chapter 4: wave equations
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(condensed version). Chapter 4: Wave equations. Features of today’s lecture: 55slides 10 meters of rope 1song. This idea has guided my research: - PowerPoint PPT PresentationTRANSCRIPT
Chapter 4: Wave equations
Features of today’s lecture:55 slides10 meters of rope1 song
(condensed version)
This idea has guided my research: for matter, just as much as for radiation, in particular light, we must introduce at one and the same time the corpuscle concept and wave concept.
Louis de Broglie
0 1 2 3
Waves move
t0 t1 > t0 t2 > t1 t3 > t2
x
f(x)
v
A wave is…a disturbance in a medium
-propagating in space with velocity v-transporting energy -leaving the medium undisturbed
let’s make some waves
To displace f(x) to the right: x x-a, where a >0.
Let a = vt, where v is velocity and t is time-displacement increases with time, and-pulse maintains its shape.
So x' = f(x -vt) represents a rightward, or forward, propagating wave.x' = f(x+vt) represents a leftward, or backward, propagating
wave.
0 1 2 3
t0 t1 > t0 t2 > t1 t3 > t2
x
f(x)
v
1D traveling wave
The wave equation
works for anything that moves!
Let y = f (x'), where x' = x ± vt. So and
Now, use the chain rule:
So and
Combine to get the 1D differential wave equation:
2
2
22
2 1
t
y
vx
y
1
x
xv
t
x
x
x
x
f
x
y
t
x
x
f
t
y
x
f
x
y
2
2
2
2
x
f
x
y
x
fv
t
y
2
22
2
2
x
fv
t
y
Harmonic waves
• periodic (smooth patterns that repeat endlessly)•generated by undamped oscillators undergoing harmonic motion
• characterized by sine or cosine functions -for example,
-complete set (linear combination of sine or cosine functions can represent any periodic waveform)
vtxkAvtxfy sin)(
Snapshots of harmonic waves
T
A
at a fixed time: at a fixed point:
A
frequency: = 1/T angular frequency: = 2
propagation constant: k = 2/wave number: = 1/
≠ v v = velocity (m/s) = frequency (1/s)
v =
Note:
The phase, , is everything inside the sine or cosine (the argument).
y = A sin[k(x ± vt)]
= k(x ± vt)
For constant phase, d = 0 = k(dx ± vdt)
which confirms that v is the wave velocity.
vdt
dx
The phase of a harmonic wave
A = amplitude
0 = initial phase angle (or absolute phase) at x = 0 and t =0
Absolute phase
y = A sin[k(x ± vt) + 0]
How fast is the wave traveling?
The phase velocity is the wavelength/period: v = /T
Since = 1/T:
In terms of k, k = 2/, and the angular frequency, = 2/T, this is:
v = v =
v = /k v = /k
Phase velocity vs. Group velocity
Here, phase velocity = group velocity (the medium is non-dispersive).
In a dispersive medium, the phase velocity ≠ group velocity.
kvphase
dk
dvgroup
works for any periodic waveany ??
Complex numbers make it less complex!
x: real and y: imaginary
P = x + i y = A cos() + i A sin()
where
P = (x,y)
1i
“one of the most remarkable formulas in mathematics”Euler’s formula
Links the trigonometric functions and the complex exponential function
ei = cos + i sin
so the point, P = A cos() + i A sin(), can also be written:
P = A exp(i) = A eiφ
where
A = Amplitude
= Phase
Harmonic waves as complex functions
Using Euler’s formula, we can describe the wave as
y = Aei(kx-t)
so that y = Re(y) = A cos(kx – t)
y = Im(y) = A sin(kx – t)
~
~
~
Why? Math is easier with exponential functions than with trigonometry.
Plane waves
• equally spaced• separated by one wavelength apart• perpendicular to direction or propagation
The wavefronts of a wave sweep along
at the speed of light.
A plane wave’s contours of maximum field, called wavefronts, are planes. They extend over all space.
Usually we just draw lines; it’s easier.
