Part 1 - Properties of Laplace Transform

Page 1

DIFFERENTIAL EQUATIONS 2.1

PROPERTIES OF LAPLACE TRANSFORMATION

Let f be a function defined for t ≥ 0. Then the integral 

e

ℒ{ f(t)} =

 st

f (t ) dt

0

is said to be the Laplace transform of f, provided the integral converges.

Transforms of Some Basic Functions. (a) ℒ{1} = (c) ℒ{eat} =

1 s

(b) ℒ{tn} = n!/sn+1, n = 1, 2, 3, …

1 sa

(e) ℒ{cos kt} =

s s  k2

(g) ℒ{cosh kt} =

2

(d) ℒ{sin kt} =

k s  k2

(f) ℒ{sinh kt} =

k s  k2

2

2

s s  k2 2

Theorem 2.1.1: Linearity Property ℒ is a linear transform. From a linear combination of functions we can write 

 e af (t )  st

 bg (t ) dt  a  e

0

0

 st

f (t )dt  b  e st g (t )dt 0

whenever both integrals converge for s > c. Hence it follows that ℒ af (t )  bg (t )  aℒ  f (t ) + bℒ g (t ) = aF(s) + bG(s)

(1)

First Translation Theorem Theorem 2.1.2: First-Shift Property If ℒ{ f(t)} = F(s) exists for s > c, and a is any real number, then ℒ{ e at f (t ) } = ℒ  f (t ) ssa = F(s  a) for s > c + a.

(2)


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