(306557551) laplace (12) (1)

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S. Boyd EE10 2 Lecture 3 The Laplace transfo rm definition & examples properties & formulas – linearity – the inverse Laplace transform – time scaling – exponential scaling – time delay – derivative – integral – multiplication by t – convolution 3– 1

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Page 1: (306557551) laplace (12) (1)

S. Boyd EE102

Lecture 3The Laplace transform

definition & examples•

properties & formulas

– linearity– the inverse Laplace transform– time scaling– exponential scaling– time delay– derivative– integral– multiplication by t– convolution

3–1

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Idea

the Laplace transform converts integral and differentialalgebraic equations

equations into

this is like phasors, but

• applies to general signals, not just

sinusoids

• handles non-steady-state conditionsallows us to analyze

• LCCODEs

• complicated

• complicated

circuits with sources, Ls,

systems with integrators,

Rs, and Cs

differentiators, gains

The Laplace transform 3–2

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Complex

complex number in Cartesian form: z

• x = <z, the real part of z

• y = =z, the imaginary part of z

• j = √−1 (engineering notation);

numbers

= x + jy

= √−1 is polite term in mixedicompany

rejφcomplex number in polar form: z =

• r is the modulus or magnitude of z

• φ is the angle or phase of z

• exp(jφ) = cos φ + j sin φ

complex exponential of z = x + jy:

ez ex+jy exejy ex(cos y= = = + j sin y)

The Laplace transform 3–3

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The Laplace transform

defined for t ≥ 0

signal (function) f is the

we’ll be interested in signals

function F = L(f )the Laplace transform of adefined by Z ∞

f (t)e−st dtF (s) =0

for those s ∈ C for which the integral makes sense

• F is a complex-valued function of complex numbers

• s is called the (complex) frequency variable, with units sec−1; t is calledthe time variable (in sec); st is unitless

• for now, we assume f contains no impulses at t = 0

common notation convention: lower case letter denotes signal; capitalletter denotes its Laplace transform, e.g., U denotes L(u),L(vin), etc.

The Laplace transform

Vin denotes

3–4

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Example

let’s find Laplace transform of f (t) = et:¯Z Z ∞¯0

1 e(1−s)t 1 ∞ ∞

et e−st e(1−s)tF (s) = dt = = =dt1 − s

which

s − 1¯0 0

e(1−s)t → 0 as t → ∞, is true for <s > 1:provided we can say¯

(1−s)t¯ ¯

−j(=s)t¯ ¯

(1−<s)t¯

(1−<s)t= ¯e =¯¯e

¯ ¯ ¯ ¯ ¯e¯

e¯ ¯ ¯|

=z

1

• the integral defining F makes sense for all s ∈ C with <s > 1 (the‘region of convergence’ of F )

• but the resulting formula for F makes sense for all s ∈ C except s = 1

we’ll ignore these (sometimes important) details and just say that

1L(et) =

s − 1

The Laplace transform 3–5

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More examples

constant: (or unit step) f (t) = 1 (for t ≥ 0)

¯∞Z1 1∞ ¯

e−st e−stF (s) = dt = − =¯s s¯

00

e−st → 0 as t → ∞, which is true for <s > 0 sinceprovided we can say¯

−j(=s)t¯ ¯

−(<s)t¯¯ ¯

¯e−st¯ −(<s)t= ¯e = e¯ ¯ ¯ ¯e

¯¯ ¯

|=z

1

0• the integral defining F makes sense for all s with <s >

• but the resulting formula for F makes sense for all s except s = 0

The Laplace transform 3–6

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sinusoid: first express f (t) = cos ωt as

f (t) = (1/2)ejωt + (1/2)e−jωt

now we can find F asZ ∞

e−st ¡(1/2)ejωt + (1/2)e−jωt¢ dtF (s) =

0 Z Z∞ ∞

e(−s+jω)t e(−s−jω)t= (1/2) dt + (1/2) dt0 0

1 1= (1/2) + (1/2)

