Wave Phenomena
Physics 15c
Lecture 11 Fourier Analysis
(H&L Sections 13.1–4) (Georgi Chapter 10)
Wave Phenomena Physics 15c Lecture 11 Fourier Analysis (H&L - - PowerPoint PPT Presentation
Wave Phenomena Physics 15c Lecture 11 Fourier Analysis (H&L Sections 13.14) (Georgi Chapter 10) What We Did Last Time Studied reflection of mechanical waves Similar to reflection of electromagnetic waves = F Zv
Lecture 11 Fourier Analysis
(H&L Sections 13.1–4) (Georgi Chapter 10)
Studied reflection of mechanical waves
Similar to reflection of electromagnetic waves Mechanical impedance is defined by
For transverse/longitudinal waves: Useful in analyzing reflection
Studied standing waves
Created by reflecting sinusoidal waves Oscillation pattern has nodes and antinodes Musical instruments use standing waves to produce their
distinct sound Z T F Zv ± = [ or ]
l
K ρ =
Define Fourier integral
Fourier series is defined for repetitive functions
Discreet values of frequencies contribute
Extend the definition to include non-repetitive functions
Sum becomes an integral
Discuss pulses and wave packets
Sending information using waves Signal speed and bandwidth Connection with Quantum Mechanics
( )
1
( ) cos sin
n n n n n
f t a a t b t ω ω
∞ =
= + +
In Lecture #5, we solved the wave equation
Normal-mode solutions Using Fourier series, we can make any arbitrary waveform
with linear combination of the normal modes
Example: forward-going repetitive waves
Non-repetitive waves also OK if we make T ∞
This makes ω continuous
2 2 2 2 2
( , ) ( , )
w
x t c x t t x ξ ξ ∂ ∂ = ∂ ∂
( )
( , )
i kx t
x t e
ω
ξ ξ
±
=
w
c k ω =
( )
1
( , ) ( ) cos( ) sin( )
w n n n n n n n
x t f x c t a k x t b k x t ξ ω ω
∞ =
= − = − + −
2
n
n T π ω =
n w n
k c ω =
A little math work needed
For repetitive function f(t)
Express cosωnt and sinωnt with complex exponentials
( )
1
( ) cos sin
n n n n n
f t a a t b t ω ω
∞ =
= + +
=
T
dt t f T a ) ( 1 2 ( )cos
T n n
a f t tdt T ω = ∫ 2 ( )sin
T n n
b f t tdt T ω = ∫ 2
n
n T π ω =
( )
1 1 1 1
cos sin 2 2 2 2
n n m n
i t i t n n n n n n n n n n i t i t m m n n m n
a ib a ib a t b t e e a ib a ib e e
ω ω ω ω
ω ω
∞ ∞ − = = − ∞ − − =−∞ =
− + + = + + + = +
m n
ω ω = −
m n
b b = −
m n
a a = m n = −
Define and How do we calculate Fn? It’s useful later if I shift the integration range here Now we take it to the continuous limit…
( )
n
i t n n
f t F e
ω ∞ − =−∞
= ∑ 1 ( )
T
F f t dt T = ∫ 1 2 2 1 ( )cos ( )sin ( ) 2
n
T T T i t n n n
F f t tdt i f t tdt f t e d T T T
ω
ω ω = + =
2
n n n
a ib F + = F a =
same
2 2
1 ( )
n
T i t n T
F f t e dt T
ω −
= ∫
OK because f(t) is repetitive Sum includes n = 0
t
Make T ∞
F(ω) is the Fourier integral of f(t)
2
n
n T π ω = ( )
n
i t n n
f t F e
ω ∞ − =−∞
= ∑
2 2
1 ( )
n
T i t n T
F f t e dt T
ω −
= ∫ ( ) lim lim lim 2 ( )
n
i t in t n n T T n n i t n T i t
F f t F e e T F e d F e d
ω ω ω ω
ω ω ω π ω ω
∞ ∞ − − ∆ →∞ →∞ =−∞ =−∞ ∞ − −∞ →∞ ∞ − −∞
= = ∆ ∆ = =
2 T π ω ∆ ≡ 1 ( ) lim ( ) 2 2
i t n T
T F F f t e dt
ω
ω π π
∞ −∞ →∞
≡ =
( ) ( )
i t
f t F e d
ω
ω ω
∞ − −∞
= ∫ 1 ( ) ( ) 2
i t
F f t e dt
ω
ω π
∞ −∞
=
Fourier integral F(ω) is
A decomposition of f(t) into different frequencies An alternative, complete representation of f(t)
One can convert f(t) into F(ω) and vice versa
