
]∣∣∣N0− a
s2
[e−st cos(at)
]∣∣∣N0.
Examples of Laplace Transforms.Example
Compute L[sin(at)], where a ∈ R.
Solution: In this case we need to compute
L[sin(at)] = limN→∞
∫ N
0
e−st sin(at) dt.
Integrating by parts twice it is not difficult to obtain:∫ N
0
e−st sin(at) dt =
−1
s
[e−st sin(at)
]∣∣∣N0
− a
s2
[e−st cos(at)
]∣∣∣N0
− a2
s2
∫ N
0
e−st sin(at) dt.
This identity implies(1 +
a2
s2
) ∫ N
0
e−st sin(at) dt = −1
s
[e−st sin(at)
]∣∣∣N0− a
s2
[e−st cos(at)
]∣∣∣N0.
Examples of Laplace Transforms.Example
Compute L[sin(at)], where a ∈ R.
Solution: In this case we need to compute
L[sin(at)] = limN→∞
∫ N
0
e−st sin(at) dt.
Integrating by parts twice it is not difficult to obtain:∫ N
0
e−st sin(at) dt =
−1
s
[e−st sin(at)
]∣∣∣N0
− a
s2
[e−st cos(at)
]∣∣∣N0
− a2
s2
∫ N
0
e−st sin(at) dt.
This identity implies(1 +
a2
s2
) ∫ N
0
e−st sin(at) dt = −1
s
[e−st sin(at)
]∣∣∣N0− a
s2
[e−st cos(at)
]∣∣∣N0.
Examples of Laplace Transforms.Example
Compute L[sin(at)], where a ∈ R.
Solution: In this case we need to compute
L[sin(at)] = limN→∞
∫ N
0
e−st sin(at) dt.
Integrating by parts twice it is not difficult to obtain:∫ N
0
e−st sin(at) dt =
−1
s
[e−st sin(at)
]∣∣∣N0
− a
s2
[e−st cos(at)
]∣∣∣N0
− a2
s2
∫ N
0
e−st sin(at) dt.
This identity implies(1 +
a2
s2
) ∫ N
0
e−st sin(at) dt = −1
s
[e−st sin(at)
]∣∣∣N0− a
s2
[e−st cos(at)
]∣∣∣N0.
Examples of Laplace Transforms.
Example
Compute L[sin(at)], where a ∈ R.
Solution: Recall the identity:(1 +
a2
s2
) ∫ N
0
e−st sin(at) dt = −1
s
[e−st sin(at)
]∣∣∣N0− a
s2
[e−st cos(at)
]∣∣∣N0.
Hence, it is not difficult to see that(s2 + a2
s2
) ∫ ∞
0
e−st sin(at) dt =a
s2, s > 0,
which is equivalent to
L[sin(at)] =a
s2 + a2, s > 0. C
Examples of Laplace Transforms.
Example
Compute L[sin(at)], where a ∈ R.
Solution: Recall the identity:(1 +
a2
s2
) ∫ N
0
e−st sin(at) dt = −1
s
[e−st sin(at)
]∣∣∣N0− a
s2
[e−st cos(at)
]∣∣∣N0.
Hence, it is not difficult to see that(s2 + a2
s2
) ∫ ∞
0
e−st sin(at) dt =a
s2, s > 0,
which is equivalent to
L[sin(at)] =a
s2 + a2, s > 0. C
Examples of Laplace Transforms.
Example
Compute L[sin(at)], where a ∈ R.
Solution: Recall the identity:(1 +
a2
s2
) ∫ N
0
e−st sin(at) dt = −1
s
[e−st sin(at)
]∣∣∣N0− a
s2
[e−st cos(at)
]∣∣∣N0.
Hence, it is not difficult to see that(s2 + a2
s2
) ∫ ∞
0
e−st sin(at) dt =a
s2, s > 0,
which is equivalent to
L[sin(at)] =a
s2 + a2, s > 0. C
The Laplace Transform (Sect. 4.1).
I The definition of the Laplace Transform.
I Review: Improper integrals.
I Examples of Laplace Transforms.
I A table of Laplace Transforms.
I Properties of the Laplace Transform.
I Laplace Transform and differential equations.
A table of Laplace Transforms.
f (t) = 1 F (s) =1
ss > 0,
f (t) = eat F (s) =1
s − as > max{a, 0},
f (t) = tn F (s) =n!
s(n+1)s > 0,
f (t) = sin(at) F (s) =a
s2 + a2s > 0,
f (t) = cos(at) F (s) =s
s2 + a2s > 0,
f (t) = sinh(at) F (s) =a
s2 − a2s > |a|,
f (t) = cosh(at) F (s) =s
s2 − a2s > |a|,
f (t) = tneat F (s) =n!
(s − a)(n+1)s > max{a, 0},
f (t) = eat sin(bt) F (s) =b
(s − a)2 + b2s > max{a, 0}.
The Laplace Transform (Sect. 4.1).
I The definition of the Laplace Transform.
I Review: Improper integrals.
I Examples of Laplace Transforms.
I A table of Laplace Transforms.
I Properties of the Laplace Transform.
I Laplace Transform and differential equations.
Properties of the Laplace Transform.
Theorem (Sufficient conditions)
If the function f : [0,∞) → R is piecewise continuous and thereexist positive constants k and a such that
|f (t)| 6 k eat ,
then the Laplace Transform of f exists for all s > a.
Theorem (Linear combination)
If the L[f ] and L[g ] are well-defined and a, b are constants, then
L[af + bg ] = aL[f ] + bL[g ].
Proof: Integration is a linear operation:∫[a f (t) + b g(t)] dt = a
∫f (t) dt + b
∫g(t) dt.
Properties of the Laplace Transform.
Theorem (Sufficient conditions)
If the function f : [0,∞) → R is piecewise continuous and thereexist positive constants k and a such that
|f (t)| 6 k eat ,
then the Laplace Transform of f exists for all s > a.
Theorem (Linear combination)
If the L[f ] and L[g ] are well-defined and a, b are constants, then
L[af + bg ] = aL[f ] + bL[g ].
Proof: Integration is a linear operation:∫[a f (t) + b g(t)] dt = a
∫f (t) dt + b
∫g(t) dt.
Properties of the Laplace Transform.
Theorem (Sufficient conditions)
If the function f : [0,∞) → R is piecewise continuous and thereexist positive constants k and a such that
|f (t)| 6 k eat ,
then the Laplace Transform of f exists for all s > a.
Theorem (Linear combination)
If the L[f ] and L[g ] are well-defined and a, b are constants, then
L[af + bg ] = aL[f ] + bL[g ].
Proof: Integration is a linear operation:
∫[a f (t) + b g(t)] dt = a
∫f (t) dt + b
∫g(t) dt.
Properties of the Laplace Transform.
Theorem (Sufficient conditions)
If the function f : [0,∞) → R is piecewise continuous and thereexist positive constants k and a such that
|f (t)| 6 k eat ,
then the Laplace Transform of f exists for all s > a.
Theorem (Linear combination)
If the L[f ] and L[g ] are well-defined and a, b are constants, then
L[af + bg ] = aL[f ] + bL[g ].
Proof: Integration is a linear operation:∫[a f (t) + b g(t)] dt = a
∫f (t) dt + b
∫g(t) dt.
Properties of the Laplace Transform.
Theorem (Derivatives)
If the L[f ] and L[f ′] are well-defined, then holds,
L[f ′] = s L[f ]− f (0). (1)
Furthermore, if L[f ′′] is well-defined, then it also holds
L[f ′′] = s2 L[f ]− s f (0)− f ′(0). (2)
Proof of Eq (2): Use Eq. (1) twice:
L[f ′′] = L[(f ′)′] = sL[(f ′)]− f ′(0) = s(sL[f ]− f (0)
)− f ′(0),
that is,L[f ′′] = s2 L[f ]− s f (0)− f ′(0).
Properties of the Laplace Transform.
Theorem (Derivatives)
If the L[f ] and L[f ′] are well-defined, then holds,
L[f ′] = s L[f ]− f (0). (1)
Furthermore, if L[f ′′] is well-defined, then it also holds
L[f ′′] = s2 L[f ]− s f (0)− f ′(0). (2)
Proof of Eq (2):
Use Eq. (1) twice:
L[f ′′] = L[(f ′)′] = sL[(f ′)]− f ′(0) = s(sL[f ]− f (0)
)− f ′(0),
that is,L[f ′′] = s2 L[f ]− s f (0)− f ′(0).
Properties of the Laplace Transform.
Theorem (Derivatives)
If the L[f ] and L[f ′] are well-defined, then holds,
L[f ′] = s L[f ]− f (0). (1)
Furthermore, if L[f ′′] is well-defined, then it also holds
L[f ′′] = s2 L[f ]− s f (0)− f ′(0). (2)
Proof of Eq (2): Use Eq. (1) twice:
L[f ′′] = L[(f ′)′] = sL[(f ′)]− f ′(0) = s(sL[f ]− f (0)
)− f ′(0),
that is,L[f ′′] = s2 L[f ]− s f (0)− f ′(0).
Properties of the Laplace Transform.
Theorem (Derivatives)
If the L[f ] and L[f ′] are well-defined, then holds,
L[f ′] = s L[f ]− f (0). (1)
Furthermore, if L[f ′′] is well-defined, then it also holds
L[f ′′] = s2 L[f ]− s f (0)− f ′(0). (2)
Proof of Eq (2): Use Eq. (1) twice:
L[f ′′] = L[(f ′)′]
= sL[(f ′)]− f ′(0) = s(sL[f ]− f (0)
)− f ′(0),
that is,L[f ′′] = s2 L[f ]− s f (0)− f ′(0).
Properties of the Laplace Transform.
Theorem (Derivatives)
If the L[f ] and L[f ′] are well-defined, then holds,
L[f ′] = s L[f ]− f (0). (1)
Furthermore, if L[f ′′] is well-defined, then it also holds
L[f ′′] = s2 L[f ]− s f (0)− f ′(0). (2)
Proof of Eq (2): Use Eq. (1) twice:
L[f ′′] = L[(f ′)′] = sL[(f ′)]− f ′(0)
= s(sL[f ]− f (0)
)− f ′(0),
that is,L[f ′′] = s2 L[f ]− s f (0)− f ′(0).
Properties of the Laplace Transform.
Theorem (Derivatives)
If the L[f ] and L[f ′] are well-defined, then holds,
L[f ′] = s L[f ]− f (0). (1)
Furthermore, if L[f ′′] is well-defined, then it also holds
L[f ′′] = s2 L[f ]− s f (0)− f ′(0). (2)
Proof of Eq (2): Use Eq. (1) twice:
L[f ′′] = L[(f ′)′] = sL[(f ′)]− f ′(0) = s(sL[f ]− f (0)
)− f ′(0),
that is,L[f ′′] = s2 L[f ]− s f (0)− f ′(0).
Properties of the Laplace Transform.
Theorem (Derivatives)
If the L[f ] and L[f ′] are well-defined, then holds,
L[f ′] = s L[f ]− f (0). (1)
Furthermore, if L[f ′′] is well-defined, then it also holds
L[f ′′] = s2 L[f ]− s f (0)− f ′(0). (2)
Proof of Eq (2): Use Eq. (1) twice:
L[f ′′] = L[(f ′)′] = sL[(f ′)]− f ′(0) = s(sL[f ]− f (0)
)− f ′(0),
that is,L[f ′′] = s2 L[f ]− s f (0)− f ′(0).
Properties of the Laplace Transform.
Proof of Eq (1): Recall the definition of the Laplace Transform,
L[f ′] =
∫ ∞
0
e−st f ′(t) dt
= limn→∞
∫ n
0
e−st f ′(t) dt
Integrating by parts,
limn→∞
∫ n
0
e−st f ′(t) dt = limn→∞
[(e−st f (t)
)∣∣∣n0
−∫ n
0
(−s)e−st f (t) dt]
L[f ′] = limn→∞
[e−snf (n)−f (0)
]+s
∫ ∞
0
e−st f (t) dt = −f (0)+s L[f ],
where we used that limn→∞ e−snf (n) = 0 for s big enough, and wealso used that L[f ] is well-defined.
We then conclude that L[f ′] = s L[f ]− f (0).
Properties of the Laplace Transform.
Proof of Eq (1): Recall the definition of the Laplace Transform,
L[f ′] =
∫ ∞
0
e−st f ′(t) dt = limn→∞
∫ n
0
e−st f ′(t) dt
Integrating by parts,
limn→∞
∫ n
0
e−st f ′(t) dt = limn→∞
[(e−st f (t)
)∣∣∣n0
−∫ n
0
(−s)e−st f (t) dt]
L[f ′] = limn→∞
[e−snf (n)−f (0)
]+s
∫ ∞
0
e−st f (t) dt = −f (0)+s L[f ],
where we used that limn→∞ e−snf (n) = 0 for s big enough, and wealso used that L[f ] is well-defined.
We then conclude that L[f ′] = s L[f ]− f (0).
Properties of the Laplace Transform.
Proof of Eq (1): Recall the definition of the Laplace Transform,
L[f ′] =
∫ ∞
0
e−st f ′(t) dt = limn→∞
∫ n
0
e−st f ′(t) dt
Integrating by parts,
limn→∞
∫ n
0
e−st f ′(t) dt = limn→∞
[(e−st f (t)
)∣∣∣n0
−∫ n
0
(−s)e−st f (t) dt]
L[f ′] = limn→∞
[e−snf (n)−f (0)
]+s
∫ ∞
0
e−st f (t) dt = −f (0)+s L[f ],
where we used that limn→∞ e−snf (n) = 0 for s big enough, and wealso used that L[f ] is well-defined.
We then conclude that L[f ′] = s L[f ]− f (0).
Properties of the Laplace Transform.
Proof of Eq (1): Recall the definition of the Laplace Transform,
L[f ′] =
∫ ∞
0
e−st f ′(t) dt = limn→∞
∫ n
0
e−st f ′(t) dt
Integrating by parts,
limn→∞
∫ n
0
e−st f ′(t) dt = limn→∞
[(e−st f (t)
)∣∣∣n0
−∫ n
0
(−s)e−st f (t) dt]
L[f ′] = limn→∞
[e−snf (n)−f (0)
]+s
∫ ∞
0
e−st f (t) dt
= −f (0)+s L[f ],
where we used that limn→∞ e−snf (n) = 0 for s big enough, and wealso used that L[f ] is well-defined.
We then conclude that L[f ′] = s L[f ]− f (0).
Properties of the Laplace Transform.
Proof of Eq (1): Recall the definition of the Laplace Transform,
L[f ′] =
∫ ∞
0
e−st f ′(t) dt = limn→∞
∫ n
0
e−st f ′(t) dt
Integrating by parts,
limn→∞
∫ n
0
e−st f ′(t) dt = limn→∞
[(e−st f (t)
)∣∣∣n0
−∫ n
0
(−s)e−st f (t) dt]
L[f ′] = limn→∞
[e−snf (n)−f (0)
]+s
∫ ∞
0
e−st f (t) dt = −f (0)+s L[f ],
where we used that limn→∞ e−snf (n) = 0 for s big enough, and wealso used that L[f ] is well-defined.
We then conclude that L[f ′] = s L[f ]− f (0).
Properties of the Laplace Transform.
Proof of Eq (1): Recall the definition of the Laplace Transform,
L[f ′] =
∫ ∞
0
e−st f ′(t) dt = limn→∞
∫ n
0
e−st f ′(t) dt
Integrating by parts,
limn→∞
∫ n
0
e−st f ′(t) dt = limn→∞
[(e−st f (t)
)∣∣∣n0
−∫ n
0
(−s)e−st f (t) dt]
L[f ′] = limn→∞
[e−snf (n)−f (0)
]+s
∫ ∞
0
e−st f (t) dt = −f (0)+s L[f ],
where we used that limn→∞ e−snf (n) = 0 for s big enough,
and wealso used that L[f ] is well-defined.
We then conclude that L[f ′] = s L[f ]− f (0).
Properties of the Laplace Transform.
Proof of Eq (1): Recall the definition of the Laplace Transform,
L[f ′] =
∫ ∞
0
e−st f ′(t) dt = limn→∞
∫ n
0
e−st f ′(t) dt
Integrating by parts,
limn→∞
∫ n
0
e−st f ′(t) dt = limn→∞
[(e−st f (t)
)∣∣∣n0
−∫ n
0
(−s)e−st f (t) dt]
L[f ′] = limn→∞
[e−snf (n)−f (0)
]+s
∫ ∞
0
e−st f (t) dt = −f (0)+s L[f ],
where we used that limn→∞ e−snf (n) = 0 for s big enough, and wealso used that L[f ] is well-defined.
We then conclude that L[f ′] = s L[f ]− f (0).
Properties of the Laplace Transform.
Proof of Eq (1): Recall the definition of the Laplace Transform,
L[f ′] =
∫ ∞
0
e−st f ′(t) dt = limn→∞
∫ n
0
e−st f ′(t) dt
Integrating by parts,
limn→∞
∫ n
0
e−st f ′(t) dt = limn→∞
[(e−st f (t)
)∣∣∣n0
−∫ n
0
(−s)e−st f (t) dt]
L[f ′] = limn→∞
[e−snf (n)−f (0)
]+s
∫ ∞
0
e−st f (t) dt = −f (0)+s L[f ],
where we used that limn→∞ e−snf (n) = 0 for s big enough, and wealso used that L[f ] is well-defined.
We then conclude that L[f ′] = s L[f ]− f (0).
The Laplace Transform (Sect. 4.1).
I The definition of the Laplace Transform.
I Review: Improper integrals.
I Examples of Laplace Transforms.
I A table of Laplace Transforms.
I Properties of the Laplace Transform.
I Laplace Transform and differential equations.
Laplace Transform and differential equations.
Remark: Laplace Transforms can be used to find solutions todifferential equations with constant coefficients.
Idea of the method:
L
[Differential Eq.
for y(t).
](1)−→
Algebraic Eq.
for L[y(t)].
(2)−→
(2)−→Solve the
Algebraic Eq.
for L[y(t)].
(3)−→Transform back
to obtain y(t).
(Using the table.)
Laplace Transform and differential equations.
Remark: Laplace Transforms can be used to find solutions todifferential equations with constant coefficients.
Idea of the method:
L
[Differential Eq.
for y(t).
](1)−→
Algebraic Eq.
for L[y(t)].
(2)−→
(2)−→Solve the
Algebraic Eq.
for L[y(t)].
(3)−→Transform back
to obtain y(t).
(Using the table.)
Laplace Transform and differential equations.
Remark: Laplace Transforms can be used to find solutions todifferential equations with constant coefficients.
Idea of the method:
L
[Differential Eq.
for y(t).
]
(1)−→Algebraic Eq.
for L[y(t)].
(2)−→
(2)−→Solve the
Algebraic Eq.
for L[y(t)].
(3)−→Transform back
to obtain y(t).
(Using the table.)
Laplace Transform and differential equations.
Remark: Laplace Transforms can be used to find solutions todifferential equations with constant coefficients.
Idea of the method:
L
[Differential Eq.
for y(t).
](1)−→
Algebraic Eq.
for L[y(t)].
(2)−→
(2)−→Solve the
Algebraic Eq.
for L[y(t)].
