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 sa
(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 ) ssa = F(s a) for s > c + a.
(2)