s + jωs − jω s

=s2 ω2+

> 0; OK for s = ±jω)(valid for <s final formula

The Laplace transform 3–7

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tnpowers of t: f (t) = (n ≥ 1)

we’ll integrate by parts, i.e., use¯bb bZ Z

u(t)v0(t) dt = u(t)v(t)¯

v(t)u0(t) dt¯ −¯aa a

with u(t) = tn, v0(t) = e−st, a = 0, b = ∞µ −e−st ¶¯∞

Z Z ∞ n ∞¯tne−st tn

n s

tn−1e−stF (s) = dt = + dt¯sn−1

s¯00 0

= L(t )

tne−st → 0 <s > 0provided if t → ∞, which is truewe obtain

forapplying the formula recusively,

n! F (s) =

sn+1

valid for <s > 0;

The Laplace transform

final formula OK for all s = 0

3–8

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Impulses at t = 0

if f contains impulses at t = 0 we choose to include them in the integral defining F :

Z ∞

f (t)e−st dtF (s) =0−

(you can also choose to not include them, but this changes we’ll see & use)

example: impulse function, f = δZ

some formulas

e−st¯δ(t)e−st dt =F (s) = = 1¯t=0

0−

δ(k)similarly for f = we have¯Z

k∞

= (−1)k d e−st¯ ske−st¯δ(k)(t)e−st skF (s) = = =dt ¯ ¯

t=0kdt ¯t=00−

The Laplace transform 3–9

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Linearity

the Laplace transform is linear : if f and g arescalar, we have

any signals, and a is any

L(af ) = aF,

i.e., homogeneity & superposition

L(f + g)

hold

= F + G

example:

L ¡3δ(t) − 2et¢ 3L(δ(t)) − 2L(et)=

2= 3 −

s − 13s − 5=s − 1

The Laplace transform 3–10

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One-to-one property

the Laplace transform is one-to-one : if L(f ) = L(g)(well, almost; see below)

f =then g

• F determines f

• inverse Laplace transform(not easy to show)

L−1 is well defined

example (previous page):µ

3s − 5¶L−1 t= 3δ(t) − 2e

s − 1

in other words, the only function f such that

3s − 5F (s) =s − 1

is f (t) = 3δ(t) − 2et

The Laplace transform 3–11

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what ‘almost’ means: if f and g differ only at a finite number of pointsimpulses) then F = G(where there aren’t

examples:

• f defined as ½10

t = 2t = 2f (t) =

has F = 0

• f defined as ½1/21

=>

00

ttf (t) =

has F = 1/s (same as unit step)

The Laplace transform 3–12

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Inverse Laplace transform

in principle we can recover f from F via

σ+j∞Z1 stf (t) = F (s)e ds

2πj σ−j∞

enough that F (s) is definedwhere σ is large for <s ≥ σ

surprisingly, this formula isn’t really useful!

The Laplace transform 3–13

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Time scaling

define signal g by g(t) = f (at), where a > 0; then

G(s) = (1/a)F (s/a)

scaled by a, frequencies by 1/amakes sense: times are

let’s check:Z Z∞ ∞

f (at)e−st f (τ )e−(s/a)τG(s) = dt = (1/a) = (1/a)F (s/a)dτ0 0

where τ = at

example: L(et) = 1/(s − 1) so

L(eat) = (1/a)1 1

=(s/a) − 1 s − a

The Laplace transform 3–14

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Exponential scaling

let f be a signal and a a scalar, and define g(t) = eatf (t); then

G(s) = F (s − a)

let’s check:Z Z∞ ∞

e−steatf (t) e−(s−a)tf (t)G(s) = dt = dt = F (s − a)0 0

example: L(cos t) = s/(s2 + 1), and hence

s + 1 + 1sL(e−t cos t) = =(s + 1)2 + 1 s2 + 2s + 2

The Laplace transform 3–15

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Time delay

let f be a signal and T > 0; define the signal g as½

0f (t − T )