(3)−→Transform back
to obtain y(t).
(Using the table.)
Laplace Transform and differential equations.
Remark: Laplace Transforms can be used to find solutions todifferential equations with constant coefficients.
Idea of the method:
L
[Differential Eq.
for y(t).
](1)−→
Algebraic Eq.
for L[y(t)].
(2)−→
(2)−→Solve the
Algebraic Eq.
for L[y(t)].
(3)−→Transform back
to obtain y(t).
(Using the table.)
Laplace Transform and differential equations.
Remark: Laplace Transforms can be used to find solutions todifferential equations with constant coefficients.
Idea of the method:
L
[Differential Eq.
for y(t).
](1)−→
Algebraic Eq.
for L[y(t)].
(2)−→
(2)−→Solve the
Algebraic Eq.
for L[y(t)].
(3)−→Transform back
to obtain y(t).
(Using the table.)
Laplace Transform and differential equations.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′ + 2y = 0, y(0) = 3.
Solution: We know the solution: y(t) = 3e−2t .
(1): Compute the Laplace transform of the differential equation,
L[y ′ + 2y ] = L[0] ⇒ L[y ′ + 2y ] = 0.
Find an algebraic equation for L[y ]. Recall linearity:
L[y ′] + 2L[y ] = 0.
Also recall the property: L[y ′] = s L[y ]− y(0), that is,[s L[y ]− y(0)
]+ 2L[y ] = 0 ⇒ (s + 2)L[y ] = y(0).
Laplace Transform and differential equations.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′ + 2y = 0, y(0) = 3.
Solution: We know the solution: y(t) = 3e−2t .
(1): Compute the Laplace transform of the differential equation,
L[y ′ + 2y ] = L[0] ⇒ L[y ′ + 2y ] = 0.
Find an algebraic equation for L[y ]. Recall linearity:
L[y ′] + 2L[y ] = 0.
Also recall the property: L[y ′] = s L[y ]− y(0), that is,[s L[y ]− y(0)
]+ 2L[y ] = 0 ⇒ (s + 2)L[y ] = y(0).
Laplace Transform and differential equations.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′ + 2y = 0, y(0) = 3.
Solution: We know the solution: y(t) = 3e−2t .
(1): Compute the Laplace transform of the differential equation,
L[y ′ + 2y ] = L[0]
⇒ L[y ′ + 2y ] = 0.
Find an algebraic equation for L[y ]. Recall linearity:
L[y ′] + 2L[y ] = 0.
Also recall the property: L[y ′] = s L[y ]− y(0), that is,[s L[y ]− y(0)
]+ 2L[y ] = 0 ⇒ (s + 2)L[y ] = y(0).
Laplace Transform and differential equations.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′ + 2y = 0, y(0) = 3.
Solution: We know the solution: y(t) = 3e−2t .
(1): Compute the Laplace transform of the differential equation,
L[y ′ + 2y ] = L[0] ⇒ L[y ′ + 2y ] = 0.
Find an algebraic equation for L[y ]. Recall linearity:
L[y ′] + 2L[y ] = 0.
Also recall the property: L[y ′] = s L[y ]− y(0), that is,[s L[y ]− y(0)
]+ 2L[y ] = 0 ⇒ (s + 2)L[y ] = y(0).
Laplace Transform and differential equations.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′ + 2y = 0, y(0) = 3.
Solution: We know the solution: y(t) = 3e−2t .
(1): Compute the Laplace transform of the differential equation,
L[y ′ + 2y ] = L[0] ⇒ L[y ′ + 2y ] = 0.
Find an algebraic equation for L[y ].
Recall linearity:
L[y ′] + 2L[y ] = 0.
Also recall the property: L[y ′] = s L[y ]− y(0), that is,[s L[y ]− y(0)
]+ 2L[y ] = 0 ⇒ (s + 2)L[y ] = y(0).
Laplace Transform and differential equations.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′ + 2y = 0, y(0) = 3.
Solution: We know the solution: y(t) = 3e−2t .
(1): Compute the Laplace transform of the differential equation,
L[y ′ + 2y ] = L[0] ⇒ L[y ′ + 2y ] = 0.
Find an algebraic equation for L[y ]. Recall linearity:
L[y ′] + 2L[y ] = 0.
Also recall the property: L[y ′] = s L[y ]− y(0), that is,[s L[y ]− y(0)
]+ 2L[y ] = 0 ⇒ (s + 2)L[y ] = y(0).
Laplace Transform and differential equations.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′ + 2y = 0, y(0) = 3.
Solution: We know the solution: y(t) = 3e−2t .
(1): Compute the Laplace transform of the differential equation,
L[y ′ + 2y ] = L[0] ⇒ L[y ′ + 2y ] = 0.
Find an algebraic equation for L[y ]. Recall linearity:
L[y ′] + 2L[y ] = 0.
Also recall the property: L[y ′] = s L[y ]− y(0),
that is,[s L[y ]− y(0)
]+ 2L[y ] = 0 ⇒ (s + 2)L[y ] = y(0).
Laplace Transform and differential equations.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′ + 2y = 0, y(0) = 3.
Solution: We know the solution: y(t) = 3e−2t .
(1): Compute the Laplace transform of the differential equation,
L[y ′ + 2y ] = L[0] ⇒ L[y ′ + 2y ] = 0.
Find an algebraic equation for L[y ]. Recall linearity:
L[y ′] + 2L[y ] = 0.
Also recall the property: L[y ′] = s L[y ]− y(0), that is,[s L[y ]− y(0)
]+ 2L[y ] = 0 ⇒ (s + 2)L[y ] = y(0).
Laplace Transform and differential equations.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′ + 2y = 0, y(0) = 3.
Solution: Recall: (s + 2)L[y ] = y(0).
(2): Solve the algebraic equation for L[y ].
L[y ] =y(0)
s + 2, y(0) = 3, ⇒ L[y ] =
3
s + 2.
(3): Transform back to y(t). From the table:
L[eat ] =1
s − a⇒ 3
s + 2= 3L[e−2t ] ⇒ 3
s + 2= L[3e−2t ].
Hence, L[y ] = L[3e−2t ] ⇒ y(t) = 3e−2t . C
Laplace Transform and differential equations.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′ + 2y = 0, y(0) = 3.
Solution: Recall: (s + 2)L[y ] = y(0).
(2): Solve the algebraic equation for L[y ].
L[y ] =y(0)
s + 2, y(0) = 3, ⇒ L[y ] =
3
s + 2.
(3): Transform back to y(t). From the table:
L[eat ] =1
s − a⇒ 3
s + 2= 3L[e−2t ] ⇒ 3
s + 2= L[3e−2t ].
Hence, L[y ] = L[3e−2t ] ⇒ y(t) = 3e−2t . C
Laplace Transform and differential equations.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′ + 2y = 0, y(0) = 3.
Solution: Recall: (s + 2)L[y ] = y(0).
(2): Solve the algebraic equation for L[y ].
L[y ] =y(0)
s + 2,
y(0) = 3, ⇒ L[y ] =3
s + 2.
(3): Transform back to y(t). From the table:
L[eat ] =1
s − a⇒ 3
s + 2= 3L[e−2t ] ⇒ 3
s + 2= L[3e−2t ].
Hence, L[y ] = L[3e−2t ] ⇒ y(t) = 3e−2t . C
Laplace Transform and differential equations.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′ + 2y = 0, y(0) = 3.
Solution: Recall: (s + 2)L[y ] = y(0).
(2): Solve the algebraic equation for L[y ].
L[y ] =y(0)
s + 2, y(0) = 3,
⇒ L[y ] =3
s + 2.
(3): Transform back to y(t). From the table:
L[eat ] =1
s − a⇒ 3
s + 2= 3L[e−2t ] ⇒ 3
s + 2= L[3e−2t ].
Hence, L[y ] = L[3e−2t ] ⇒ y(t) = 3e−2t . C
Laplace Transform and differential equations.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′ + 2y = 0, y(0) = 3.
Solution: Recall: (s + 2)L[y ] = y(0).
(2): Solve the algebraic equation for L[y ].
L[y ] =y(0)
s + 2, y(0) = 3, ⇒ L[y ] =
3
s + 2.
(3): Transform back to y(t). From the table:
L[eat ] =1
s − a⇒ 3
s + 2= 3L[e−2t ] ⇒ 3
s + 2= L[3e−2t ].
Hence, L[y ] = L[3e−2t ] ⇒ y(t) = 3e−2t . C
Laplace Transform and differential equations.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′ + 2y = 0, y(0) = 3.
Solution: Recall: (s + 2)L[y ] = y(0).
(2): Solve the algebraic equation for L[y ].
L[y ] =y(0)
s + 2, y(0) = 3, ⇒ L[y ] =
3
s + 2.
(3): Transform back to y(t).
From the table:
L[eat ] =1
s − a⇒ 3
s + 2= 3L[e−2t ] ⇒ 3
s + 2= L[3e−2t ].
Hence, L[y ] = L[3e−2t ] ⇒ y(t) = 3e−2t . C
Laplace Transform and differential equations.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′ + 2y = 0, y(0) = 3.
Solution: Recall: (s + 2)L[y ] = y(0).
(2): Solve the algebraic equation for L[y ].
L[y ] =y(0)
s + 2, y(0) = 3, ⇒ L[y ] =
3
s + 2.
(3): Transform back to y(t). From the table:
L[eat ] =1
s − a
⇒ 3
s + 2= 3L[e−2t ] ⇒ 3
s + 2= L[3e−2t ].
Hence, L[y ] = L[3e−2t ] ⇒ y(t) = 3e−2t . C
Laplace Transform and differential equations.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′ + 2y = 0, y(0) = 3.
Solution: Recall: (s + 2)L[y ] = y(0).
(2): Solve the algebraic equation for L[y ].
L[y ] =y(0)
s + 2, y(0) = 3, ⇒ L[y ] =
3
s + 2.
(3): Transform back to y(t). From the table:
L[eat ] =1
s − a⇒ 3
s + 2= 3L[e−2t ]
⇒ 3
s + 2= L[3e−2t ].
Hence, L[y ] = L[3e−2t ] ⇒ y(t) = 3e−2t . C
Laplace Transform and differential equations.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′ + 2y = 0, y(0) = 3.
Solution: Recall: (s + 2)L[y ] = y(0).
(2): Solve the algebraic equation for L[y ].
L[y ] =y(0)
s + 2, y(0) = 3, ⇒ L[y ] =
3
s + 2.
(3): Transform back to y(t). From the table:
L[eat ] =1
s − a⇒ 3
s + 2= 3L[e−2t ] ⇒ 3
s + 2= L[3e−2t ].
Hence, L[y ] = L[3e−2t ] ⇒ y(t) = 3e−2t . C
Laplace Transform and differential equations.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′ + 2y = 0, y(0) = 3.
Solution: Recall: (s + 2)L[y ] = y(0).
(2): Solve the algebraic equation for L[y ].
L[y ] =y(0)
s + 2, y(0) = 3, ⇒ L[y ] =
3
s + 2.
(3): Transform back to y(t). From the table:
L[eat ] =1
s − a⇒ 3
s + 2= 3L[e−2t ] ⇒ 3
s + 2= L[3e−2t ].
Hence, L[y ] = L[3e−2t ]
⇒ y(t) = 3e−2t . C
Laplace Transform and differential equations.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′ + 2y = 0, y(0) = 3.
Solution: Recall: (s + 2)L[y ] = y(0).
(2): Solve the algebraic equation for L[y ].
L[y ] =y(0)
s + 2, y(0) = 3, ⇒ L[y ] =
3
s + 2.
(3): Transform back to y(t). From the table:
L[eat ] =1
s − a⇒ 3
s + 2= 3L[e−2t ] ⇒ 3
s + 2= L[3e−2t ].
Hence, L[y ] = L[3e−2t ] ⇒ y(t) = 3e−2t . C
The Laplace Transform and the IVP (Sect. 4.2).
I Solving differential equations using L[ ].I Homogeneous IVP.I First, second, higher order equations.I Non-homogeneous IVP.
Solving differential equations using L[ ].
Remark: The method works with:
I Constant coefficient equations.
I Homogeneous and non-homogeneous equations.
I First, second, higher order equations.
Idea of the method:
L
[Differential Eq.
for y(t).
](1)−→
Algebraic Eq.
for L[y(t)].
(2)−→
(2)−→Solve the
Algebraic Eq.
for L[y(t)].
(3)−→Transform back
to obtain y(t).
(Using the table.)
Solving differential equations using L[ ].
Remark: The method works with:
I Constant coefficient equations.
I Homogeneous and non-homogeneous equations.
I First, second, higher order equations.
Idea of the method:
L
[Differential Eq.
for y(t).
](1)−→
Algebraic Eq.
for L[y(t)].
(2)−→
(2)−→Solve the
Algebraic Eq.
for L[y(t)].
(3)−→Transform back
to obtain y(t).
(Using the table.)
Solving differential equations using L[ ].
Remark: The method works with:
I Constant coefficient equations.
I Homogeneous and non-homogeneous equations.
I First, second, higher order equations.
Idea of the method:
L
[Differential Eq.
for y(t).
](1)−→
Algebraic Eq.
for L[y(t)].
(2)−→
(2)−→Solve the
Algebraic Eq.
for L[y(t)].
(3)−→Transform back
to obtain y(t).
(Using the table.)
Solving differential equations using L[ ].
Remark: The method works with:
I Constant coefficient equations.
I Homogeneous and non-homogeneous equations.
I First, second, higher order equations.
Idea of the method:
L
[Differential Eq.
for y(t).
](1)−→
Algebraic Eq.
for L[y(t)].
(2)−→
(2)−→Solve the
Algebraic Eq.
for L[y(t)].
(3)−→Transform back
to obtain y(t).
(Using the table.)
Solving differential equations using L[ ].
Remark: The method works with:
I Constant coefficient equations.
I Homogeneous and non-homogeneous equations.
I First, second, higher order equations.
Idea of the method:
L
[Differential Eq.
for y(t).
](1)−→
Algebraic Eq.
for L[y(t)].
(2)−→
(2)−→Solve the
Algebraic Eq.
for L[y(t)].
(3)−→Transform back
to obtain y(t).
(Using the table.)
Solving differential equations using L[ ].
Remark: The method works with:
I Constant coefficient equations.
I Homogeneous and non-homogeneous equations.
I First, second, higher order equations.
Idea of the method:
L
[Differential Eq.
for y(t).
]
(1)−→Algebraic Eq.
for L[y(t)].
(2)−→
(2)−→Solve the
Algebraic Eq.
for L[y(t)].
(3)−→Transform back
to obtain y(t).
(Using the table.)
Solving differential equations using L[ ].
Remark: The method works with:
I Constant coefficient equations.
I Homogeneous and non-homogeneous equations.
I First, second, higher order equations.
Idea of the method:
L
[Differential Eq.
for y(t).
](1)−→
Algebraic Eq.
for L[y(t)].
(2)−→
(2)−→Solve the
Algebraic Eq.
for L[y(t)].
(3)−→Transform back
to obtain y(t).
(Using the table.)
Solving differential equations using L[ ].
Remark: The method works with:
I Constant coefficient equations.
I Homogeneous and non-homogeneous equations.
I First, second, higher order equations.
Idea of the method:
L
[Differential Eq.
for y(t).
](1)−→
Algebraic Eq.
for L[y(t)].
(2)−→
(2)−→Solve the
Algebraic Eq.
for L[y(t)].
(3)−→Transform back
to obtain y(t).
(Using the table.)
Solving differential equations using L[ ].
Remark: The method works with:
I Constant coefficient equations.
I Homogeneous and non-homogeneous equations.
I First, second, higher order equations.
Idea of the method:
L
[Differential Eq.
for y(t).
](1)−→
Algebraic Eq.
for L[y(t)].
(2)−→
(2)−→Solve the
Algebraic Eq.
for L[y(t)].
(3)−→Transform back
to obtain y(t).
(Using the table.)
Solving differential equations using L[ ].
Idea of the method:
L
[Differential Eq.
for y(t).
](1)−→
Algebraic Eq.
for L[y(t)].
(2)−→
(2)−→Solve the
Algebraic Eq.
for L[y(t)].
(3)−→Transform back
to obtain y(t).
(Using the table.)
Recall:
(a) L[a f (t) + b g(t)] = aL[f (t)] + bL[g(t)];
(b) L[y (n)
]= sn L[y ]− s(n−1) y(0)− s(n−2) y ′(0)−· · ·−y (n−1)(0).
Solving differential equations using L[ ].
Idea of the method:
L
[Differential Eq.
for y(t).
](1)−→
Algebraic Eq.
for L[y(t)].
(2)−→
(2)−→Solve the
Algebraic Eq.
for L[y(t)].
(3)−→Transform back
to obtain y(t).
(Using the table.)
Recall:
(a) L[a f (t) + b g(t)] = aL[f (t)] + bL[g(t)];
(b) L[y (n)
]= sn L[y ]− s(n−1) y(0)− s(n−2) y ′(0)−· · ·−y (n−1)(0).
Solving differential equations using L[ ].
Idea of the method:
L
[Differential Eq.
for y(t).
](1)−→
Algebraic Eq.
for L[y(t)].
(2)−→
(2)−→Solve the
Algebraic Eq.
for L[y(t)].
(3)−→Transform back
to obtain y(t).
(Using the table.)
Recall:
(a) L[a f (t) + b g(t)] = aL[f (t)] + bL[g(t)];
(b) L[y (n)
]= sn L[y ]− s(n−1) y(0)− s(n−2) y ′(0)−· · ·−y (n−1)(0).
The Laplace Transform and the IVP (Sect. 4.2).
I Solving differential equations using L[ ].I Homogeneous IVP.I First, second, higher order equations.I Non-homogeneous IVP.
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Compute the L[ ] of the differential equation,
L[y ′′ − y ′ − 2y ] = L[0] ⇒ L[y ′′ − y ′ − 2y ] = 0.
The L[ ] is a linear function, so
L[y ′′]− L[y ′]− 2L[y ] = 0.
Derivatives are transformed into power functions,[s2 L[y ]− s y(0)− y ′(0)
]−
[s L[y ]− y(0)
]− 2L[y ] = 0,
We the obtain (s2 − s − 2)L[y ] = (s − 1) y(0) + y ′(0).
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Compute the L[ ] of the differential equation,
L[y ′′ − y ′ − 2y ] = L[0] ⇒ L[y ′′ − y ′ − 2y ] = 0.
The L[ ] is a linear function, so
L[y ′′]− L[y ′]− 2L[y ] = 0.
Derivatives are transformed into power functions,[s2 L[y ]− s y(0)− y ′(0)
]−
[s L[y ]− y(0)
]− 2L[y ] = 0,
We the obtain (s2 − s − 2)L[y ] = (s − 1) y(0) + y ′(0).
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Compute the L[ ] of the differential equation,
L[y ′′ − y ′ − 2y ] = L[0]
⇒ L[y ′′ − y ′ − 2y ] = 0.
The L[ ] is a linear function, so
L[y ′′]− L[y ′]− 2L[y ] = 0.