f(t) is in the time domain F(ω) is in the frequency domain
( ) ( )
i t
f t F e d
ω
ω ω
∞ − −∞
= ∫ 1 ( ) ( ) 2
i t
F f t e dt
ω
ω π
∞ −∞
=
F(ω) and f(t) are two equally-good representations
Different conventions exist in Fourier integrals
( ) ( )
i t
f t F e d
ω
ω ω
∞ − −∞
= ∫ 1 ( ) ( ) 2
i t
f t F e d
ω
ω ω π
∞ − −∞
=
1 ( ) ( ) 2
i t
F f t e dt
ω
ω π
∞ −∞
=
( ) ( )
i t
F f t e dt
ω
ω
∞ −∞
= ∫
and and
1 ( ) ( ) 2
i t
f t F e d
ω
ω ω π
∞ − −∞
=
and
1 ( ) ( ) 2
i t
F f t e dt
ω
ω π
∞ −∞
=
Consider a short pulse with unit area
F(ω) is a bunch of little ripples
around ω = 0
Height is 1/2π Area is 1/T
T 1 T
1 2 2
( )
T T T
t f t t < = >
2 2
1 1 1 ( ) ( ) sin 2 2 2
T i t i t T
T F f t e dt e dt T T
ω ω
ω ω π π πω
∞ −∞ −
= = =
Fourier
ω 2 T π 1 (0) 2 F π =
Pulse of duration T
The shorter the pulse, the wider the F(ω) (width in t) × (width in ω) = 2π = const
This is a general feature of Fourier transformation
Example: Gaussian function
1 ( ) sin 2 T F T ω ω πω =
“width” 2
T π
2 2
2
1 ( ) 2
t T
f t e T π
−
=
2 2
2
1 ( ) 2
T
F e
ω
ω π
−
= T 1 T
Consider sending information using waves
Voice in the air Voice converted into EM signals on a phone cable Video signals through a TV cable
You can’t do it with pure sine waves cos(kx – ωt)
It just goes on Completely predictable No information You need waves that change patterns with time
What you really need are pulses
Pulse width T determines the speed
Pulses must be separated by at least T
Audio signals range from 20 to 20 kHz
Too low for efficient radio transmission Use a better frequency and modulate amplitude
Modulated waves are no longer pure sine waves
What is the frequency composition?
Carrier wave Audio signal Amplitude-modulated waves
Consider carrier waves modulated by a pulse
This makes a short train of waves
A wave packet
T = 1/(20 kHz) for audio signals
Fourier integral is
T ( ) f t
2 2
( )
i t T T
e t f t t
ω −
< = >
2 2
( ) 1 1 ( ) sin 2 ( ) 2
T i t i t T
T F e e dt
ω ω
ω ω ω π π ω ω
− −
− = = −
Similar to the square pulse
Width is 2π/T Centered at ω = ω0 This is called the bandwidth of your radio station This limits how close the frequencies of radio stations can be
You need 20 kHz for HiFi audio
It’s more like 5 kHz in commercial AM stations
( ) 1 ( ) sin ( ) 2 T F ω ω ω π ω ω − = − ω ω 2 T π To send pulses every T second, your signal must have a minimum spread of 2π/T in ω, which corresponds to 1/T in frequency
Speed of information transfer = # of pulses / second
Determined by the pulse width in the time domain Translated into bandwidth in the frequency domain We say “bandwidth” to mean “speed of communication”
“Broadband” means “fast communication”
Each medium has its maximum bandwidth
You can split it into smaller bandwidth “channels”
Radio wave frequencies Regulated by the government Cable TV 750 MHz / 6 MHz = 125 channels
You want to minimize the bandwidth of each channel
Telephones carry only between 400 and 3400 Hz
Take the square pulse again
Make it narrower by T → 0 The height grows 1/T → ∞
We get an infinitely narrow pulse with unit area
Dirac’s delta function δ(t) For any function f(t)
T 1 T ( ) t t t δ ∞ = = ≠ ( ) 1 t dt δ
∞ −∞
=
( ) ( ) (0) f t t dt f δ
∞ −∞
=
( ) ( ) ( ) f t t t dt f t δ
∞ −∞
− =
and
What is the Fourier integral of δ(t)?