0 ≤ t < Tt ≥ Tg(t) =

(g is f , delayed by T seconds & ‘zero-padded’ up to T )

f (t) g(t)

t tt = T

The Laplace transform 3–16

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then we have G(s) = e−sT F (s)

derivation:Z Z∞ ∞

e−stg(t) e−stf (t − T ) dt

e−s(τ +T )f (τ )

G(s) = =dt0 T

∞Z

= dτ0

e−sT F (s)=

The Laplace transform 3–17

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example: let’s find the Laplace transform of a rectangular pulse signal½

10

if a ≤ t ≤otherwise

bf (t) =

where 0 < a < b

we can write f as f = f1 − f2 where½ ½

10

10

t ≥ at < a

tt

≥ b< bf1(t) = f2(t) =

i.e., f is a unit step delayed

hence

a seconds, minus a unit step delayed b seconds

F (s) = L(f1) − L(f2)

e− − e as −bs=

s

(can check by direct integration)

The Laplace transform 3–18

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Derivative

if signal f is continuous at t = 0, then

L(f 0) = sF (s) − f (0)

• time-domain differentiation becomes multiplicationvariable s (as with phasors)

by frequency

• plus a term that includes initial condition (i.e., −f (0))

higher-order derivatives: applying derivative formula twice yields

L(f 00) ==

=

sL(f 0) − f 0(0)

s(sF (s) − f (0)) − f 0(0)

s2F (s) − sf (0) − f 0(0)

similar formulas hold for L(f (k))

The Laplace transform 3–19

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examples

• f (t) = et, etso f 0(t) = and

1L(f ) = L(f 0) =

1

s − 1

which isusing the formula, L(f 0) = s(s

) − 1,1 the same−

1 d−• sin ωt = cos ωt, soω dtµ ¶

− 1

=

1 s ωL(sin ωt) = −ω

ss2 ω2 s2 ω2+ +

• f is unit ramp, so f 0 is unit stepµ ¶

1L(f 0) = s 0 = 1/s−s2

The Laplace transform 3–20

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derivation of derivative formula: start from the defining integralZ ∞

f 0(t)e−stdtG(s) =0

integration by parts yieldsZ ∞

e−stf (t)¯∞ − f (t)(−se−st)G(s) = dt¯

00

lim f (t)e−st − f (0) + sF (s)=t→∞

for <s large enough the limit is zero, and we recover the formula

G(s) = sF (s) − f (0)

The Laplace transform 3–21

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derivative formula for discontinuous functions

if signal f is discontinuous at t = 0, then

L(f 0) = sF (s) − f (0−)

so f 0(t) = δ(t)example: f is unit step,

µ1

L(f 0) = − 0 = 1ss

The Laplace transform 3–22

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Example: RC circuit

yu 1F

t = 0, i.e., y(0) = 0• capacitor is uncharged at

• u(t) is a unit step

from last lecture,y0(t) + y(t) = u(t)

take Laplace transform, term by term:

sY (s) + Y (s) = 1/s

(using y(0) = 0 and U (s) = 1/s)

The Laplace transform 3–23

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solve for Y (s) (just algebra!) to get

1/s 1Y (s) = =

s + 1 s(s + 1)

to find y, we first express Y as

1 1Y (s) = − s + 1s

(check!)

therefore we have

y(t) = L−1(1/s) − L−1(1/(s + 1)) = 1 − e−t

Laplace transform turned a differential equation into an algebraic equation(more on this later)