Derivatives are transformed into power functions,[s2 L[y ]− s y(0)− y ′(0)
]−
[s L[y ]− y(0)
]− 2L[y ] = 0,
We the obtain (s2 − s − 2)L[y ] = (s − 1) y(0) + y ′(0).
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Compute the L[ ] of the differential equation,
L[y ′′ − y ′ − 2y ] = L[0] ⇒ L[y ′′ − y ′ − 2y ] = 0.
The L[ ] is a linear function, so
L[y ′′]− L[y ′]− 2L[y ] = 0.
Derivatives are transformed into power functions,[s2 L[y ]− s y(0)− y ′(0)
]−
[s L[y ]− y(0)
]− 2L[y ] = 0,
We the obtain (s2 − s − 2)L[y ] = (s − 1) y(0) + y ′(0).
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Compute the L[ ] of the differential equation,
L[y ′′ − y ′ − 2y ] = L[0] ⇒ L[y ′′ − y ′ − 2y ] = 0.
The L[ ] is a linear function,
so
L[y ′′]− L[y ′]− 2L[y ] = 0.
Derivatives are transformed into power functions,[s2 L[y ]− s y(0)− y ′(0)
]−
[s L[y ]− y(0)
]− 2L[y ] = 0,
We the obtain (s2 − s − 2)L[y ] = (s − 1) y(0) + y ′(0).
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Compute the L[ ] of the differential equation,
L[y ′′ − y ′ − 2y ] = L[0] ⇒ L[y ′′ − y ′ − 2y ] = 0.
The L[ ] is a linear function, so
L[y ′′]− L[y ′]− 2L[y ] = 0.
Derivatives are transformed into power functions,[s2 L[y ]− s y(0)− y ′(0)
]−
[s L[y ]− y(0)
]− 2L[y ] = 0,
We the obtain (s2 − s − 2)L[y ] = (s − 1) y(0) + y ′(0).
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Compute the L[ ] of the differential equation,
L[y ′′ − y ′ − 2y ] = L[0] ⇒ L[y ′′ − y ′ − 2y ] = 0.
The L[ ] is a linear function, so
L[y ′′]− L[y ′]− 2L[y ] = 0.
Derivatives are transformed into power functions,[s2 L[y ]− s y(0)− y ′(0)
]−
[s L[y ]− y(0)
]− 2L[y ] = 0,
We the obtain (s2 − s − 2)L[y ] = (s − 1) y(0) + y ′(0).
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Compute the L[ ] of the differential equation,
L[y ′′ − y ′ − 2y ] = L[0] ⇒ L[y ′′ − y ′ − 2y ] = 0.
The L[ ] is a linear function, so
L[y ′′]− L[y ′]− 2L[y ] = 0.
Derivatives are transformed into power functions,[s2 L[y ]− s y(0)− y ′(0)
]−
[s L[y ]− y(0)
]− 2L[y ] = 0,
We the obtain (s2 − s − 2)L[y ] = (s − 1) y(0) + y ′(0).
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Recall: (s2 − s − 2)L[y ] = (s − 1) y(0) + y ′(0).
Differential equation for yL[ ]−→ Algebraic equation for L[y ].
Introduce the initial condition,
(s2 − s − 2)L[y ] = (s − 1).
We can solve for the unknown L[y ] as follows,
L[y ] =(s − 1)
(s2 − s − 2).
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Recall: (s2 − s − 2)L[y ] = (s − 1) y(0) + y ′(0).
Differential equation for yL[ ]−→ Algebraic equation for L[y ].
Introduce the initial condition,
(s2 − s − 2)L[y ] = (s − 1).
We can solve for the unknown L[y ] as follows,
L[y ] =(s − 1)
(s2 − s − 2).
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Recall: (s2 − s − 2)L[y ] = (s − 1) y(0) + y ′(0).
Differential equation for yL[ ]−→ Algebraic equation for L[y ].
Introduce the initial condition,
(s2 − s − 2)L[y ] = (s − 1).
We can solve for the unknown L[y ] as follows,
L[y ] =(s − 1)
(s2 − s − 2).
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Recall: (s2 − s − 2)L[y ] = (s − 1) y(0) + y ′(0).
Differential equation for yL[ ]−→ Algebraic equation for L[y ].
Introduce the initial condition,
(s2 − s − 2)L[y ] = (s − 1).
We can solve for the unknown L[y ] as follows,
L[y ] =(s − 1)
(s2 − s − 2).
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Recall: (s2 − s − 2)L[y ] = (s − 1) y(0) + y ′(0).
Differential equation for yL[ ]−→ Algebraic equation for L[y ].
Introduce the initial condition,
(s2 − s − 2)L[y ] = (s − 1).
We can solve for the unknown L[y ] as follows,
L[y ] =(s − 1)
(s2 − s − 2).
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Recall: (s2 − s − 2)L[y ] = (s − 1) y(0) + y ′(0).
Differential equation for yL[ ]−→ Algebraic equation for L[y ].
Introduce the initial condition,
(s2 − s − 2)L[y ] = (s − 1).
We can solve for the unknown L[y ] as follows,
L[y ] =(s − 1)
(s2 − s − 2).
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Recall: L[y ] =(s − 1)
(s2 − s − 2).
The partial fraction method: Find the zeros of the denominator,
s2 − s − 2 = 0 ⇒ s± =1
2
[1±
√1 + 8
]⇒
{s+ = 2,
s− = −1,
Therefore, we rewrite: L[y ] =(s − 1)
(s − 2)(s + 1).
Find constants a and b such that
(s − 1)
(s − 2)(s + 1)=
a
s − 2+
b
s + 1.
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Recall: L[y ] =(s − 1)
(s2 − s − 2).
The partial fraction method: Find the zeros of the denominator,
s2 − s − 2 = 0
⇒ s± =1
2
[1±
√1 + 8
]⇒
{s+ = 2,
s− = −1,
Therefore, we rewrite: L[y ] =(s − 1)
(s − 2)(s + 1).
Find constants a and b such that
(s − 1)
(s − 2)(s + 1)=
a
s − 2+
b
s + 1.
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Recall: L[y ] =(s − 1)
(s2 − s − 2).
The partial fraction method: Find the zeros of the denominator,
s2 − s − 2 = 0 ⇒ s± =1
2
[1±
√1 + 8
]
⇒
{s+ = 2,
s− = −1,
Therefore, we rewrite: L[y ] =(s − 1)
(s − 2)(s + 1).
Find constants a and b such that
(s − 1)
(s − 2)(s + 1)=
a
s − 2+
b
s + 1.
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Recall: L[y ] =(s − 1)
(s2 − s − 2).
The partial fraction method: Find the zeros of the denominator,
s2 − s − 2 = 0 ⇒ s± =1
2
[1±
√1 + 8
]⇒
{s+ = 2,
s− = −1,
Therefore, we rewrite: L[y ] =(s − 1)
(s − 2)(s + 1).
Find constants a and b such that
(s − 1)
(s − 2)(s + 1)=
a
s − 2+
b
s + 1.
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Recall: L[y ] =(s − 1)
(s2 − s − 2).
The partial fraction method: Find the zeros of the denominator,
s2 − s − 2 = 0 ⇒ s± =1
2
[1±
√1 + 8
]⇒
{s+ = 2,
s− = −1,
Therefore, we rewrite: L[y ] =(s − 1)
(s − 2)(s + 1).
Find constants a and b such that
(s − 1)
(s − 2)(s + 1)=
a
s − 2+
b
s + 1.
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Recall: L[y ] =(s − 1)
(s2 − s − 2).
The partial fraction method: Find the zeros of the denominator,
s2 − s − 2 = 0 ⇒ s± =1
2
[1±
√1 + 8
]⇒
{s+ = 2,
s− = −1,
Therefore, we rewrite: L[y ] =(s − 1)
(s − 2)(s + 1).
Find constants a and b such that
(s − 1)
(s − 2)(s + 1)=
a
s − 2+
b
s + 1.
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Recall:(s − 1)
(s − 2)(s + 1)=
a
s − 2+
b
s + 1.
A simple calculation shows
(s − 1)
(s − 2)(s + 1)=
a
s − 2+
b
s + 1=
a(s + 1) + b(s − 2)
(s − 2)(s + 1)
(s − 1) = s(a + b) + (a− 2b) ⇒
{a + b = 1,
a− 2b = −1
Hence, a =1
3and b =
2
3. Then, L[y ] =
1
3
1
(s − 2)+
2
3
1
(s + 1).
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Recall:(s − 1)
(s − 2)(s + 1)=
a
s − 2+
b
s + 1.
A simple calculation shows
(s − 1)
(s − 2)(s + 1)=
a
s − 2+
b
s + 1
=a(s + 1) + b(s − 2)
(s − 2)(s + 1)
(s − 1) = s(a + b) + (a− 2b) ⇒
{a + b = 1,
a− 2b = −1
Hence, a =1
3and b =
2
3. Then, L[y ] =
1
3
1
(s − 2)+
2
3
1
(s + 1).
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Recall:(s − 1)
(s − 2)(s + 1)=
a
s − 2+
b
s + 1.
A simple calculation shows
(s − 1)
(s − 2)(s + 1)=
a
s − 2+
b
s + 1=
a(s + 1) + b(s − 2)
(s − 2)(s + 1)
(s − 1) = s(a + b) + (a− 2b) ⇒
{a + b = 1,
a− 2b = −1
Hence, a =1
3and b =
2
3. Then, L[y ] =
1
3
1
(s − 2)+
2
3
1
(s + 1).
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Recall:(s − 1)
(s − 2)(s + 1)=
a
s − 2+
b
s + 1.
A simple calculation shows
(s − 1)
(s − 2)(s + 1)=
a
s − 2+
b
s + 1=
a(s + 1) + b(s − 2)
(s − 2)(s + 1)
(s − 1) = s(a + b) + (a− 2b)
⇒
{a + b = 1,
a− 2b = −1
Hence, a =1
3and b =
2
3. Then, L[y ] =
1
3
1
(s − 2)+
2
3
1
(s + 1).
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Recall:(s − 1)
(s − 2)(s + 1)=
a
s − 2+
b
s + 1.
A simple calculation shows
(s − 1)
(s − 2)(s + 1)=
a
s − 2+
b
s + 1=
a(s + 1) + b(s − 2)
(s − 2)(s + 1)
(s − 1) = s(a + b) + (a− 2b) ⇒
{a + b = 1,
a− 2b = −1
Hence, a =1
3and b =
2
3. Then, L[y ] =
1
3
1
(s − 2)+
2
3
1
(s + 1).
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Recall:(s − 1)
(s − 2)(s + 1)=
a
s − 2+
b
s + 1.
A simple calculation shows
(s − 1)
(s − 2)(s + 1)=
a
s − 2+
b
s + 1=
a(s + 1) + b(s − 2)
(s − 2)(s + 1)
(s − 1) = s(a + b) + (a− 2b) ⇒
{a + b = 1,
a− 2b = −1
Hence, a =1
3and b =
2
3.
Then, L[y ] =1
3
1
(s − 2)+
2
3
1
(s + 1).
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Recall:(s − 1)
(s − 2)(s + 1)=
a
s − 2+
b
s + 1.
A simple calculation shows
(s − 1)
(s − 2)(s + 1)=
a
s − 2+
b
s + 1=
a(s + 1) + b(s − 2)
(s − 2)(s + 1)
(s − 1) = s(a + b) + (a− 2b) ⇒
{a + b = 1,
a− 2b = −1
Hence, a =1
3and b =
2
3. Then, L[y ] =
1
3
1
(s − 2)+
2
3
1
(s + 1).
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Recall: L[y ] =1
3
1
(s − 2)+
2
3
1
(s + 1).
From the table:
L[eat ] =1
s − a⇒ 1
s − 2= L[e2t ],
1
s + 1= L[e−t ].
So we arrive at the equation
L[y ] =1
3L[e2t ] +
2
3L[e−t ] = L
[1
3
(e2t + 2e−t
)]We conclude that: y(t) =
1
3
(e2t + 2e−t
). C
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Recall: L[y ] =1
3
1
(s − 2)+
2
3
1
(s + 1). From the table:
L[eat ] =1
s − a
⇒ 1
s − 2= L[e2t ],
1
s + 1= L[e−t ].
So we arrive at the equation
L[y ] =1
3L[e2t ] +
2
3L[e−t ] = L
[1
3
(e2t + 2e−t
)]We conclude that: y(t) =
1
3
(e2t + 2e−t
). C
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Recall: L[y ] =1
3
1
(s − 2)+
2
3
1
(s + 1). From the table:
L[eat ] =1
s − a⇒ 1
s − 2= L[e2t ],
1
s + 1= L[e−t ].
So we arrive at the equation
L[y ] =1
3L[e2t ] +
2
3L[e−t ] = L
[1
3
(e2t + 2e−t
)]We conclude that: y(t) =
1
3
(e2t + 2e−t
). C
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Recall: L[y ] =1
3
1
(s − 2)+
2
3
1
(s + 1). From the table:
L[eat ] =1
s − a⇒ 1
s − 2= L[e2t ],
1
s + 1= L[e−t ].
So we arrive at the equation
L[y ] =1
3L[e2t ] +
2
3L[e−t ] = L
[1
3
(e2t + 2e−t
)]We conclude that: y(t) =
1
3
(e2t + 2e−t
). C
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Recall: L[y ] =1
3
1
(s − 2)+
2
3
1
(s + 1). From the table:
L[eat ] =1
s − a⇒ 1
s − 2= L[e2t ],
1
s + 1= L[e−t ].
So we arrive at the equation
L[y ] =1
3L[e2t ] +
2
3L[e−t ]
= L[1
3
(e2t + 2e−t
)]We conclude that: y(t) =
1
3
(e2t + 2e−t
). C
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Recall: L[y ] =1
3
1
(s − 2)+
2
3
1
(s + 1). From the table:
L[eat ] =1
s − a⇒ 1
s − 2= L[e2t ],
1
s + 1= L[e−t ].
So we arrive at the equation
L[y ] =1
3L[e2t ] +
2
3L[e−t ] = L
[1
3
(e2t + 2e−t
)]
We conclude that: y(t) =1
3
(e2t + 2e−t
). C
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − y ′ − 2y = 0, y(0) = 1, y ′(0) = 0.
Solution: Recall: L[y ] =1
3
1
(s − 2)+
2
3
1
(s + 1). From the table:
L[eat ] =1
s − a⇒ 1
s − 2= L[e2t ],
1
s + 1= L[e−t ].
So we arrive at the equation
L[y ] =1
3L[e2t ] +
2
3L[e−t ] = L
[1
3
(e2t + 2e−t
)]We conclude that: y(t) =
1
3
(e2t + 2e−t
). C
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Compute the L[ ] of the differential equation,
L[y ′′ − 4y ′ + 4y ] = L[0] = 0.
The L[ ] is a linear function,
L[y ′′]− 4L[y ′] + 4L[y ] = 0.
Derivatives are transformed into power functions,[s2 L[y ]− s y(0)− y ′(0)
]− 4
[s L[y ]− y(0)
]+ 4L[y ] = 0,
Therefore, (s2 − 4s + 4)L[y ] = (s − 4) y(0) + y ′(0).
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Compute the L[ ] of the differential equation,
L[y ′′ − 4y ′ + 4y ] = L[0] = 0.
The L[ ] is a linear function,
L[y ′′]− 4L[y ′] + 4L[y ] = 0.
Derivatives are transformed into power functions,[s2 L[y ]− s y(0)− y ′(0)
]− 4
[s L[y ]− y(0)
]+ 4L[y ] = 0,
Therefore, (s2 − 4s + 4)L[y ] = (s − 4) y(0) + y ′(0).
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Compute the L[ ] of the differential equation,
L[y ′′ − 4y ′ + 4y ] = L[0] = 0.
The L[ ] is a linear function,
L[y ′′]− 4L[y ′] + 4L[y ] = 0.
Derivatives are transformed into power functions,[s2 L[y ]− s y(0)− y ′(0)
]− 4
[s L[y ]− y(0)
]+ 4L[y ] = 0,
Therefore, (s2 − 4s + 4)L[y ] = (s − 4) y(0) + y ′(0).
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Compute the L[ ] of the differential equation,
L[y ′′ − 4y ′ + 4y ] = L[0] = 0.
The L[ ] is a linear function,
L[y ′′]− 4L[y ′] + 4L[y ] = 0.
Derivatives are transformed into power functions,[s2 L[y ]− s y(0)− y ′(0)
]− 4
[s L[y ]− y(0)
]+ 4L[y ] = 0,
Therefore, (s2 − 4s + 4)L[y ] = (s − 4) y(0) + y ′(0).
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Compute the L[ ] of the differential equation,
L[y ′′ − 4y ′ + 4y ] = L[0] = 0.
The L[ ] is a linear function,
L[y ′′]− 4L[y ′] + 4L[y ] = 0.
Derivatives are transformed into power functions,[s2 L[y ]− s y(0)− y ′(0)
]− 4
[s L[y ]− y(0)
]+ 4L[y ] = 0,
Therefore, (s2 − 4s + 4)L[y ] = (s − 4) y(0) + y ′(0).
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Compute the L[ ] of the differential equation,
L[y ′′ − 4y ′ + 4y ] = L[0] = 0.
The L[ ] is a linear function,
L[y ′′]− 4L[y ′] + 4L[y ] = 0.
Derivatives are transformed into power functions,[s2 L[y ]− s y(0)− y ′(0)
]− 4
[s L[y ]− y(0)
]+ 4L[y ] = 0,
Therefore, (s2 − 4s + 4)L[y ] = (s − 4) y(0) + y ′(0).
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Recall: (s2 − 4s + 4)L[y ] = (s − 4) y(0) + y ′(0).
Introduce the initial conditions, (s2 − 4s + 4)L[y ] = s − 3.
Solve for L[y ] as follows: L[y ] =(s − 3)
(s2 − 4s + 4).
The partial fraction method: Find the roots of the denominator,
s2−4s+4 = 0 ⇒ s± =1
2
[4±
√16− 16
]⇒ s+ = s− = 2.
We obtain: L[y ] =(s − 3)
(s − 2)2.
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Recall: (s2 − 4s + 4)L[y ] = (s − 4) y(0) + y ′(0).
Introduce the initial conditions,
(s2 − 4s + 4)L[y ] = s − 3.
Solve for L[y ] as follows: L[y ] =(s − 3)
(s2 − 4s + 4).
The partial fraction method: Find the roots of the denominator,
s2−4s+4 = 0 ⇒ s± =1
2
[4±
√16− 16
]⇒ s+ = s− = 2.
We obtain: L[y ] =(s − 3)
(s − 2)2.
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Recall: (s2 − 4s + 4)L[y ] = (s − 4) y(0) + y ′(0).
Introduce the initial conditions, (s2 − 4s + 4)L[y ] = s − 3.
Solve for L[y ] as follows: L[y ] =(s − 3)
(s2 − 4s + 4).
The partial fraction method: Find the roots of the denominator,
s2−4s+4 = 0 ⇒ s± =1
2
[4±
√16− 16
]⇒ s+ = s− = 2.
We obtain: L[y ] =(s − 3)
(s − 2)2.
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Recall: (s2 − 4s + 4)L[y ] = (s − 4) y(0) + y ′(0).