δ(t) contains all frequencies equally
1 1 ( ) ( ) 2 2
i t
F t e dt
ω
ω δ π π
∞ −∞
= =
You can get this also by making T 0 in
1 ( ) sin 2 T F T ω ω πω =
1 ( ) 2
i t
t e d
ω
δ ω π
∞ − −∞
=
Another way of defining δ(t)
Consider pure sine waves with angular frequency ω0
( )
i t
f t e
ω −
=
( )
1 1 ( ) ( ) 2 2
i t i t i t
F e e dt e dt
ω ω ω ω
ω δ ω ω π π
∞ ∞ − − −∞ −∞
= = = −
t ω ω ( ) f t ( ) F ω
T infinite t width 1/T infinite ω width F(ω) f(t) Finite pulse and everything else uniform δ(t) δ pulse δ(ω0 – ω) uniform Sinusoidal ω domain t domain Waveform
Pure sine waves and δ pulses are the two extreme
cases of all waves
Everything falls in between Widths in t and ω are inversely proportional to each other
Wait… Did I prove it?
Now we consider a signal with an arbitrary shape
Let’s define the average time and the average frequency
Because (energy density) ∝ (amplitude)2
Now we define the r.m.s. widths in t and ω
( ) f t ( ) F ω
Fourier
2 2
( ) ( ) t f t dt t f t dt
∞ −∞ ∞ −∞
= ∫
2 2
( ) ( ) F d F d ω ω ω ω ω ω
∞ −∞ ∞ −∞
= ∫
( )
( )
2 2
t t t ∆ = −
( )
( )
2 2
ω ω ω ∆ = −
r.m.s. = root mean square
( )
( ) ( )
2 2 2 2 2
( ) ( ) t t f t dt t t t f t dt
∞ −∞ ∞ −∞
− ∆ = − = ∫
( )
( ) ( )
2 2 2 2 2
( ) ( ) F d F d ω ω ω ω ω ω ω ω ω
∞ −∞ ∞ −∞
− ∆ = − = ∫
What can we do with this mess??