The Laplace transform 3–24

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Integral

let g be the running integral of a signal f , i.e.,

tZ

g(t) = f (τ ) dτ0

then1

G(s) = F (s)s

integral becomes division by frequency variable s

i.e., time-domain

example: f = δ, so F (s) = 1; g is the unit step function

G(s) = 1/s

example: f is unit step function, so F (s) =function (g(t) = t for t ≥ 0),

G(s) = 1/s2

1/s; g is the unit ramp

The Laplace transform 3–25

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derivation of integral formula:

t tµZ ¶Z Z Z∞ ∞

e−st f (τ )e−st dτG(s) = f (τ ) dτ dt = dtt=0 τ =0 t=0 τ =0

over the triangle 0here we integrate horizontally firstt

≤ τ ≤ t

τ

switch the order, i.e., integratelet’s vertically first:Z µZ ¶

dt dτZ Z∞ ∞ ∞ ∞

f (τ )e−st e−stG(s) = = f (τ )dt dττ =0 t=τ τ =0

∞t=τZ

f (τ )(1/s)e−sτ dτ=τ =0

F (s)/s

=

The Laplace transform 3–26

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Multiplication by t

let f be a signal and define

g(t) = tf (t)

then we haveG(s) = −F 0(s)

just differentiate both sides ofto verify formula,Z ∞

e−stf (t) dtF (s) =0

with respect to s to getZ ∞

(−t)e−stf (t) dtF 0(s) =0

The Laplace transform 3–27

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examples

e−t, te−t• f (t) = g(t) =

1 1 d− L(te−t) = =(s + 1)2s + 1ds

= te−t, t2e−t• f (t) g(t) =

1 2 d− L(t2e−t) = =(s + 1)2 (s + 1)3ds

• in general, (k − 1)!

L(tke−t) =(s + 1)k+1

The Laplace transform 3–28

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Convolution

signals f and g, denoted h = f ∗ g, isthe convolution of the signal

tZ

h(t) = f (τ )g(t − τ ) dτ0

tZ

as h(t) = f (t − τ )g(τ ) dτ ; insame other words,•0

f ∗ g = g ∗ f

(very great) importance will soon become clear•

in terms of Laplace transforms:

H (s) = F (s)G(s)

Laplace transform turns convolution into multiplication

The Laplace transform 3–29

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let’s show that L(f

H (s)

∗ g)

=

=Z

F (s)G(s):t

µZ ¶∞

e−st

t

f (τ )g(t − τ ) dτ dtt=0

∞τ =0

Z Z

e−stf (τ )g(t − τ ) dτ dt=t=0 τ =0

the triangle 0 ≤ τ ≤ twhere we integrate overZ Z∞ ∞

e−stf (τ )g(t − τ ) dt dτH (s) =change order of integration:•τ =0 t=τ

t = t − τ ; dt = dt; region of integration becomeschange variable t to•≥ 0, ≥ 0τ t

Z Z∞ ∞

e−s(t+τ )f (τ )g(t) dtH (s) = dττ =0

µZt=0

¶ µZ ¶∞ ∞

e−sτ f (τ ) e−stg(t)= dτ dtτ =0 t=0

= F (s)G(s)

The Laplace transform 3–30

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examples

f = δ, F (s) = 1, gives•H (s) = G(s),

which is consistent withZ t

δ(τ )g(t − τ )dτ = g(t)0

f (t) = 1, F (s) = e−sT /s, gives•

H (s) = G(s)/s

which is consistent withtZ

h(t) = g(τ ) dτ0

more interesting examples later in the course . . .•

The Laplace transform 3–31

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Finding the Laplace transform

you should know the Laplace transforms of some basic signals, e.g.,

• unit step (F (s) = 1/s), impulse function (F (s) = 1)

• exponential: L(eat) = 1/(s − a)

• sinusoids L(cos ωt) = s/(s2 + ω2), L(sin ωt) = ω/(s2 + ω2)

these, combined with a table of Laplace transforms and the propertiesgiven above (linearity, scaling, . . . ) will get you pretty far

and of course you can always integrate, using the defining formulaZ ∞

f (t)e−st dtF (s) = . . .0

The Laplace transform 3–32

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Patterns

while the details differ, you can see some interesting symmetricbetween

patterns

the time domain (i.e., signals), and

the frequency domain (i.e., their Laplace transforms)

differentiation in one domain corresponds to multiplication by thevariable in the other

multiplication by an exponential in one domain corresponds to a shift(or delay) in the other

we’ll see these patterns (and others) throughout the course

The Laplace transform 3–33