Introduce the initial conditions, (s2 − 4s + 4)L[y ] = s − 3.
Solve for L[y ] as follows:
L[y ] =(s − 3)
(s2 − 4s + 4).
The partial fraction method: Find the roots of the denominator,
s2−4s+4 = 0 ⇒ s± =1
2
[4±
√16− 16
]⇒ s+ = s− = 2.
We obtain: L[y ] =(s − 3)
(s − 2)2.
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Recall: (s2 − 4s + 4)L[y ] = (s − 4) y(0) + y ′(0).
Introduce the initial conditions, (s2 − 4s + 4)L[y ] = s − 3.
Solve for L[y ] as follows: L[y ] =(s − 3)
(s2 − 4s + 4).
The partial fraction method: Find the roots of the denominator,
s2−4s+4 = 0 ⇒ s± =1
2
[4±
√16− 16
]⇒ s+ = s− = 2.
We obtain: L[y ] =(s − 3)
(s − 2)2.
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Recall: (s2 − 4s + 4)L[y ] = (s − 4) y(0) + y ′(0).
Introduce the initial conditions, (s2 − 4s + 4)L[y ] = s − 3.
Solve for L[y ] as follows: L[y ] =(s − 3)
(s2 − 4s + 4).
The partial fraction method:
Find the roots of the denominator,
s2−4s+4 = 0 ⇒ s± =1
2
[4±
√16− 16
]⇒ s+ = s− = 2.
We obtain: L[y ] =(s − 3)
(s − 2)2.
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Recall: (s2 − 4s + 4)L[y ] = (s − 4) y(0) + y ′(0).
Introduce the initial conditions, (s2 − 4s + 4)L[y ] = s − 3.
Solve for L[y ] as follows: L[y ] =(s − 3)
(s2 − 4s + 4).
The partial fraction method: Find the roots of the denominator,
s2−4s+4 = 0
⇒ s± =1
2
[4±
√16− 16
]⇒ s+ = s− = 2.
We obtain: L[y ] =(s − 3)
(s − 2)2.
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Recall: (s2 − 4s + 4)L[y ] = (s − 4) y(0) + y ′(0).
Introduce the initial conditions, (s2 − 4s + 4)L[y ] = s − 3.
Solve for L[y ] as follows: L[y ] =(s − 3)
(s2 − 4s + 4).
The partial fraction method: Find the roots of the denominator,
s2−4s+4 = 0 ⇒ s± =1
2
[4±
√16− 16
]
⇒ s+ = s− = 2.
We obtain: L[y ] =(s − 3)
(s − 2)2.
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Recall: (s2 − 4s + 4)L[y ] = (s − 4) y(0) + y ′(0).
Introduce the initial conditions, (s2 − 4s + 4)L[y ] = s − 3.
Solve for L[y ] as follows: L[y ] =(s − 3)
(s2 − 4s + 4).
The partial fraction method: Find the roots of the denominator,
s2−4s+4 = 0 ⇒ s± =1
2
[4±
√16− 16
]⇒ s+ = s− = 2.
We obtain: L[y ] =(s − 3)
(s − 2)2.
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Recall: (s2 − 4s + 4)L[y ] = (s − 4) y(0) + y ′(0).
Introduce the initial conditions, (s2 − 4s + 4)L[y ] = s − 3.
Solve for L[y ] as follows: L[y ] =(s − 3)
(s2 − 4s + 4).
The partial fraction method: Find the roots of the denominator,
s2−4s+4 = 0 ⇒ s± =1
2
[4±
√16− 16
]⇒ s+ = s− = 2.
We obtain: L[y ] =(s − 3)
(s − 2)2.
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Recall: L[y ] =(s − 3)
(s − 2)2.
We find the partial fraction,
(s − 3)
(s − 2)2=
a
(s − 2)+
b
(s − 2)2⇒ s − 3 = a(s − 2) + b
If s = 2, then b = −1. If s = 3, then a = 1. Hence
L[y ] =1
s − 2− 1
(s − 2)2.
From the Laplace transforms table:
L[eat ] =1
s − a⇒ 1
s − 2= L[e2t ],
L[tneat ] =n!
(s − a)(n+1)⇒ 1
(s − 2)2= L[te2t ].
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Recall: L[y ] =(s − 3)
(s − 2)2. We find the partial fraction,
(s − 3)
(s − 2)2=
a
(s − 2)+
b
(s − 2)2
⇒ s − 3 = a(s − 2) + b
If s = 2, then b = −1. If s = 3, then a = 1. Hence
L[y ] =1
s − 2− 1
(s − 2)2.
From the Laplace transforms table:
L[eat ] =1
s − a⇒ 1
s − 2= L[e2t ],
L[tneat ] =n!
(s − a)(n+1)⇒ 1
(s − 2)2= L[te2t ].
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Recall: L[y ] =(s − 3)
(s − 2)2. We find the partial fraction,
(s − 3)
(s − 2)2=
a
(s − 2)+
b
(s − 2)2⇒ s − 3 = a(s − 2) + b
If s = 2, then b = −1. If s = 3, then a = 1. Hence
L[y ] =1
s − 2− 1
(s − 2)2.
From the Laplace transforms table:
L[eat ] =1
s − a⇒ 1
s − 2= L[e2t ],
L[tneat ] =n!
(s − a)(n+1)⇒ 1
(s − 2)2= L[te2t ].
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Recall: L[y ] =(s − 3)
(s − 2)2. We find the partial fraction,
(s − 3)
(s − 2)2=
a
(s − 2)+
b
(s − 2)2⇒ s − 3 = a(s − 2) + b
If s = 2,
then b = −1. If s = 3, then a = 1. Hence
L[y ] =1
s − 2− 1
(s − 2)2.
From the Laplace transforms table:
L[eat ] =1
s − a⇒ 1
s − 2= L[e2t ],
L[tneat ] =n!
(s − a)(n+1)⇒ 1
(s − 2)2= L[te2t ].
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Recall: L[y ] =(s − 3)
(s − 2)2. We find the partial fraction,
(s − 3)
(s − 2)2=
a
(s − 2)+
b
(s − 2)2⇒ s − 3 = a(s − 2) + b
If s = 2, then b = −1.
If s = 3, then a = 1. Hence
L[y ] =1
s − 2− 1
(s − 2)2.
From the Laplace transforms table:
L[eat ] =1
s − a⇒ 1
s − 2= L[e2t ],
L[tneat ] =n!
(s − a)(n+1)⇒ 1
(s − 2)2= L[te2t ].
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Recall: L[y ] =(s − 3)
(s − 2)2. We find the partial fraction,
(s − 3)
(s − 2)2=
a
(s − 2)+
b
(s − 2)2⇒ s − 3 = a(s − 2) + b
If s = 2, then b = −1. If s = 3,
then a = 1. Hence
L[y ] =1
s − 2− 1
(s − 2)2.
From the Laplace transforms table:
L[eat ] =1
s − a⇒ 1
s − 2= L[e2t ],
L[tneat ] =n!
(s − a)(n+1)⇒ 1
(s − 2)2= L[te2t ].
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Recall: L[y ] =(s − 3)
(s − 2)2. We find the partial fraction,
(s − 3)
(s − 2)2=
a
(s − 2)+
b
(s − 2)2⇒ s − 3 = a(s − 2) + b
If s = 2, then b = −1. If s = 3, then a = 1.
Hence
L[y ] =1
s − 2− 1
(s − 2)2.
From the Laplace transforms table:
L[eat ] =1
s − a⇒ 1
s − 2= L[e2t ],
L[tneat ] =n!
(s − a)(n+1)⇒ 1
(s − 2)2= L[te2t ].
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Recall: L[y ] =(s − 3)
(s − 2)2. We find the partial fraction,
(s − 3)
(s − 2)2=
a
(s − 2)+
b
(s − 2)2⇒ s − 3 = a(s − 2) + b
If s = 2, then b = −1. If s = 3, then a = 1. Hence
L[y ] =1
s − 2− 1
(s − 2)2.
From the Laplace transforms table:
L[eat ] =1
s − a⇒ 1
s − 2= L[e2t ],
L[tneat ] =n!
(s − a)(n+1)⇒ 1
(s − 2)2= L[te2t ].
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Recall: L[y ] =(s − 3)
(s − 2)2. We find the partial fraction,
(s − 3)
(s − 2)2=
a
(s − 2)+
b
(s − 2)2⇒ s − 3 = a(s − 2) + b
If s = 2, then b = −1. If s = 3, then a = 1. Hence
L[y ] =1
s − 2− 1
(s − 2)2.
From the Laplace transforms table:
L[eat ] =1
s − a
⇒ 1
s − 2= L[e2t ],
L[tneat ] =n!
(s − a)(n+1)⇒ 1
(s − 2)2= L[te2t ].
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Recall: L[y ] =(s − 3)
(s − 2)2. We find the partial fraction,
(s − 3)
(s − 2)2=
a
(s − 2)+
b
(s − 2)2⇒ s − 3 = a(s − 2) + b
If s = 2, then b = −1. If s = 3, then a = 1. Hence
L[y ] =1
s − 2− 1
(s − 2)2.
From the Laplace transforms table:
L[eat ] =1
s − a⇒ 1
s − 2= L[e2t ],
L[tneat ] =n!
(s − a)(n+1)⇒ 1
(s − 2)2= L[te2t ].
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Recall: L[y ] =(s − 3)
(s − 2)2. We find the partial fraction,
(s − 3)
(s − 2)2=
a
(s − 2)+
b
(s − 2)2⇒ s − 3 = a(s − 2) + b
If s = 2, then b = −1. If s = 3, then a = 1. Hence
L[y ] =1
s − 2− 1
(s − 2)2.
From the Laplace transforms table:
L[eat ] =1
s − a⇒ 1
s − 2= L[e2t ],
L[tneat ] =n!
(s − a)(n+1)
⇒ 1
(s − 2)2= L[te2t ].
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Recall: L[y ] =(s − 3)
(s − 2)2. We find the partial fraction,
(s − 3)
(s − 2)2=
a
(s − 2)+
b
(s − 2)2⇒ s − 3 = a(s − 2) + b
If s = 2, then b = −1. If s = 3, then a = 1. Hence
L[y ] =1
s − 2− 1
(s − 2)2.
From the Laplace transforms table:
L[eat ] =1
s − a⇒ 1
s − 2= L[e2t ],
L[tneat ] =n!
(s − a)(n+1)⇒ 1
(s − 2)2= L[te2t ].
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Recall: L[y ] =1
s − 2− 1
(s − 2)2and
1
s − 2= L[e2t ],
1
(s − 2)2= L[te2t ].
So we arrive at the equation
L[y ] = L[e2t ]− L[te2t ] = L[e2t − te2t
].
We conclude that y(t) = e2t − te2t . C
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Recall: L[y ] =1
s − 2− 1
(s − 2)2and
1
s − 2= L[e2t ],
1
(s − 2)2= L[te2t ].
So we arrive at the equation
L[y ] = L[e2t ]− L[te2t ]
= L[e2t − te2t
].
We conclude that y(t) = e2t − te2t . C
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Recall: L[y ] =1
s − 2− 1
(s − 2)2and
1
s − 2= L[e2t ],
1
(s − 2)2= L[te2t ].
So we arrive at the equation
L[y ] = L[e2t ]− L[te2t ] = L[e2t − te2t
].
We conclude that y(t) = e2t − te2t . C
Homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 0, y(0) = 1, y ′(0) = 1.
Solution: Recall: L[y ] =1
s − 2− 1
(s − 2)2and
1
s − 2= L[e2t ],
1
(s − 2)2= L[te2t ].
So we arrive at the equation
L[y ] = L[e2t ]− L[te2t ] = L[e2t − te2t
].
We conclude that y(t) = e2t − te2t . C
The Laplace Transform and the IVP (Sect. 4.2).
I Solving differential equations using L[ ].I Homogeneous IVP.I First, second, higher order equations.I Non-homogeneous IVP.
First, second, higher order equations.
Example
Use the Laplace Transform to find the solution of y (4) − 4y = 0,
y(0) = 1, y ′(0) = 1, y ′′(0) = −2, y ′′′(0) = 0.
Solution: Compute the L[ ] of the equation,
L[y (4)
]− 4L[y ] = 0.
[s4 L[y ]− s3 y(0)− s2 y ′(0)− s y ′′(0)− y ′′′(0)
]− 4L[y ] = 0.
[s4 L[y ]− s3 + 2s
]− 4L[y ] = 0 ⇒ (s4 − 4)L[y ] = s3 − 2s,
We obtain, L[y ] =s3 − 2s
(s4 − 4).
First, second, higher order equations.
Example
Use the Laplace Transform to find the solution of y (4) − 4y = 0,
y(0) = 1, y ′(0) = 1, y ′′(0) = −2, y ′′′(0) = 0.
Solution: Compute the L[ ] of the equation,
L[y (4)
]− 4L[y ] = 0.
[s4 L[y ]− s3 y(0)− s2 y ′(0)− s y ′′(0)− y ′′′(0)
]− 4L[y ] = 0.
[s4 L[y ]− s3 + 2s
]− 4L[y ] = 0 ⇒ (s4 − 4)L[y ] = s3 − 2s,
We obtain, L[y ] =s3 − 2s
(s4 − 4).
First, second, higher order equations.
Example
Use the Laplace Transform to find the solution of y (4) − 4y = 0,
y(0) = 1, y ′(0) = 1, y ′′(0) = −2, y ′′′(0) = 0.
Solution: Compute the L[ ] of the equation,
L[y (4)
]− 4L[y ] = 0.
[s4 L[y ]− s3 y(0)− s2 y ′(0)− s y ′′(0)− y ′′′(0)
]− 4L[y ] = 0.
[s4 L[y ]− s3 + 2s
]− 4L[y ] = 0 ⇒ (s4 − 4)L[y ] = s3 − 2s,
We obtain, L[y ] =s3 − 2s
(s4 − 4).
First, second, higher order equations.
Example
Use the Laplace Transform to find the solution of y (4) − 4y = 0,
y(0) = 1, y ′(0) = 1, y ′′(0) = −2, y ′′′(0) = 0.
Solution: Compute the L[ ] of the equation,
L[y (4)
]− 4L[y ] = 0.
[s4 L[y ]− s3 y(0)− s2 y ′(0)− s y ′′(0)− y ′′′(0)
]− 4L[y ] = 0.
[s4 L[y ]− s3 + 2s
]− 4L[y ] = 0
⇒ (s4 − 4)L[y ] = s3 − 2s,
We obtain, L[y ] =s3 − 2s
(s4 − 4).
First, second, higher order equations.
Example
Use the Laplace Transform to find the solution of y (4) − 4y = 0,
y(0) = 1, y ′(0) = 1, y ′′(0) = −2, y ′′′(0) = 0.
Solution: Compute the L[ ] of the equation,
L[y (4)
]− 4L[y ] = 0.
[s4 L[y ]− s3 y(0)− s2 y ′(0)− s y ′′(0)− y ′′′(0)
]− 4L[y ] = 0.
[s4 L[y ]− s3 + 2s
]− 4L[y ] = 0 ⇒ (s4 − 4)L[y ] = s3 − 2s,
We obtain, L[y ] =s3 − 2s
(s4 − 4).
First, second, higher order equations.
Example
Use the Laplace Transform to find the solution of y (4) − 4y = 0,
y(0) = 1, y ′(0) = 1, y ′′(0) = −2, y ′′′(0) = 0.
Solution: Compute the L[ ] of the equation,
L[y (4)
]− 4L[y ] = 0.
[s4 L[y ]− s3 y(0)− s2 y ′(0)− s y ′′(0)− y ′′′(0)
]− 4L[y ] = 0.
[s4 L[y ]− s3 + 2s
]− 4L[y ] = 0 ⇒ (s4 − 4)L[y ] = s3 − 2s,
We obtain, L[y ] =s3 − 2s
(s4 − 4).
First, second, higher order equations.
Example
Use the Laplace Transform to find the solution of y (4) − 4y = 0,
y(0) = 1, y ′(0) = 1, y ′′(0) = −2, y ′′′(0) = 0.
Solution: Recall: L[y ] =s3 − 2s
(s4 − 4).
L[y ] =s(s2 − 2)
(s2 − 2)(s2 + 2)⇒ L[y ] =
s
(s2 + 2).
The last expression is in the table of Laplace Transforms,
L[y ] =s(
s2 +[√
2]2) = L
[cos(
√2 t)
].
We conclude that y(t) = cos(√
2 t). C
First, second, higher order equations.
Example
Use the Laplace Transform to find the solution of y (4) − 4y = 0,
y(0) = 1, y ′(0) = 1, y ′′(0) = −2, y ′′′(0) = 0.
Solution: Recall: L[y ] =s3 − 2s
(s4 − 4).
L[y ] =s(s2 − 2)
(s2 − 2)(s2 + 2)⇒ L[y ] =
s
(s2 + 2).
The last expression is in the table of Laplace Transforms,
L[y ] =s(
s2 +[√
2]2) = L
[cos(
√2 t)
].
We conclude that y(t) = cos(√
2 t). C
First, second, higher order equations.
Example
Use the Laplace Transform to find the solution of y (4) − 4y = 0,
y(0) = 1, y ′(0) = 1, y ′′(0) = −2, y ′′′(0) = 0.
Solution: Recall: L[y ] =s3 − 2s
(s4 − 4).
L[y ] =s(s2 − 2)
(s2 − 2)(s2 + 2)
⇒ L[y ] =s
(s2 + 2).
The last expression is in the table of Laplace Transforms,
L[y ] =s(
s2 +[√
2]2) = L
[cos(
√2 t)
].
We conclude that y(t) = cos(√
2 t). C
First, second, higher order equations.
Example
Use the Laplace Transform to find the solution of y (4) − 4y = 0,
y(0) = 1, y ′(0) = 1, y ′′(0) = −2, y ′′′(0) = 0.
Solution: Recall: L[y ] =s3 − 2s
(s4 − 4).
L[y ] =s(s2 − 2)
(s2 − 2)(s2 + 2)⇒ L[y ] =
s
(s2 + 2).
The last expression is in the table of Laplace Transforms,
L[y ] =s(
s2 +[√
2]2) = L
[cos(
√2 t)
].
We conclude that y(t) = cos(√
2 t). C
First, second, higher order equations.
Example
Use the Laplace Transform to find the solution of y (4) − 4y = 0,
y(0) = 1, y ′(0) = 1, y ′′(0) = −2, y ′′′(0) = 0.
Solution: Recall: L[y ] =s3 − 2s
(s4 − 4).
L[y ] =s(s2 − 2)
(s2 − 2)(s2 + 2)⇒ L[y ] =
s
(s2 + 2).
The last expression is in the table of Laplace Transforms,
L[y ] =s(
s2 +[√
2]2) = L
[cos(
√2 t)
].
We conclude that y(t) = cos(√
2 t). C
First, second, higher order equations.
Example
Use the Laplace Transform to find the solution of y (4) − 4y = 0,
y(0) = 1, y ′(0) = 1, y ′′(0) = −2, y ′′′(0) = 0.
Solution: Recall: L[y ] =s3 − 2s
(s4 − 4).
L[y ] =s(s2 − 2)
(s2 − 2)(s2 + 2)⇒ L[y ] =
s
(s2 + 2).