We can express F(ω) with f(t) as
2 * ( ) 2 * 2
1 ( ) ( ) ( ) 4 1 ( ) ( ) ( ) 2 1 ( ) 2
i t s
F d f t f s e d dtds f t f s t s dtds f t dt
ω
ω ω ω π δ π π
∞ ∞ ∞ ∞ − −∞ −∞ −∞ −∞ ∞ ∞ −∞ −∞ ∞ −∞
= = − =
∫ ∫ ∫ ∫ ∫ ∫ ∫
1 2
( ) ( )
i t
F f t e dt
ω π
ω
∞ −∞
=
Next we take
We can use this to construct
( ) ( )
i t
f t F e d
ω
ω ω
∞ − −∞
= ∫
Differentiate with t
[ ]
( ) ( )
i t
d f t i F e d dt
ω
ω ω ω
∞ − −∞
= − ∫
[ ]
( ) ( )
i t
d F e d i f t dt
ω
ω ω ω
∞ − −∞
=
( ) ( ) ( )
( )
( ) ( )
2 2 * ( ) * 2
( ) ( ) ( ) 1 ( ) ( ) 2 1 ( ) 2
i t
F d F F d d F F e d d d d i f t dt dt
ω ω
ω ω ω ω ω ω ω ω ω ω δ ω ω ω ω ω ω ω ω ω ω ω ω π ω π
∞ ∞ ∞ −∞ −∞ −∞ ∞ ∞ ∞ − − −∞ −∞ −∞ ∞ −∞
′ ′ ′ ′ ′ − = − − − ′ ′ ′ ′ = − − = −
∫ ∫ ∫ ∫ ∫ ∫ ∫
t
Now we have
Here comes the trick: we calculate the integral
It’s a positive number divided by a positive number κ is a real number
( )
( )
2 2 2
( ) ( ) t t f t dt t f t dt
∞ −∞ ∞ −∞
− ∆ = ∫
( )
2 2 2
( ) ( ) d i f t dt dt f t dt ω ω
∞ −∞ ∞ −∞
− ∆ = ∫
( )
2 2
( ) ( ) d t t i i f t dt dt I f t dt κ ω κ
∞ −∞ ∞ −∞
− − − = >
The integral in the denominator becomes Integrate the first term in parts
( ) ( )
* *
( ) ( ) ( ) ( ) d d t t f t f t f t t t f t dt dt dt κ
∞ −∞
− + −
( ) ( )
2 * *
( ) ( ) ( ) ( ) ( ) d d t t f t t t f t f t f t t t f t d dt dt
∞ ∞ −∞ −∞
− + − − + −
= 0 because the pulse has a finite extent
( )
2 * *
( ) ( ) ( ) ( ) ( ) d d tf t f t f t tf t dt f t dt dt dt κ κ
∞ ∞ −∞ −∞
− + = −
( ) ( ) ( )
( ) ( )
* * 2 2 2 2
( ) ( ) ( ) ( ) ( ) d d t t f t i i f t i i f t t t f t dt dt dt I t f t dt κ ω κ ω κ κ ω
∞ −∞ ∞ −∞
− − − + − − − = ∆ + ∆ + ∫
∫
( )
t κ κ
We’ve come a long way
Now we got If a quadratic function of κ is always positive,
( ) ( ) ( )
2 2 2
I t κ κ ω κ = ∆ + ∆ − >
( ) ( )
2 2
1 4 D t ω = − ∆ ∆ < 1 2 t ω ∆ ∆ >
finally!
For any signal, the product of the r.m.s. widths ∆t and ∆ω in the time and frequency domain is greater than 1/2
We have studied Fourier transformation in time t and
frequency ω
We can also do it in space x and wavenumber k Everything works the same way In particular, for any signal traveling in space
Why is it important?
( ) ( )
ikx
f x F k e dk
∞ − −∞
= ∫ 1 ( ) ( ) 2
ikx
F k f x e dx π
∞ −∞
=
1 2 x k ∆ ∆ >
In Quantum Mechanics, particles are wave packets
Unlike a classical particle, wave packet has a length The position cannot be determined more accurately than ∆x
Momentum is related to the wavenumber by
This means
p k = h 2 h π = h
Planck’s constant = 6.63 × 10−34 J s
2 x p x k ∆ ∆ = ∆ ∆ > h h Heisenberg’s Uncertainty Principle
Defined Fourier integral
f(t) and F(ω) represent a function in time/frequency domains
Analyzed pulses and wave packets
Time resolution ∆t and bandwidth ∆ω related by
Proved for arbitrary waveform
Rate of information transmission ∝ bandwidth Dirac’s δ(t) a limiting case of infinitely fast pulse Connection with Heisenberg’s Uncertainty Principle in QM
( ) ( )
i t
f t F e d
ω
ω ω
∞ − −∞
= ∫ 1 ( ) ( ) 2
i t
F f t e dt
ω
ω π
∞ −∞
=
1 2 t ω ∆ ∆ >