The last expression is in the table of Laplace Transforms,
L[y ] =s(
s2 +[√
2]2)
= L[cos(
√2 t)
].
We conclude that y(t) = cos(√
2 t). C
First, second, higher order equations.
Example
Use the Laplace Transform to find the solution of y (4) − 4y = 0,
y(0) = 1, y ′(0) = 1, y ′′(0) = −2, y ′′′(0) = 0.
Solution: Recall: L[y ] =s3 − 2s
(s4 − 4).
L[y ] =s(s2 − 2)
(s2 − 2)(s2 + 2)⇒ L[y ] =
s
(s2 + 2).
The last expression is in the table of Laplace Transforms,
L[y ] =s(
s2 +[√
2]2) = L
[cos(
√2 t)
].
We conclude that y(t) = cos(√
2 t). C
First, second, higher order equations.
Example
Use the Laplace Transform to find the solution of y (4) − 4y = 0,
y(0) = 1, y ′(0) = 1, y ′′(0) = −2, y ′′′(0) = 0.
Solution: Recall: L[y ] =s3 − 2s
(s4 − 4).
L[y ] =s(s2 − 2)
(s2 − 2)(s2 + 2)⇒ L[y ] =
s
(s2 + 2).
The last expression is in the table of Laplace Transforms,
L[y ] =s(
s2 +[√
2]2) = L
[cos(
√2 t)
].
We conclude that y(t) = cos(√
2 t). C
The Laplace Transform and the IVP (Sect. 4.2).
I Solving differential equations using L[ ].I Homogeneous IVP.I First, second, higher order equations.I Non-homogeneous IVP.
Non-homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: Compute the Laplace transform of the equation,
L[y ′′ − 4y ′ + 4y ] = L[3 sin(2t)].
The right-hand side above can be expressed as follows,
L[3 sin(2t)] = 3L[sin(2t)] = 32
s2 + 22=
6
s2 + 4.
Introduce this source term in the differential equation,
L[y ′′]− 4L[y ′] + 4L[y ] =6
s2 + 4.
Non-homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: Compute the Laplace transform of the equation,
L[y ′′ − 4y ′ + 4y ] = L[3 sin(2t)].
The right-hand side above can be expressed as follows,
L[3 sin(2t)] = 3L[sin(2t)] = 32
s2 + 22=
6
s2 + 4.
Introduce this source term in the differential equation,
L[y ′′]− 4L[y ′] + 4L[y ] =6
s2 + 4.
Non-homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: Compute the Laplace transform of the equation,
L[y ′′ − 4y ′ + 4y ] = L[3 sin(2t)].
The right-hand side above can be expressed as follows,
L[3 sin(2t)] = 3L[sin(2t)] = 32
s2 + 22=
6
s2 + 4.
Introduce this source term in the differential equation,
L[y ′′]− 4L[y ′] + 4L[y ] =6
s2 + 4.
Non-homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: Compute the Laplace transform of the equation,
L[y ′′ − 4y ′ + 4y ] = L[3 sin(2t)].
The right-hand side above can be expressed as follows,
L[3 sin(2t)] = 3L[sin(2t)] = 32
s2 + 22=
6
s2 + 4.
Introduce this source term in the differential equation,
L[y ′′]− 4L[y ′] + 4L[y ] =6
s2 + 4.
Non-homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: Compute the Laplace transform of the equation,
L[y ′′ − 4y ′ + 4y ] = L[3 sin(2t)].
The right-hand side above can be expressed as follows,
L[3 sin(2t)] = 3L[sin(2t)]
= 32
s2 + 22=
6
s2 + 4.
Introduce this source term in the differential equation,
L[y ′′]− 4L[y ′] + 4L[y ] =6
s2 + 4.
Non-homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: Compute the Laplace transform of the equation,
L[y ′′ − 4y ′ + 4y ] = L[3 sin(2t)].
The right-hand side above can be expressed as follows,
L[3 sin(2t)] = 3L[sin(2t)] = 32
s2 + 22
=6
s2 + 4.
Introduce this source term in the differential equation,
L[y ′′]− 4L[y ′] + 4L[y ] =6
s2 + 4.
Non-homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: Compute the Laplace transform of the equation,
L[y ′′ − 4y ′ + 4y ] = L[3 sin(2t)].
The right-hand side above can be expressed as follows,
L[3 sin(2t)] = 3L[sin(2t)] = 32
s2 + 22=
6
s2 + 4.
Introduce this source term in the differential equation,
L[y ′′]− 4L[y ′] + 4L[y ] =6
s2 + 4.
Non-homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: Compute the Laplace transform of the equation,
L[y ′′ − 4y ′ + 4y ] = L[3 sin(2t)].
The right-hand side above can be expressed as follows,
L[3 sin(2t)] = 3L[sin(2t)] = 32
s2 + 22=
6
s2 + 4.
Introduce this source term in the differential equation,
L[y ′′]− 4L[y ′] + 4L[y ] =6
s2 + 4.
Non-homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: Compute the Laplace transform of the equation,
L[y ′′ − 4y ′ + 4y ] = L[3 sin(2t)].
The right-hand side above can be expressed as follows,
L[3 sin(2t)] = 3L[sin(2t)] = 32
s2 + 22=
6
s2 + 4.
Introduce this source term in the differential equation,
L[y ′′]− 4L[y ′] + 4L[y ] =6
s2 + 4.
Non-homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: Recall: L[y ′′]− 4L[y ′] + 4L[y ] =6
s2 + 4.
Derivatives are transformed into power functions,[s2 L[y ]− s y(0)− y ′(0)
]− 4
[s L[y ]− y(0)
]+ 4L[y ] =
6
s2 + 4.
Rewrite the above equation,
(s2 − 4s + 4)L[y ] = (s − 4) y(0) + y ′(0) +6
s2 + 4.
Introduce the initial conditions,
(s2 − 4s + 4)L[y ] = s − 3 +6
s2 + 4.
Non-homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: Recall: L[y ′′]− 4L[y ′] + 4L[y ] =6
s2 + 4.
Derivatives are transformed into power functions,[s2 L[y ]− s y(0)− y ′(0)
]− 4
[s L[y ]− y(0)
]+ 4L[y ] =
6
s2 + 4.
Rewrite the above equation,
(s2 − 4s + 4)L[y ] = (s − 4) y(0) + y ′(0) +6
s2 + 4.
Introduce the initial conditions,
(s2 − 4s + 4)L[y ] = s − 3 +6
s2 + 4.
Non-homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: Recall: L[y ′′]− 4L[y ′] + 4L[y ] =6
s2 + 4.
Derivatives are transformed into power functions,[s2 L[y ]− s y(0)− y ′(0)
]− 4
[s L[y ]− y(0)
]+ 4L[y ] =
6
s2 + 4.
Rewrite the above equation,
(s2 − 4s + 4)L[y ] = (s − 4) y(0) + y ′(0) +6
s2 + 4.
Introduce the initial conditions,
(s2 − 4s + 4)L[y ] = s − 3 +6
s2 + 4.
Non-homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: Recall: L[y ′′]− 4L[y ′] + 4L[y ] =6
s2 + 4.
Derivatives are transformed into power functions,[s2 L[y ]− s y(0)− y ′(0)
]− 4
[s L[y ]− y(0)
]+ 4L[y ] =
6
s2 + 4.
Rewrite the above equation,
(s2 − 4s + 4)L[y ] = (s − 4) y(0) + y ′(0) +6
s2 + 4.
Introduce the initial conditions,
(s2 − 4s + 4)L[y ] = s − 3 +6
s2 + 4.
Non-homogeneous IVP.Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: Recall: (s2 − 4s + 4)L[y ] = s − 3 +6
s2 + 4.
Therefore, L[y ] =(s − 3)
(s2 − 4s + 4)+
6
(s2 − 4 + 4)(s2 + 4).
From an Example above: s2 − 4s + 4 = (s − 2)2,
L[y ] =1
s − 2− 1
(s − 2)2+
6
(s − 2)2(s2 + 4).
From an Example above we know that
L[e2t − te2t ] =1
s − 2− 1
(s − 2)2.
Non-homogeneous IVP.Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: Recall: (s2 − 4s + 4)L[y ] = s − 3 +6
s2 + 4.
Therefore, L[y ] =(s − 3)
(s2 − 4s + 4)+
6
(s2 − 4 + 4)(s2 + 4).
From an Example above: s2 − 4s + 4 = (s − 2)2,
L[y ] =1
s − 2− 1
(s − 2)2+
6
(s − 2)2(s2 + 4).
From an Example above we know that
L[e2t − te2t ] =1
s − 2− 1
(s − 2)2.
Non-homogeneous IVP.Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: Recall: (s2 − 4s + 4)L[y ] = s − 3 +6
s2 + 4.
Therefore, L[y ] =(s − 3)
(s2 − 4s + 4)+
6
(s2 − 4 + 4)(s2 + 4).
From an Example above: s2 − 4s + 4 = (s − 2)2,
L[y ] =1
s − 2− 1
(s − 2)2+
6
(s − 2)2(s2 + 4).
From an Example above we know that
L[e2t − te2t ] =1
s − 2− 1
(s − 2)2.
Non-homogeneous IVP.Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: Recall: (s2 − 4s + 4)L[y ] = s − 3 +6
s2 + 4.
Therefore, L[y ] =(s − 3)
(s2 − 4s + 4)+
6
(s2 − 4 + 4)(s2 + 4).
From an Example above: s2 − 4s + 4 = (s − 2)2,
L[y ] =1
s − 2− 1
(s − 2)2+
6
(s − 2)2(s2 + 4).
From an Example above we know that
L[e2t − te2t ] =1
s − 2− 1
(s − 2)2.
Non-homogeneous IVP.Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: Recall: (s2 − 4s + 4)L[y ] = s − 3 +6
s2 + 4.
Therefore, L[y ] =(s − 3)
(s2 − 4s + 4)+
6
(s2 − 4 + 4)(s2 + 4).
From an Example above: s2 − 4s + 4 = (s − 2)2,
L[y ] =1
s − 2− 1
(s − 2)2+
6
(s − 2)2(s2 + 4).
From an Example above we know that
L[e2t − te2t ] =1
s − 2− 1
(s − 2)2.
Non-homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: Recall: L[y ] = L[e2t − te2t ] +6
(s − 2)2(s2 + 4).
Use Partial fractions to simplify the last term above.
Find constants a, b, c , d , such that
6
(s − 2)2 (s2 + 4)=
as + b
s2 + 4+
c
(s − 2)+
d
(s − 2)2
6
(s − 2)2 (s2 + 4)=
(as + b)(s − 2)2 + c(s − 2)(s2 + 4) + d(s2 + 4)
(s2 + 4)(s − 2)2
6 = (as + b)(s − 2)2 + c(s − 2)(s2 + 4) + d(s2 + 4).
Non-homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: Recall: L[y ] = L[e2t − te2t ] +6
(s − 2)2(s2 + 4).
Use Partial fractions to simplify the last term above.
Find constants a, b, c , d , such that
6
(s − 2)2 (s2 + 4)=
as + b
s2 + 4+
c
(s − 2)+
d
(s − 2)2
6
(s − 2)2 (s2 + 4)=
(as + b)(s − 2)2 + c(s − 2)(s2 + 4) + d(s2 + 4)
(s2 + 4)(s − 2)2
6 = (as + b)(s − 2)2 + c(s − 2)(s2 + 4) + d(s2 + 4).
Non-homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: Recall: L[y ] = L[e2t − te2t ] +6
(s − 2)2(s2 + 4).
Use Partial fractions to simplify the last term above.
Find constants a, b, c , d , such that
6
(s − 2)2 (s2 + 4)=
as + b
s2 + 4+
c
(s − 2)+
d
(s − 2)2
6
(s − 2)2 (s2 + 4)=
(as + b)(s − 2)2 + c(s − 2)(s2 + 4) + d(s2 + 4)
(s2 + 4)(s − 2)2
6 = (as + b)(s − 2)2 + c(s − 2)(s2 + 4) + d(s2 + 4).
Non-homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: Recall: L[y ] = L[e2t − te2t ] +6
(s − 2)2(s2 + 4).
Use Partial fractions to simplify the last term above.
Find constants a, b, c , d , such that
6
(s − 2)2 (s2 + 4)=
as + b
s2 + 4+
c
(s − 2)+
d
(s − 2)2
6
(s − 2)2 (s2 + 4)=
(as + b)(s − 2)2 + c(s − 2)(s2 + 4) + d(s2 + 4)
(s2 + 4)(s − 2)2
6 = (as + b)(s − 2)2 + c(s − 2)(s2 + 4) + d(s2 + 4).
Non-homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: Recall: L[y ] = L[e2t − te2t ] +6
(s − 2)2(s2 + 4).
Use Partial fractions to simplify the last term above.
Find constants a, b, c , d , such that
6
(s − 2)2 (s2 + 4)=
as + b
s2 + 4+
c
(s − 2)+
d
(s − 2)2
6
(s − 2)2 (s2 + 4)=
(as + b)(s − 2)2 + c(s − 2)(s2 + 4) + d(s2 + 4)
(s2 + 4)(s − 2)2
6 = (as + b)(s − 2)2 + c(s − 2)(s2 + 4) + d(s2 + 4).
Non-homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: 6 = (as + b)(s − 2)2 + c(s − 2)(s2 + 4) + d(s2 + 4).
6 = (as + b)(s2 − 4s + 4) + c(s3 + 4s − 2s2 − 8) + d(s2 + 4)
6 = a(s3−4s2+4s)+b(s2−4s+4)+c(s3+4s−2s2−8)+d(s2+4).
6 = (a + c)s3 + (−4a + b − 2c + d)s2
+ (4a− 4b + 4c)s + (4b − 8c + 4d).
We obtain the system
a + c= 0, −4a + b − 2c + d= 0,
4a− 4b + 4c= 0, 4b − 8c + 4d = 6.
Non-homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: 6 = (as + b)(s − 2)2 + c(s − 2)(s2 + 4) + d(s2 + 4).
6 = (as + b)(s2 − 4s + 4) + c(s3 + 4s − 2s2 − 8) + d(s2 + 4)
6 = a(s3−4s2+4s)+b(s2−4s+4)+c(s3+4s−2s2−8)+d(s2+4).
6 = (a + c)s3 + (−4a + b − 2c + d)s2
+ (4a− 4b + 4c)s + (4b − 8c + 4d).
We obtain the system
a + c= 0, −4a + b − 2c + d= 0,
4a− 4b + 4c= 0, 4b − 8c + 4d = 6.
Non-homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: 6 = (as + b)(s − 2)2 + c(s − 2)(s2 + 4) + d(s2 + 4).
6 = (as + b)(s2 − 4s + 4) + c(s3 + 4s − 2s2 − 8) + d(s2 + 4)
6 = a(s3−4s2+4s)+b(s2−4s+4)+c(s3+4s−2s2−8)+d(s2+4).
6 = (a + c)s3 + (−4a + b − 2c + d)s2
+ (4a− 4b + 4c)s + (4b − 8c + 4d).
We obtain the system
a + c= 0, −4a + b − 2c + d= 0,
4a− 4b + 4c= 0, 4b − 8c + 4d = 6.
Non-homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: 6 = (as + b)(s − 2)2 + c(s − 2)(s2 + 4) + d(s2 + 4).
6 = (as + b)(s2 − 4s + 4) + c(s3 + 4s − 2s2 − 8) + d(s2 + 4)
6 = a(s3−4s2+4s)+b(s2−4s+4)+c(s3+4s−2s2−8)+d(s2+4).
6 = (a + c)s3 + (−4a + b − 2c + d)s2
+ (4a− 4b + 4c)s + (4b − 8c + 4d).
We obtain the system
a + c= 0, −4a + b − 2c + d= 0,
4a− 4b + 4c= 0, 4b − 8c + 4d = 6.
Non-homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: 6 = (as + b)(s − 2)2 + c(s − 2)(s2 + 4) + d(s2 + 4).
6 = (as + b)(s2 − 4s + 4) + c(s3 + 4s − 2s2 − 8) + d(s2 + 4)
6 = a(s3−4s2+4s)+b(s2−4s+4)+c(s3+4s−2s2−8)+d(s2+4).
6 = (a + c)s3 + (−4a + b − 2c + d)s2
+ (4a− 4b + 4c)s + (4b − 8c + 4d).
We obtain the system
a + c= 0, −4a + b − 2c + d= 0,
4a− 4b + 4c= 0, 4b − 8c + 4d = 6.
Non-homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: The solution for this linear system is
a =3
8, b = 0, c = −3
8, d =
3
4.
6
(s − 2)2 (s2 + 4)=
3
8
s
s2 + 4− 3
8
1
(s − 2)+
3
4
1
(s − 2)2.
Use the table of Laplace Transforms
6
(s − 2)2 (s2 + 4)=
3
8L[cos(2t)]− 3
8L[e2t ] +
3
4L[te2t ].
6
(s − 2)2 (s2 + 4)= L
[3
8cos(2t)− 3
8e2t +
3
4te2t
].
Non-homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: The solution for this linear system is
a =3
8, b = 0, c = −3
8, d =
3
4.
6
(s − 2)2 (s2 + 4)=
3
8
s
s2 + 4− 3
8
1
(s − 2)+
3
4
1
(s − 2)2.
Use the table of Laplace Transforms
6
(s − 2)2 (s2 + 4)=
3
8L[cos(2t)]− 3
8L[e2t ] +
3
4L[te2t ].
6
(s − 2)2 (s2 + 4)= L
[3
8cos(2t)− 3
8e2t +
3
4te2t
].
Non-homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: The solution for this linear system is
a =3
8, b = 0, c = −3
8, d =
3
4.
6
(s − 2)2 (s2 + 4)=
3
8
s
s2 + 4− 3
8
1
(s − 2)+
3
4
1
(s − 2)2.
Use the table of Laplace Transforms
6
(s − 2)2 (s2 + 4)=
3
8L[cos(2t)]− 3
8L[e2t ] +
3
4L[te2t ].
6
(s − 2)2 (s2 + 4)= L
[3
8cos(2t)− 3
8e2t +
3
4te2t
].
Non-homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: The solution for this linear system is
a =3
8, b = 0, c = −3
8, d =
3
4.
6
(s − 2)2 (s2 + 4)=
3
8
s
s2 + 4− 3
8
1
(s − 2)+
3
4
1
(s − 2)2.
Use the table of Laplace Transforms
6
(s − 2)2 (s2 + 4)=
3
8L[cos(2t)]− 3
8L[e2t ] +
3
4L[te2t ].
6
(s − 2)2 (s2 + 4)= L
[3
8cos(2t)− 3
8e2t +
3
4te2t
].
Non-homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: Summary: L[y ] = L[e2t − te2t ] +6
(s − 2)2(s2 + 4),
6
(s − 2)2 (s2 + 4)= L
[3
8cos(2t)− 3
8e2t +
3
4te2t
].
L[y(t)] = L[(1− t) e2t +
3
8(−1 + 2t) e2t +
3
8cos(2t)
].
We conclude that
y(t) = (1− t) e2t +3
8(2t − 1) e2t +
3
8cos(2t). C
Non-homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: Summary: L[y ] = L[e2t − te2t ] +6
(s − 2)2(s2 + 4),
6
(s − 2)2 (s2 + 4)= L
[3
8cos(2t)− 3
8e2t +
3
4te2t
].
L[y(t)] = L[(1− t) e2t +
3
8(−1 + 2t) e2t +
3
8cos(2t)
].
We conclude that
y(t) = (1− t) e2t +3
8(2t − 1) e2t +
3
8cos(2t). C
Non-homogeneous IVP.
Example
Use the Laplace transform to find the solution y(t) to the IVP
y ′′ − 4y ′ + 4y = 3 sin(2t), y(0) = 1, y ′(0) = 1.
Solution: Summary: L[y ] = L[e2t − te2t ] +6
(s − 2)2(s2 + 4),
6
(s − 2)2 (s2 + 4)= L
[3
8cos(2t)− 3
8e2t +
3
4te2t
].
L[y(t)] = L[(1− t) e2t +
3
8(−1 + 2t) e2t +
3
8cos(2t)
].
We conclude that
y(t) = (1− t) e2t +3
8(2t − 1) e2t +
3
8cos(2t). C
The Laplace Transform of step functions (Sect. 4.3).
I Overview and notation.
I The definition of a step function.
I Piecewise discontinuous functions.
I The Laplace Transform of discontinuous functions.
I Properties of the Laplace Transform.
Overview and notation.
Overview: The Laplace Transform method can be used to solveconstant coefficients differential equations with discontinuoussource functions.
Notation:If L[f (t)] = F (s), then we denote L−1[F (s)] = f (t).
Remark: One can show that for a particular type of functions f ,that includes all functions we work with in this Section, thenotation above is well-defined.
Example
From the Laplace Transform table we know that L[eat
]=
1
s − a.
Then also holds that L−1[ 1
s − a
]= eat . C
Overview and notation.
Overview: The Laplace Transform method can be used to solveconstant coefficients differential equations with discontinuoussource functions.
Notation:If L[f (t)] = F (s), then we denote L−1[F (s)] = f (t).
Remark: One can show that for a particular type of functions f ,that includes all functions we work with in this Section, thenotation above is well-defined.
Example
From the Laplace Transform table we know that L[eat
]=
1
s − a.
Then also holds that L−1[ 1
s − a
]= eat . C
Overview and notation.
Overview: The Laplace Transform method can be used to solveconstant coefficients differential equations with discontinuoussource functions.
Notation:If L[f (t)] = F (s), then we denote L−1[F (s)] = f (t).
Remark: One can show that for a particular type of functions f ,that includes all functions we work with in this Section, thenotation above is well-defined.
Example
From the Laplace Transform table we know that L[eat
]=
1
s − a.
Then also holds that L−1[ 1
s − a
]= eat . C
Overview and notation.
Overview: The Laplace Transform method can be used to solveconstant coefficients differential equations with discontinuoussource functions.
Notation:If L[f (t)] = F (s), then we denote L−1[F (s)] = f (t).
Remark: One can show that for a particular type of functions f ,that includes all functions we work with in this Section, thenotation above is well-defined.
Example
From the Laplace Transform table we know that L[eat
]=
1
s − a.
Then also holds that L−1[ 1
s − a
]= eat . C
Overview and notation.
Overview: The Laplace Transform method can be used to solveconstant coefficients differential equations with discontinuoussource functions.
Notation:If L[f (t)] = F (s), then we denote L−1[F (s)] = f (t).
Remark: One can show that for a particular type of functions f ,that includes all functions we work with in this Section, thenotation above is well-defined.
Example
From the Laplace Transform table we know that L[eat
]=
1
s − a.
Then also holds that L−1[ 1
s − a
]= eat . C
The Laplace Transform of step functions (Sect. 4.3).
I Overview and notation.
I The definition of a step function.
I Piecewise discontinuous functions.
I The Laplace Transform of discontinuous functions.
I Properties of the Laplace Transform.
The definition of a step function.
DefinitionA function u is called a step function at t = 0 iff holds
u(t) =
{0 for t < 0,
1 for t > 0.
Example
Graph the step function values u(t) above, and the translationsu(t − c) and u(t + c) with c > 0.
Solution:u(t)
t
1
0
u(t − c)
t
1
0 c
u(t + c)
0
1
t− c
C
The definition of a step function.
DefinitionA function u is called a step function at t = 0 iff holds
u(t) =
{0 for t < 0,
1 for t > 0.
Example
Graph the step function values u(t) above, and the translationsu(t − c) and u(t + c) with c > 0.
Solution:u(t)
t
1
0
u(t − c)
t
1
0 c
u(t + c)
0
1
t− c
C
The definition of a step function.
DefinitionA function u is called a step function at t = 0 iff holds
u(t) =
{0 for t < 0,
1 for t > 0.
Example
Graph the step function values u(t) above, and the translationsu(t − c) and u(t + c) with c > 0.
Solution:u(t)
t
1
0
u(t − c)
t
1
0 c
u(t + c)
0
1
t− c
C
The definition of a step function.
DefinitionA function u is called a step function at t = 0 iff holds
u(t) =
{0 for t < 0,
1 for t > 0.
Example
Graph the step function values u(t) above, and the translationsu(t − c) and u(t + c) with c > 0.
Solution:u(t)
t
1
0
u(t − c)
t
1
0 c
u(t + c)
0
1
t− c
C
The definition of a step function.
DefinitionA function u is called a step function at t = 0 iff holds
u(t) =
{0 for t < 0,
1 for t > 0.
Example
Graph the step function values u(t) above, and the translationsu(t − c) and u(t + c) with c > 0.
Solution:u(t)
t
1
0
u(t − c)
t
1
0 c
u(t + c)
0
1
t− c
C
The definition of a step function.
Remark: Given any function values f (t) and c > 0, then f (t − c)is a right translation of f and f (t + c) is a left translation of f .
Example
f ( t ) = e
0 t
a t
1
f ( t ) f ( t ) = e
0 t
1
c
a ( t − c )f ( t )
a t
0 t
f ( t )
1
f ( t ) = u ( t ) e f ( t ) = u ( t − c ) e
0 t
1
c
a ( t − c )f ( t )
The definition of a step function.
Remark: Given any function values f (t) and c > 0, then f (t − c)is a right translation of f and f (t + c) is a left translation of f .
Example
f ( t ) = e
0 t
a t
1
f ( t )
f ( t ) = e
0 t
1
c
a ( t − c )f ( t )
a t
0 t
f ( t )
1
f ( t ) = u ( t ) e f ( t ) = u ( t − c ) e
0 t
1
c
a ( t − c )f ( t )
The definition of a step function.
Remark: Given any function values f (t) and c > 0, then f (t − c)is a right translation of f and f (t + c) is a left translation of f .
Example
f ( t ) = e
0 t
a t
1
f ( t ) f ( t ) = e
0 t
1
c
a ( t − c )f ( t )
a t
0 t
f ( t )
1
f ( t ) = u ( t ) e f ( t ) = u ( t − c ) e
0 t
1
c
a ( t − c )f ( t )
The definition of a step function.
Remark: Given any function values f (t) and c > 0, then f (t − c)is a right translation of f and f (t + c) is a left translation of f .
Example
f ( t ) = e
0 t
a t
1
f ( t ) f ( t ) = e
0 t
1
c
a ( t − c )f ( t )
a t
0 t
f ( t )
1
f ( t ) = u ( t ) e
f ( t ) = u ( t − c ) e
0 t
1
c
a ( t − c )f ( t )
The definition of a step function.
Remark: Given any function values f (t) and c > 0, then f (t − c)is a right translation of f and f (t + c) is a left translation of f .
Example
f ( t ) = e
0 t
a t
1
f ( t ) f ( t ) = e
0 t
1
c
a ( t − c )f ( t )
a t
0 t
f ( t )
1
f ( t ) = u ( t ) e f ( t ) = u ( t − c ) e
0 t
1
c
a ( t − c )f ( t )
The Laplace Transform of step functions (Sect. 4.3).
I Overview and notation.
I The definition of a step function.
I Piecewise discontinuous functions.
I The Laplace Transform of discontinuous functions.
I Properties of the Laplace Transform.
Piecewise discontinuous functions.
Example
Graph of the function b(t) = u(t − a)− u(t − b), with 0 < a < b.
Solution: The bump function b can be graphed as follows:
u(t −a)
0 a b
1
t
u(t −b)
0 a b
1
t
t0 a b
b(t)
1
C
Piecewise discontinuous functions.
Example
Graph of the function b(t) = u(t − a)− u(t − b), with 0 < a < b.
Solution: The bump function b can be graphed as follows:
u(t −a)
0 a b
1
t
u(t −b)
0 a b
1
t
t0 a b
b(t)
1
C
Piecewise discontinuous functions.
Example
Graph of the function b(t) = u(t − a)− u(t − b), with 0 < a < b.
Solution: The bump function b can be graphed as follows:
u(t −a)
0 a b
1
t
u(t −b)
0 a b
1
t
t0 a b
b(t)
1
C
Piecewise discontinuous functions.
Example
Graph of the function b(t) = u(t − a)− u(t − b), with 0 < a < b.
Solution: The bump function b can be graphed as follows:
u(t −a)
0 a b
1
t
u(t −b)
0 a b
1
t
t0 a b
b(t)
1
C
Piecewise discontinuous functions.
Example
Graph of the function f (t) = eat[u(t − 1)− u(t − 2)
].
Solution:
a t
t1 2
1
a t
f ( t ) = e [ u ( t −1 ) − u ( t −2 ) ]
[ u ( t −1 ) − u ( t −2 ) ]
e
y
Notation: It is common in the literature to denote the functionvalues u(t − c) as uc(t).
Piecewise discontinuous functions.
Example
Graph of the function f (t) = eat[u(t − 1)− u(t − 2)
].
Solution:
a t
t1 2
1
a t
f ( t ) = e [ u ( t −1 ) − u ( t −2 ) ]
[ u ( t −1 ) − u ( t −2 ) ]
e
y
Notation: It is common in the literature to denote the functionvalues u(t − c) as uc(t).
Piecewise discontinuous functions.
Example
Graph of the function f (t) = eat[u(t − 1)− u(t − 2)
].
Solution:
a t
t1 2
1
a t
f ( t ) = e [ u ( t −1 ) − u ( t −2 ) ]
[ u ( t −1 ) − u ( t −2 ) ]
e
y
Notation: It is common in the literature to denote the functionvalues u(t − c) as uc(t).
The Laplace Transform of step functions (Sect. 4.3).
I Overview and notation.
I The definition of a step function.
I Piecewise discontinuous functions.
I The Laplace Transform of discontinuous functions.
I Properties of the Laplace Transform.
The Laplace Transform of discontinuous functions.
TheoremGiven any real number c > 0, the following equation holds,
L[u(t − c)] =e−cs
s, s > 0.
Proof:
L[u(t − c)] =
∫ ∞
0
e−stu(t − c) dt =
∫ ∞
ce−st dt,
L[u(t − c)] = limN→∞
−1
s
(e−Ns − e−cs
)=
e−cs
s, s > 0.
We conclude that L[u(t − c)] =e−cs
s.
The Laplace Transform of discontinuous functions.
TheoremGiven any real number c > 0, the following equation holds,
L[u(t − c)] =e−cs
s, s > 0.
Proof:
L[u(t − c)] =
∫ ∞
0
e−stu(t − c) dt
=
∫ ∞
ce−st dt,
L[u(t − c)] = limN→∞
−1
s
(e−Ns − e−cs
)=
e−cs
s, s > 0.
We conclude that L[u(t − c)] =e−cs
s.
The Laplace Transform of discontinuous functions.
TheoremGiven any real number c > 0, the following equation holds,
L[u(t − c)] =e−cs
s, s > 0.
Proof:
L[u(t − c)] =
∫ ∞
0
e−stu(t − c) dt =
∫ ∞
ce−st dt,
L[u(t − c)] = limN→∞
−1
s
(e−Ns − e−cs
)=
e−cs
s, s > 0.
We conclude that L[u(t − c)] =e−cs
s.
The Laplace Transform of discontinuous functions.
TheoremGiven any real number c > 0, the following equation holds,
L[u(t − c)] =e−cs
s, s > 0.
Proof:
L[u(t − c)] =
∫ ∞
0
e−stu(t − c) dt =
∫ ∞
ce−st dt,
L[u(t − c)] = limN→∞
−1
s
(e−Ns − e−cs
)
=e−cs
s, s > 0.
We conclude that L[u(t − c)] =e−cs
s.
The Laplace Transform of discontinuous functions.
TheoremGiven any real number c > 0, the following equation holds,
L[u(t − c)] =e−cs
s, s > 0.
Proof:
L[u(t − c)] =
∫ ∞
0
e−stu(t − c) dt =
∫ ∞
ce−st dt,
L[u(t − c)] = limN→∞
−1
s
(e−Ns − e−cs
)=
e−cs
s, s > 0.
We conclude that L[u(t − c)] =e−cs
s.
The Laplace Transform of discontinuous functions.
Example
Compute L[3u(t − 2)].
Solution: L[3u(t − 2)] = 3L[u(t − 2)] = 3e−2s
s.
We conclude: L[3u(t − 2)] =3e−2s
s. C
Example
Compute L−1[2e−3s
s
].
Solution: Since L[u(t − c)] =e−cs
s, for c = 3 we get
L−1[e−3s
s
]= u(t − 3). Therefore, L−1
[2e−3s
s
]= 2u(t − 3). C
The Laplace Transform of discontinuous functions.
Example
Compute L[3u(t − 2)].
Solution: L[3u(t − 2)] = 3L[u(t − 2)]
= 3e−2s
s.
We conclude: L[3u(t − 2)] =3e−2s
s. C
Example
Compute L−1[2e−3s
s
].
Solution: Since L[u(t − c)] =e−cs
s, for c = 3 we get
L−1[e−3s
s
]= u(t − 3). Therefore, L−1
[2e−3s
s
]= 2u(t − 3). C
The Laplace Transform of discontinuous functions.
Example
Compute L[3u(t − 2)].
Solution: L[3u(t − 2)] = 3L[u(t − 2)] = 3e−2s
s.
We conclude: L[3u(t − 2)] =3e−2s
s. C
Example
Compute L−1[2e−3s
s
].
Solution: Since L[u(t − c)] =e−cs
s, for c = 3 we get
L−1[e−3s
s
]= u(t − 3). Therefore, L−1
[2e−3s
s
]= 2u(t − 3). C
The Laplace Transform of discontinuous functions.
Example
Compute L[3u(t − 2)].
Solution: L[3u(t − 2)] = 3L[u(t − 2)] = 3e−2s
s.
We conclude: L[3u(t − 2)] =3e−2s
s. C
Example
Compute L−1[2e−3s
s
].
Solution: Since L[u(t − c)] =e−cs
s, for c = 3 we get
L−1[e−3s
s
]= u(t − 3). Therefore, L−1
[2e−3s
s
]= 2u(t − 3). C
The Laplace Transform of discontinuous functions.
Example
Compute L[3u(t − 2)].
Solution: L[3u(t − 2)] = 3L[u(t − 2)] = 3e−2s
s.
We conclude: L[3u(t − 2)] =3e−2s
s. C
Example
Compute L−1[2e−3s
s
].
Solution: Since L[u(t − c)] =e−cs
s, for c = 3 we get
L−1[e−3s
s
]= u(t − 3). Therefore, L−1
[2e−3s
s
]= 2u(t − 3). C
The Laplace Transform of discontinuous functions.
Example
Compute L[3u(t − 2)].
Solution: L[3u(t − 2)] = 3L[u(t − 2)] = 3e−2s
s.
We conclude: L[3u(t − 2)] =3e−2s
s. C
Example
Compute L−1[2e−3s
s
].
Solution: Since L[u(t − c)] =e−cs
s,
for c = 3 we get
L−1[e−3s
s
]= u(t − 3). Therefore, L−1
[2e−3s
s
]= 2u(t − 3). C
The Laplace Transform of discontinuous functions.
Example
Compute L[3u(t − 2)].
Solution: L[3u(t − 2)] = 3L[u(t − 2)] = 3e−2s
s.
We conclude: L[3u(t − 2)] =3e−2s
s. C
Example
Compute L−1[2e−3s
s
].
Solution: Since L[u(t − c)] =e−cs
s, for c = 3 we get
L−1[e−3s
s
]
= u(t − 3). Therefore, L−1[2e−3s
s
]= 2u(t − 3). C
The Laplace Transform of discontinuous functions.
Example
Compute L[3u(t − 2)].
Solution: L[3u(t − 2)] = 3L[u(t − 2)] = 3e−2s
s.
We conclude: L[3u(t − 2)] =3e−2s
s. C
Example
Compute L−1[2e−3s
s
].
Solution: Since L[u(t − c)] =e−cs
s, for c = 3 we get
L−1[e−3s
s
]= u(t − 3).
Therefore, L−1[2e−3s
s
]= 2u(t − 3). C
The Laplace Transform of discontinuous functions.
Example
Compute L[3u(t − 2)].
Solution: L[3u(t − 2)] = 3L[u(t − 2)] = 3e−2s
s.
We conclude: L[3u(t − 2)] =3e−2s
s. C
Example
Compute L−1[2e−3s
s
].
Solution: Since L[u(t − c)] =e−cs
s, for c = 3 we get
L−1[e−3s
s
]= u(t − 3). Therefore, L−1
[2e−3s
s
]= 2u(t − 3). C
The Laplace Transform of step functions (Sect. 4.3).
I Overview and notation.
I The definition of a step function.
I Piecewise discontinuous functions.
I The Laplace Transform of discontinuous functions.
I Properties of the Laplace Transform.
Properties of the Laplace Transform.
Theorem (Translations)
If F (s) = L[f (t)] exists for s > a > 0 and c > 0, then holds
L[u(t − c)f (t − c)] = e−cs F (s), s > a.
Furthermore,
L[ect f (t)] = F (s − c), s > a + c .
Remark:
I L[translation (uf )
]= (exp)
(L[f ]
).
I L[(exp) (f )
]= translation
(L[f ]
).
Equivalent notation:
I L[u(t − c)f (t − c)] = e−cs L[f (t)],
I L[ect f (t)] = L[f ](s − c).
Properties of the Laplace Transform.
Theorem (Translations)
If F (s) = L[f (t)] exists for s > a > 0 and c > 0, then holds
L[u(t − c)f (t − c)] = e−cs F (s), s > a.
Furthermore,
L[ect f (t)] = F (s − c), s > a + c .
Remark:
I L[translation (uf )
]= (exp)
(L[f ]
).
I L[(exp) (f )
]= translation
(L[f ]
).
Equivalent notation:
I L[u(t − c)f (t − c)] = e−cs L[f (t)],
I L[ect f (t)] = L[f ](s − c).
Properties of the Laplace Transform.
Theorem (Translations)
If F (s) = L[f (t)] exists for s > a > 0 and c > 0, then holds
L[u(t − c)f (t − c)] = e−cs F (s), s > a.
Furthermore,
L[ect f (t)] = F (s − c), s > a + c .
Remark:
I L[translation (uf )
]= (exp)
(L[f ]
).
I L[(exp) (f )
]= translation
(L[f ]
).
Equivalent notation:
I L[u(t − c)f (t − c)] = e−cs L[f (t)],
I L[ect f (t)] = L[f ](s − c).
Properties of the Laplace Transform.
Theorem (Translations)
If F (s) = L[f (t)] exists for s > a > 0 and c > 0, then holds
L[u(t − c)f (t − c)] = e−cs F (s), s > a.
Furthermore,
L[ect f (t)] = F (s − c), s > a + c .
Remark:
I L[translation (uf )
]= (exp)
(L[f ]
).
I L[(exp) (f )
]= translation
(L[f ]
).
Equivalent notation:
I L[u(t − c)f (t − c)] = e−cs L[f (t)],
I L[ect f (t)] = L[f ](s − c).
Properties of the Laplace Transform.
Theorem (Translations)
If F (s) = L[f (t)] exists for s > a > 0 and c > 0, then holds
L[u(t − c)f (t − c)] = e−cs F (s), s > a.
Furthermore,
L[ect f (t)] = F (s − c), s > a + c .
Remark:
I L[translation (uf )
]= (exp)
(L[f ]
).
I L[(exp) (f )
]= translation
(L[f ]
).
Equivalent notation:
I L[u(t − c)f (t − c)] = e−cs L[f (t)],
I L[ect f (t)] = L[f ](s − c).
Properties of the Laplace Transform.
Example
Compute L[u(t − 2) sin(a(t − 2))
].
Solution: L[sin(at)] =a
s2 + a2, L[u(t − c)f (t − c)] = e−cs L[f (t)].
L[u(t − 2) sin(a(t − 2))
]= e−2s L[sin(at)] = e−2s a
s2 + a2.
We conclude: L[u(t − 2) sin(a(t − 2))
]= e−2s a
s2 + a2. C
Example
Compute L[e3t sin(at)
].
Solution: Recall: L[ect f (t)] = L[f ](s − c), L[sin(at)] =a
s2 + a2.
We conclude: L[e3t sin(at)
]=
a
(s − 3)2 + a2, with s > 3. C
Properties of the Laplace Transform.
Example
Compute L[u(t − 2) sin(a(t − 2))
].
Solution: L[sin(at)] =a
s2 + a2,
L[u(t − c)f (t − c)] = e−cs L[f (t)].
L[u(t − 2) sin(a(t − 2))
]= e−2s L[sin(at)] = e−2s a
s2 + a2.
We conclude: L[u(t − 2) sin(a(t − 2))
]= e−2s a
s2 + a2. C
Example
Compute L[e3t sin(at)
].
Solution: Recall: L[ect f (t)] = L[f ](s − c), L[sin(at)] =a
s2 + a2.
We conclude: L[e3t sin(at)
]=
a
(s − 3)2 + a2, with s > 3. C
Properties of the Laplace Transform.
Example
Compute L[u(t − 2) sin(a(t − 2))
].
Solution: L[sin(at)] =a
s2 + a2, L[u(t − c)f (t − c)] = e−cs L[f (t)].
L[u(t − 2) sin(a(t − 2))
]= e−2s L[sin(at)] = e−2s a
s2 + a2.
We conclude: L[u(t − 2) sin(a(t − 2))
]= e−2s a
s2 + a2. C
Example
Compute L[e3t sin(at)
].
Solution: Recall: L[ect f (t)] = L[f ](s − c), L[sin(at)] =a
s2 + a2.
We conclude: L[e3t sin(at)
]=
a
(s − 3)2 + a2, with s > 3. C
Properties of the Laplace Transform.
Example
Compute L[u(t − 2) sin(a(t − 2))
].
Solution: L[sin(at)] =a
s2 + a2, L[u(t − c)f (t − c)] = e−cs L[f (t)].
L[u(t − 2) sin(a(t − 2))
]= e−2s L[sin(at)]
= e−2s a
s2 + a2.
We conclude: L[u(t − 2) sin(a(t − 2))
]= e−2s a
s2 + a2. C
Example
Compute L[e3t sin(at)
].
Solution: Recall: L[ect f (t)] = L[f ](s − c), L[sin(at)] =a
s2 + a2.
We conclude: L[e3t sin(at)
]=
a
(s − 3)2 + a2, with s > 3. C
Properties of the Laplace Transform.
Example
Compute L[u(t − 2) sin(a(t − 2))
].
Solution: L[sin(at)] =a
s2 + a2, L[u(t − c)f (t − c)] = e−cs L[f (t)].
L[u(t − 2) sin(a(t − 2))
]= e−2s L[sin(at)] = e−2s a
s2 + a2.
We conclude: L[u(t − 2) sin(a(t − 2))
]= e−2s a
s2 + a2. C
Example
Compute L[e3t sin(at)
].
Solution: Recall: L[ect f (t)] = L[f ](s − c), L[sin(at)] =a
s2 + a2.
We conclude: L[e3t sin(at)
]=
a
(s − 3)2 + a2, with s > 3. C
Properties of the Laplace Transform.
Example
Compute L[u(t − 2) sin(a(t − 2))
].
Solution: L[sin(at)] =a
s2 + a2, L[u(t − c)f (t − c)] = e−cs L[f (t)].
L[u(t − 2) sin(a(t − 2))
]= e−2s L[sin(at)] = e−2s a
s2 + a2.
We conclude: L[u(t − 2) sin(a(t − 2))
]= e−2s a
s2 + a2. C
Example
Compute L[e3t sin(at)
].
Solution: Recall: L[ect f (t)] = L[f ](s − c), L[sin(at)] =a
s2 + a2.
We conclude: L[e3t sin(at)
]=
a
(s − 3)2 + a2, with s > 3. C
Properties of the Laplace Transform.
Example
Compute L[u(t − 2) sin(a(t − 2))
].
Solution: L[sin(at)] =a
s2 + a2, L[u(t − c)f (t − c)] = e−cs L[f (t)].
L[u(t − 2) sin(a(t − 2))
]= e−2s L[sin(at)] = e−2s a
s2 + a2.
We conclude: L[u(t − 2) sin(a(t − 2))
]= e−2s a
s2 + a2. C
Example
Compute L[e3t sin(at)
].
Solution: Recall: L[ect f (t)] = L[f ](s − c), L[sin(at)] =a
s2 + a2.
We conclude: L[e3t sin(at)
]=
a
(s − 3)2 + a2, with s > 3. C
Properties of the Laplace Transform.
Example
Compute L[u(t − 2) sin(a(t − 2))
].
Solution: L[sin(at)] =a
s2 + a2, L[u(t − c)f (t − c)] = e−cs L[f (t)].
L[u(t − 2) sin(a(t − 2))
]= e−2s L[sin(at)] = e−2s a
s2 + a2.
We conclude: L[u(t − 2) sin(a(t − 2))
]= e−2s a
s2 + a2. C
Example
Compute L[e3t sin(at)
].
Solution: Recall: L[ect f (t)] = L[f ](s − c),
L[sin(at)] =a
s2 + a2.
We conclude: L[e3t sin(at)
]=
a
(s − 3)2 + a2, with s > 3. C
Properties of the Laplace Transform.
Example
Compute L[u(t − 2) sin(a(t − 2))
].
Solution: L[sin(at)] =a
s2 + a2, L[u(t − c)f (t − c)] = e−cs L[f (t)].
L[u(t − 2) sin(a(t − 2))
]= e−2s L[sin(at)] = e−2s a
s2 + a2.
We conclude: L[u(t − 2) sin(a(t − 2))
]= e−2s a
s2 + a2. C
Example
Compute L[e3t sin(at)
].
Solution: Recall: L[ect f (t)] = L[f ](s − c), L[sin(at)] =a
s2 + a2.
We conclude: L[e3t sin(at)
]=
a
(s − 3)2 + a2, with s > 3. C
Properties of the Laplace Transform.
Example
Compute L[u(t − 2) sin(a(t − 2))
].
Solution: L[sin(at)] =a
s2 + a2, L[u(t − c)f (t − c)] = e−cs L[f (t)].
L[u(t − 2) sin(a(t − 2))
]= e−2s L[sin(at)] = e−2s a
s2 + a2.
We conclude: L[u(t − 2) sin(a(t − 2))
]= e−2s a
s2 + a2. C
Example
Compute L[e3t sin(at)
].
Solution: Recall: L[ect f (t)] = L[f ](s − c), L[sin(at)] =a
s2 + a2.
We conclude: L[e3t sin(at)
]=
a
(s − 3)2 + a2, with s > 3. C
Properties of the Laplace Transform.
Example
Find the Laplace transform of f (t) =
{0, t < 1,
(t2 − 2t + 2), t > 1.
Solution: Using step function notation,
f (t) = u(t − 1)(t2 − 2t + 2).
Completing the square we obtain,
t2 − 2t + 2 = (t2 − 2t + 1)− 1 + 2 = (t − 1)2 + 1.
This is a parabola t2 translated to theright by 1 and up by one. Because ofthe step function, this is a discontinuousfunction at t = 1.
1
10
f ( t )
t
Properties of the Laplace Transform.
Example
Find the Laplace transform of f (t) =
{0, t < 1,
(t2 − 2t + 2), t > 1.
Solution: Using step function notation,
f (t) = u(t − 1)(t2 − 2t + 2).
Completing the square we obtain,
t2 − 2t + 2 = (t2 − 2t + 1)− 1 + 2 = (t − 1)2 + 1.
This is a parabola t2 translated to theright by 1 and up by one. Because ofthe step function, this is a discontinuousfunction at t = 1.
1
10
f ( t )
t
Properties of the Laplace Transform.
Example
Find the Laplace transform of f (t) =
{0, t < 1,
(t2 − 2t + 2), t > 1.
Solution: Using step function notation,
f (t) = u(t − 1)(t2 − 2t + 2).
Completing the square we obtain,
t2 − 2t + 2 = (t2 − 2t + 1)− 1 + 2 = (t − 1)2 + 1.
This is a parabola t2 translated to theright by 1 and up by one. Because ofthe step function, this is a discontinuousfunction at t = 1.
1
10
f ( t )
t
Properties of the Laplace Transform.
Example
Find the Laplace transform of f (t) =
{0, t < 1,
(t2 − 2t + 2), t > 1.
Solution: Using step function notation,
f (t) = u(t − 1)(t2 − 2t + 2).
Completing the square we obtain,
t2 − 2t + 2 = (t2 − 2t + 1)− 1 + 2
= (t − 1)2 + 1.
This is a parabola t2 translated to theright by 1 and up by one. Because ofthe step function, this is a discontinuousfunction at t = 1.
1
10
f ( t )
t
Properties of the Laplace Transform.
Example
Find the Laplace transform of f (t) =
{0, t < 1,
(t2 − 2t + 2), t > 1.
Solution: Using step function notation,
f (t) = u(t − 1)(t2 − 2t + 2).
Completing the square we obtain,
t2 − 2t + 2 = (t2 − 2t + 1)− 1 + 2 = (t − 1)2 + 1.
This is a parabola t2 translated to theright by 1 and up by one. Because ofthe step function, this is a discontinuousfunction at t = 1.
1
10
f ( t )
t
Properties of the Laplace Transform.
Example
Find the Laplace transform of f (t) =
{0, t < 1,
(t2 − 2t + 2), t > 1.
Solution: Using step function notation,
f (t) = u(t − 1)(t2 − 2t + 2).
Completing the square we obtain,
t2 − 2t + 2 = (t2 − 2t + 1)− 1 + 2 = (t − 1)2 + 1.
This is a parabola t2 translated to theright by 1 and up by one.
Because ofthe step function, this is a discontinuousfunction at t = 1.
1
10
f ( t )
t
Properties of the Laplace Transform.
Example
Find the Laplace transform of f (t) =
{0, t < 1,
(t2 − 2t + 2), t > 1.
Solution: Using step function notation,
f (t) = u(t − 1)(t2 − 2t + 2).
Completing the square we obtain,
t2 − 2t + 2 = (t2 − 2t + 1)− 1 + 2 = (t − 1)2 + 1.
This is a parabola t2 translated to theright by 1 and up by one. Because ofthe step function, this is a discontinuousfunction at t = 1.
1
10
f ( t )
t
Properties of the Laplace Transform.
Example
Find the Laplace transform of f (t) =
{0, t < 1,
(t2 − 2t + 2), t > 1.
Solution: Using step function notation,
f (t) = u(t − 1)(t2 − 2t + 2).
Completing the square we obtain,
t2 − 2t + 2 = (t2 − 2t + 1)− 1 + 2 = (t − 1)2 + 1.
This is a parabola t2 translated to theright by 1 and up by one. Because ofthe step function, this is a discontinuousfunction at t = 1.
1
10
f ( t )
t
Properties of the Laplace Transform.
Example
Find the Laplace transform of f (t) =
{0, t < 1,
(t2 − 2t + 2), t > 1.
Solution: Recall: f (t) = u(t − 1)[(t − 1)2 + 1
].
This is equivalent to
f (t) = u(t − 1) (t − 1)2 + u(t − 1).
Since L[t2] = 2/s3, and L[u(t − c)g(t − c)] = e−cs L[g(t)], then
L[f (t)] = L[u(t − 1) (t − 1)2] + L[u(t − 1)] = e−s 2
s3+ e−s 1
s.
We conclude: L[f (t)] =e−s
s3
(2 + s2
). C
Properties of the Laplace Transform.
Example
Find the Laplace transform of f (t) =
{0, t < 1,
(t2 − 2t + 2), t > 1.
Solution: Recall: f (t) = u(t − 1)[(t − 1)2 + 1
].
This is equivalent to
f (t) = u(t − 1) (t − 1)2 + u(t − 1).
Since L[t2] = 2/s3, and L[u(t − c)g(t − c)] = e−cs L[g(t)], then
L[f (t)] = L[u(t − 1) (t − 1)2] + L[u(t − 1)] = e−s 2
s3+ e−s 1
s.
We conclude: L[f (t)] =e−s
s3
(2 + s2
). C
Properties of the Laplace Transform.
Example
Find the Laplace transform of f (t) =
{0, t < 1,
(t2 − 2t + 2), t > 1.
Solution: Recall: f (t) = u(t − 1)[(t − 1)2 + 1
].
This is equivalent to
f (t) = u(t − 1) (t − 1)2 + u(t − 1).
Since L[t2] = 2/s3,
and L[u(t − c)g(t − c)] = e−cs L[g(t)], then
L[f (t)] = L[u(t − 1) (t − 1)2] + L[u(t − 1)] = e−s 2
s3+ e−s 1
s.
We conclude: L[f (t)] =e−s
s3
(2 + s2
). C
Properties of the Laplace Transform.
Example
Find the Laplace transform of f (t) =
{0, t < 1,
(t2 − 2t + 2), t > 1.
Solution: Recall: f (t) = u(t − 1)[(t − 1)2 + 1
].
This is equivalent to
f (t) = u(t − 1) (t − 1)2 + u(t − 1).
Since L[t2] = 2/s3, and L[u(t − c)g(t − c)] = e−cs L[g(t)],
then
L[f (t)] = L[u(t − 1) (t − 1)2] + L[u(t − 1)] = e−s 2
s3+ e−s 1
s.
We conclude: L[f (t)] =e−s
s3
(2 + s2
). C
Properties of the Laplace Transform.
Example
Find the Laplace transform of f (t) =
{0, t < 1,
(t2 − 2t + 2), t > 1.
Solution: Recall: f (t) = u(t − 1)[(t − 1)2 + 1
].
This is equivalent to
f (t) = u(t − 1) (t − 1)2 + u(t − 1).
Since L[t2] = 2/s3, and L[u(t − c)g(t − c)] = e−cs L[g(t)], then
L[f (t)] = L[u(t − 1) (t − 1)2] + L[u(t − 1)]
= e−s 2
s3+ e−s 1
s.
We conclude: L[f (t)] =e−s
s3
(2 + s2
). C
Properties of the Laplace Transform.
Example
Find the Laplace transform of f (t) =
{0, t < 1,
(t2 − 2t + 2), t > 1.
Solution: Recall: f (t) = u(t − 1)[(t − 1)2 + 1
].
This is equivalent to
f (t) = u(t − 1) (t − 1)2 + u(t − 1).
Since L[t2] = 2/s3, and L[u(t − c)g(t − c)] = e−cs L[g(t)], then
L[f (t)] = L[u(t − 1) (t − 1)2] + L[u(t − 1)] = e−s 2
s3+ e−s 1
s.
We conclude: L[f (t)] =e−s
s3
(2 + s2
). C
Properties of the Laplace Transform.
Example
Find the Laplace transform of f (t) =
{0, t < 1,
(t2 − 2t + 2), t > 1.
Solution: Recall: f (t) = u(t − 1)[(t − 1)2 + 1
].
This is equivalent to
f (t) = u(t − 1) (t − 1)2 + u(t − 1).
Since L[t2] = 2/s3, and L[u(t − c)g(t − c)] = e−cs L[g(t)], then
L[f (t)] = L[u(t − 1) (t − 1)2] + L[u(t − 1)] = e−s 2
s3+ e−s 1
s.
We conclude: L[f (t)] =e−s
s3
(2 + s2
). C
Properties of the Laplace Transform.
Remark: The inverse of the formulas in the Theorem above are:
L−1[e−cs F (s)
]= u(t − c) f (t − c),
L−1[F (s − c)
]= ect f (t).
Example
Find L−1[ e−4s
s2 + 9
].
Solution: L−1[ e−4s
s2 + 9
]=
1
3L−1
[e−4s 3
s2 + 9
].
Recall: L−1[ a
s2 + a2
]= sin(at). Then, we conclude that
L−1[ e−4s
s2 + 9
]=
1
3u(t − 4) sin
(3(t − 4)
). C
Properties of the Laplace Transform.
Remark: The inverse of the formulas in the Theorem above are:
L−1[e−cs F (s)
]= u(t − c) f (t − c),
L−1[F (s − c)
]= ect f (t).
Example
Find L−1[ e−4s
s2 + 9
].
Solution: L−1[ e−4s
s2 + 9
]=
1
3L−1
[e−4s 3
s2 + 9
].
Recall: L−1[ a
s2 + a2
]= sin(at). Then, we conclude that
L−1[ e−4s
s2 + 9
]=
1
3u(t − 4) sin
(3(t − 4)
). C
Properties of the Laplace Transform.
Remark: The inverse of the formulas in the Theorem above are:
L−1[e−cs F (s)
]= u(t − c) f (t − c),
L−1[F (s − c)
]= ect f (t).
Example
Find L−1[ e−4s
s2 + 9
].
Solution: L−1[ e−4s
s2 + 9
]=
1
3L−1
[e−4s 3
s2 + 9
].
Recall: L−1[ a
s2 + a2
]= sin(at). Then, we conclude that
L−1[ e−4s
s2 + 9
]=
1
3u(t − 4) sin
(3(t − 4)
). C
Properties of the Laplace Transform.
Remark: The inverse of the formulas in the Theorem above are:
L−1[e−cs F (s)
]= u(t − c) f (t − c),
L−1[F (s − c)
]= ect f (t).
Example
Find L−1[ e−4s
s2 + 9
].
Solution: L−1[ e−4s
s2 + 9
]=
1
3L−1
[e−4s 3
s2 + 9
].
Recall: L−1[ a
s2 + a2
]= sin(at). Then, we conclude that
L−1[ e−4s
s2 + 9
]=
1
3u(t − 4) sin
(3(t − 4)
). C
Properties of the Laplace Transform.
Remark: The inverse of the formulas in the Theorem above are:
L−1[e−cs F (s)
]= u(t − c) f (t − c),
L−1[F (s − c)
]= ect f (t).
Example
Find L−1[ e−4s
s2 + 9
].
Solution: L−1[ e−4s
s2 + 9
]=
1
3L−1
[e−4s 3
s2 + 9
].
Recall: L−1[ a
s2 + a2
]= sin(at).
Then, we conclude that
L−1[ e−4s
s2 + 9
]=
1
3u(t − 4) sin
(3(t − 4)
). C
Properties of the Laplace Transform.
Remark: The inverse of the formulas in the Theorem above are:
L−1[e−cs F (s)
]= u(t − c) f (t − c),
L−1[F (s − c)
]= ect f (t).
Example
Find L−1[ e−4s
s2 + 9
].
Solution: L−1[ e−4s
s2 + 9
]=
1
3L−1
[e−4s 3
s2 + 9
].
Recall: L−1[ a
s2 + a2
]= sin(at). Then, we conclude that
L−1[ e−4s
s2 + 9
]=
1
3u(t − 4) sin
(3(t − 4)
). C
Properties of the Laplace Transform.
Example
Find L−1[ (s − 2)
(s − 2)2 + 9
].
Solution: L−1[ s
s2 + a2
]= cos(at), L−1
[F (s − c)
]= ect f (t).
We conclude: L−1[ (s − 2)
(s − 2)2 + 9
]= e2t cos(3t). C
Example
Find L−1[ 2e−3s
s2 − 4
].
Solution: Recall: L−1[ a
s2 − a2
]= sinh(at)
and L−1[e−cs F (s)
]= u(t − c) f (t − c).
Properties of the Laplace Transform.
Example
Find L−1[ (s − 2)
(s − 2)2 + 9
].
Solution: L−1[ s
s2 + a2
]= cos(at),
L−1[F (s − c)
]= ect f (t).
We conclude: L−1[ (s − 2)
(s − 2)2 + 9
]= e2t cos(3t). C
Example
Find L−1[ 2e−3s
s2 − 4
].
Solution: Recall: L−1[ a
s2 − a2
]= sinh(at)
and L−1[e−cs F (s)
]= u(t − c) f (t − c).
Properties of the Laplace Transform.
Example
Find L−1[ (s − 2)
(s − 2)2 + 9
].
Solution: L−1[ s
s2 + a2
]= cos(at), L−1
[F (s − c)
]= ect f (t).
We conclude: L−1[ (s − 2)
(s − 2)2 + 9
]= e2t cos(3t). C
Example
Find L−1[ 2e−3s
s2 − 4
].
Solution: Recall: L−1[ a
s2 − a2
]= sinh(at)
and L−1[e−cs F (s)
]= u(t − c) f (t − c).
Properties of the Laplace Transform.
Example
Find L−1[ (s − 2)
(s − 2)2 + 9
].
Solution: L−1[ s
s2 + a2
]= cos(at), L−1
[F (s − c)
]= ect f (t).
We conclude: L−1[ (s − 2)
(s − 2)2 + 9
]= e2t cos(3t). C
Example
Find L−1[ 2e−3s
s2 − 4
].
Solution: Recall: L−1[ a
s2 − a2
]= sinh(at)
and L−1[e−cs F (s)
]= u(t − c) f (t − c).
Properties of the Laplace Transform.
Example
Find L−1[ (s − 2)
(s − 2)2 + 9
].
Solution: L−1[ s
s2 + a2
]= cos(at), L−1
[F (s − c)
]= ect f (t).
We conclude: L−1[ (s − 2)
(s − 2)2 + 9
]= e2t cos(3t). C
Example
Find L−1[ 2e−3s
s2 − 4
].
Solution: Recall: L−1[ a
s2 − a2
]= sinh(at)
and L−1[e−cs F (s)
]= u(t − c) f (t − c).
Properties of the Laplace Transform.
Example
Find L−1[ (s − 2)
(s − 2)2 + 9
].
Solution: L−1[ s
s2 + a2
]= cos(at), L−1
[F (s − c)
]= ect f (t).
We conclude: L−1[ (s − 2)
(s − 2)2 + 9
]= e2t cos(3t). C
Example
Find L−1[ 2e−3s
s2 − 4
].
Solution: Recall: L−1[ a
s2 − a2
]= sinh(at)
and L−1[e−cs F (s)
]= u(t − c) f (t − c).
Properties of the Laplace Transform.
Example
Find L−1[ (s − 2)
(s − 2)2 + 9
].
Solution: L−1[ s
s2 + a2
]= cos(at), L−1
[F (s − c)
]= ect f (t).
We conclude: L−1[ (s − 2)
(s − 2)2 + 9
]= e2t cos(3t). C
Example
Find L−1[ 2e−3s
s2 − 4
].
Solution: Recall: L−1[ a
s2 − a2
]= sinh(at)
and L−1[e−cs F (s)
]= u(t − c) f (t − c).
Properties of the Laplace Transform.
Example
Find L−1[ 2e−3s
s2 − 4
].
Solution: Recall:
L−1[ a
s2 − a2
]= sinh(at), L−1
[e−cs F (s)
]= u(t − c) f (t − c).
L−1[ 2e−3s
s2 − 4
]= L−1
[e−3s 2
s2 − 4
].
We conclude: L−1[ 2e−3s
s2 − 4
]= u(t − 3) sinh
(2(t − 3)
). C
Properties of the Laplace Transform.
Example
Find L−1[ 2e−3s
s2 − 4
].
Solution: Recall:
L−1[ a
s2 − a2
]= sinh(at), L−1
[e−cs F (s)
]= u(t − c) f (t − c).
L−1[ 2e−3s
s2 − 4
]= L−1
[e−3s 2
s2 − 4
].
We conclude: L−1[ 2e−3s
s2 − 4
]= u(t − 3) sinh
(2(t − 3)
). C
Properties of the Laplace Transform.
Example
Find L−1[ 2e−3s
s2 − 4
].
Solution: Recall:
L−1[ a
s2 − a2
]= sinh(at), L−1
[e−cs F (s)
]= u(t − c) f (t − c).
L−1[ 2e−3s
s2 − 4
]= L−1
[e−3s 2
s2 − 4
].
We conclude: L−1[ 2e−3s
s2 − 4
]= u(t − 3) sinh
(2(t − 3)
). C
Properties of the Laplace Transform.
Example
Find L−1[ e−2s
s2 + s − 2
].
Solution: Find the roots of the denominator:
s± =1
2
[−1±
√1 + 8
]⇒
{s+ = 1,
s− = −2.
Therefore, s2 + s − 2 = (s − 1) (s + 2).
Use partial fractions to simplify the rational function:
1
s2 + s − 2=
1
(s − 1) (s + 2)=
a
(s − 1)+
b
(s + 2),
1
s2 + s − 2= a(s + 2) + b(s − 1) =
(a + b) s + (2a− b)
(s − 1) (s + 2).
Properties of the Laplace Transform.
Example
Find L−1[ e−2s
s2 + s − 2
].
Solution: Find the roots of the denominator:
s± =1
2
[−1±
√1 + 8
]
⇒
{s+ = 1,
s− = −2.
Therefore, s2 + s − 2 = (s − 1) (s + 2).
Use partial fractions to simplify the rational function:
1
s2 + s − 2=
1
(s − 1) (s + 2)=
a
(s − 1)+
b
(s + 2),
1
s2 + s − 2= a(s + 2) + b(s − 1) =
(a + b) s + (2a− b)
(s − 1) (s + 2).
Properties of the Laplace Transform.
Example
Find L−1[ e−2s
s2 + s − 2
].
Solution: Find the roots of the denominator:
s± =1
2
[−1±
√1 + 8
]⇒
{s+ = 1,
s− = −2.
Therefore, s2 + s − 2 = (s − 1) (s + 2).
Use partial fractions to simplify the rational function:
1
s2 + s − 2=
1
(s − 1) (s + 2)=
a
(s − 1)+
b
(s + 2),
1
s2 + s − 2= a(s + 2) + b(s − 1) =
(a + b) s + (2a− b)
(s − 1) (s + 2).
Properties of the Laplace Transform.
Example
Find L−1[ e−2s
s2 + s − 2
].
Solution: Find the roots of the denominator:
s± =1
2
[−1±
√1 + 8
]⇒
{s+ = 1,
s− = −2.
Therefore, s2 + s − 2 = (s − 1) (s + 2).
Use partial fractions to simplify the rational function:
1
s2 + s − 2=
1
(s − 1) (s + 2)=
a
(s − 1)+
b
(s + 2),
1
s2 + s − 2= a(s + 2) + b(s − 1) =
(a + b) s + (2a− b)
(s − 1) (s + 2).
Properties of the Laplace Transform.
Example
Find L−1[ e−2s
s2 + s − 2
].
Solution: Find the roots of the denominator:
s± =1
2
[−1±
√1 + 8
]⇒
{s+ = 1,
s− = −2.
Therefore, s2 + s − 2 = (s − 1) (s + 2).
Use partial fractions to simplify the rational function:
1
s2 + s − 2=
1
(s − 1) (s + 2)
=a
(s − 1)+
b
(s + 2),
1
s2 + s − 2= a(s + 2) + b(s − 1) =
(a + b) s + (2a− b)
(s − 1) (s + 2).
Properties of the Laplace Transform.
Example
Find L−1[ e−2s
s2 + s − 2
].
Solution: Find the roots of the denominator:
s± =1
2
[−1±
√1 + 8
]⇒
{s+ = 1,
s− = −2.
Therefore, s2 + s − 2 = (s − 1) (s + 2).
Use partial fractions to simplify the rational function:
1
s2 + s − 2=
1
(s − 1) (s + 2)=
a
(s − 1)+
b
(s + 2),
1
s2 + s − 2= a(s + 2) + b(s − 1) =
(a + b) s + (2a− b)
(s − 1) (s + 2).
Properties of the Laplace Transform.
Example
Find L−1[ e−2s
s2 + s − 2
].
Solution: Find the roots of the denominator:
s± =1
2
[−1±
√1 + 8
]⇒
{s+ = 1,
s− = −2.
Therefore, s2 + s − 2 = (s − 1) (s + 2).
Use partial fractions to simplify the rational function:
1
s2 + s − 2=
1
(s − 1) (s + 2)=
a
(s − 1)+
b
(s + 2),
1
s2 + s − 2= a(s + 2) + b(s − 1)
=(a + b) s + (2a− b)
(s − 1) (s + 2).
Properties of the Laplace Transform.
Example
Find L−1[ e−2s
s2 + s − 2
].
Solution: Find the roots of the denominator:
s± =1
2
[−1±
√1 + 8
]⇒
{s+ = 1,
s− = −2.
Therefore, s2 + s − 2 = (s − 1) (s + 2).
Use partial fractions to simplify the rational function:
1
s2 + s − 2=
1
(s − 1) (s + 2)=
a
(s − 1)+
b
(s + 2),
1
s2 + s − 2= a(s + 2) + b(s − 1) =
(a + b) s + (2a− b)
(s − 1) (s + 2).
Properties of the Laplace Transform.
Example
Find L−1[ e−2s
s2 + s − 2
].
Solution: Recall:1
s2 + s − 2=
(a + b) s + (2a− b)
(s − 1) (s + 2)
a + b = 0, 2a− b = 1, ⇒ a =1
3, b = −1
3.
L−1[ e−2s
s2 + s − 2
]=
1
3L−1
[e−2s 1
s − 1
]− 1
3L−1
[e−2s 1
s + 2
].
Recall: L−1[ 1
s − a
]= eat , L−1
[e−cs F (s)
]= u(t − c) f (t − c),
L−1[ e−2s
s2 + s − 2
]=
1
3u(t − 2) e(t−2) − 1
3u(t − 2) e−2(t−2).
Hence: L−1[ e−2s
s2 + s − 2
]=
1
3u(t − 2)
[e(t−2) − e−2(t−2)
]. C
Properties of the Laplace Transform.
Example
Find L−1[ e−2s
s2 + s − 2
].
Solution: Recall:1
s2 + s − 2=
(a + b) s + (2a− b)
(s − 1) (s + 2)
a + b = 0,
2a− b = 1, ⇒ a =1
3, b = −1
3.
L−1[ e−2s
s2 + s − 2
]=
1
3L−1
[e−2s 1
s − 1
]− 1
3L−1
[e−2s 1
s + 2
].
Recall: L−1[ 1
s − a
]= eat , L−1
[e−cs F (s)
]= u(t − c) f (t − c),
L−1[ e−2s
s2 + s − 2
]=
1
3u(t − 2) e(t−2) − 1
3u(t − 2) e−2(t−2).
Hence: L−1[ e−2s
s2 + s − 2
]=
1
3u(t − 2)
[e(t−2) − e−2(t−2)
]. C
Properties of the Laplace Transform.
Example
Find L−1[ e−2s
s2 + s − 2
].
Solution: Recall:1
s2 + s − 2=
(a + b) s + (2a− b)
(s − 1) (s + 2)
a + b = 0, 2a− b = 1,
⇒ a =1
3, b = −1
3.
L−1[ e−2s
s2 + s − 2
]=
1
3L−1
[e−2s 1
s − 1
]− 1
3L−1
[e−2s 1
s + 2
].
Recall: L−1[ 1
s − a
]= eat , L−1
[e−cs F (s)
]= u(t − c) f (t − c),
L−1[ e−2s
s2 + s − 2
]=
1
3u(t − 2) e(t−2) − 1
3u(t − 2) e−2(t−2).
Hence: L−1[ e−2s
s2 + s − 2
]=
1
3u(t − 2)
[e(t−2) − e−2(t−2)
]. C
Properties of the Laplace Transform.
Example
Find L−1[ e−2s
s2 + s − 2
].
Solution: Recall:1
s2 + s − 2=
(a + b) s + (2a− b)
(s − 1) (s + 2)
a + b = 0, 2a− b = 1, ⇒ a =1
3, b = −1
3.
L−1[ e−2s
s2 + s − 2
]=
1
3L−1
[e−2s 1
s − 1
]− 1
3L−1
[e−2s 1
s + 2
].
Recall: L−1[ 1
s − a
]= eat , L−1
[e−cs F (s)
]= u(t − c) f (t − c),
L−1[ e−2s
s2 + s − 2
]=
1
3u(t − 2) e(t−2) − 1
3u(t − 2) e−2(t−2).
Hence: L−1[ e−2s
s2 + s − 2
]=
1
3u(t − 2)
[e(t−2) − e−2(t−2)
]. C
Properties of the Laplace Transform.
Example
Find L−1[ e−2s
s2 + s − 2
].
Solution: Recall:1
s2 + s − 2=
(a + b) s + (2a− b)
(s − 1) (s + 2)
a + b = 0, 2a− b = 1, ⇒ a =1
3, b = −1
3.
L−1[ e−2s
s2 + s − 2
]=
1
3L−1
[e−2s 1
s − 1
]− 1
3L−1
[e−2s 1
s + 2
].
Recall: L−1[ 1
s − a
]= eat , L−1
[e−cs F (s)
]= u(t − c) f (t − c),
L−1[ e−2s
s2 + s − 2
]=
1
3u(t − 2) e(t−2) − 1
3u(t − 2) e−2(t−2).
Hence: L−1[ e−2s
s2 + s − 2
]=
1
3u(t − 2)
[e(t−2) − e−2(t−2)
]. C
Properties of the Laplace Transform.
Example
Find L−1[ e−2s
s2 + s − 2
].
Solution: Recall:1
s2 + s − 2=
(a + b) s + (2a− b)
(s − 1) (s + 2)
a + b = 0, 2a− b = 1, ⇒ a =1
3, b = −1
3.
L−1[ e−2s
s2 + s − 2
]=
1
3L−1
[e−2s 1
s − 1
]− 1
3L−1
[e−2s 1
s + 2
].
Recall: L−1[ 1
s − a
]= eat ,
L−1[e−cs F (s)
]= u(t − c) f (t − c),
L−1[ e−2s
s2 + s − 2
]=
1
3u(t − 2) e(t−2) − 1
3u(t − 2) e−2(t−2).
Hence: L−1[ e−2s
s2 + s − 2
]=
1
3u(t − 2)
[e(t−2) − e−2(t−2)
]. C
Properties of the Laplace Transform.
Example
Find L−1[ e−2s
s2 + s − 2
].
Solution: Recall:1
s2 + s − 2=
(a + b) s + (2a− b)
(s − 1) (s + 2)
a + b = 0, 2a− b = 1, ⇒ a =1
3, b = −1
3.
L−1[ e−2s
s2 + s − 2
]=
1
3L−1
[e−2s 1
s − 1
]− 1
3L−1
[e−2s 1
s + 2
].
Recall: L−1[ 1
s − a
]= eat , L−1
[e−cs F (s)
]= u(t − c) f (t − c),
L−1[ e−2s
s2 + s − 2
]=
1
3u(t − 2) e(t−2) − 1
3u(t − 2) e−2(t−2).
Hence: L−1[ e−2s
s2 + s − 2
]=
1
3u(t − 2)
[e(t−2) − e−2(t−2)
]. C
Properties of the Laplace Transform.
Example
Find L−1[ e−2s
s2 + s − 2
].
Solution: Recall:1
s2 + s − 2=
(a + b) s + (2a− b)
(s − 1) (s + 2)
a + b = 0, 2a− b = 1, ⇒ a =1
3, b = −1
3.
L−1[ e−2s
s2 + s − 2
]=
1
3L−1
[e−2s 1
s − 1
]− 1
3L−1
[e−2s 1
s + 2
].
Recall: L−1[ 1
s − a
]= eat , L−1
[e−cs F (s)
]= u(t − c) f (t − c),
L−1[ e−2s
s2 + s − 2
]=
1
3u(t − 2) e(t−2) − 1
3u(t − 2) e−2(t−2).
Hence: L−1[ e−2s
s2 + s − 2
]=
1
3u(t − 2)
[e(t−2) − e−2(t−2)
]. C
Properties of the Laplace Transform.
Example
Find L−1[ e−2s
s2 + s − 2
].
Solution: Recall:1
s2 + s − 2=
(a + b) s + (2a− b)
(s − 1) (s + 2)
a + b = 0, 2a− b = 1, ⇒ a =1
3, b = −1
3.
L−1[ e−2s
s2 + s − 2
]=
1
3L−1
[e−2s 1
s − 1
]− 1
3L−1
[e−2s 1
s + 2
].
Recall: L−1[ 1
s − a
]= eat , L−1
[e−cs F (s)
]= u(t − c) f (t − c),
L−1[ e−2s
s2 + s − 2
]=
1
3u(t − 2) e(t−2) − 1
3u(t − 2) e−2(t−2).
Hence: L−1[ e−2s
s2 + s − 2
]=
1
3u(t − 2)
[e(t−2) − e−2(t−2)
]. C