Wave vector krepresents direction of propagation
= A sin(kx – t)
Consider a snapshot in time, say t = 0:
= A sin(kx)
= A sin(kr cos)
If we turn the propagation constant (k = 2/into a vector, kr cos = k · r
= A sin(k · r – t)
• wave disturbance defined by r• propagation along the x axis
arbitrary direction
General case
k · r = xkx = yky + zkz
kr cosks
In complex form:
= Aei(k·r - t)
2
2
22
2
2
2
2
2 1
t
Ψ
vz
Ψ
y
Ψ
x
Ψ
Substituting the Laplacian operator:
2
2
22 1
t
Ψ
vΨ
Spherical waves
• harmonic waves emanating from a point source• wavefronts travel at equal rates in all directions
tkrier
AΨ
Cylindrical waves
tkieA
Ψ
the wave nature of light
Electromagnetic waves
http://www.youtube.com/watch?v=YLlvGh6aEIs
Derivation of the wave equation from Maxwell’s equations
0
0
BE E
t
EB B
t
Derivation:
I. Gauss’ law (in vacuum, no charges):
so
II. No monopoles:
so
Always!
Always!
E and B are perpendicular
0),( 0 trkjeEtr E
00 ωtrkjeEkj
00 Ek
0),( 0 trkjeBtr B
00 ωtrkjeBkj
00 Bk
k
E
k
B
Perpendicular to the direction of propagation:
III. Faraday’s law:
so
Always!
t
B
E
t
eE trkj
B
0
it
BieEjkEjk xtrkj
oyzozyˆˆ
oxoyzozy B
EkEk
EB
Perpendicular to each other:
E and B are perpendicular
E and B are harmonic
)sin(
)sin(
0
0
t
t
rkBB
rkEE
Also, at any specified point in time and space,
cBE where c is the velocity of the propagating wave,
m/s 10998.21 8
00
c
The speed of an EM wave in free space is given by:
0= permittivity of free space, = magnetic permeability of free space
To describe EM wave propagation in other media, two properties of the medium are important, its electric permittivity ε and magnetic permeability μ. These are also complex parameters.
= 0(1+ ) + i = complex permittivity
= electric conductivity = electric susceptibility (to polarization under the influence of an external field)
Note that ε and μ also depend on frequency (ω)
kc
00
1
EM wave propagation in homogeneous media
x
z
y
Simple case— plane wave with E field along x, moving along z:
which has the solution:
where
and
andx y zk r k x k y k z
, ,x y zk k k k
, ,r x y z
General case— along any direction
2
2
22 1
tc
E
E
]exp[),,,( 0 titzyx rkEE
),,( 0000 zyx EEEE
z
y
x
Arbitrary direction
constzkykxk zyx
k
= wave vectork
0E
r
tiet rkErE
0),(
k Plane of constant , constant E rk
rk
ttzyx rkEE
sin),,,( 0
Energy density (J/m3) in an electrostatic field:
Energy density (J/m3) in an magnetostatic field:
2
02
1BuB
Energy density (J/m3) in an electromagnetic wave is equally divided:
2120 0
BEuuu BEtotal
Electromagnetic waves transmit energy
202
1 EuE
2
02
1BuB
Rate of energy transport: Power (W)
ct
A
Power per unit area (W/m2):
Pointing vector
Poynting
Rate of energy transport
ucS
EBcS 20
BES
20c
t
tuAc
t
Vu
t
energyP
ucAP
k
Take the time average:
“Irradiance” (W/m2)
Poynting vector oscillates rapidly
tEE cos0 tBB cos0
tBEcS 200
20 cos
tBEcS 200
20 cos
002
021 BEcS
eES
A 2D vector field assigns a 2D vector (i.e., an arrow of unit length having a unique direction) to each point in the 2D map.
Light is a vector field
Light is a 3D vector field
A 3D vector field assigns a 3D vector (i.e., an arrow having both direction and length) to each point in 3D space.
A light wave has both electric and magnetic 3D vector fields:
Polarization
• corresponds to direction of the electric field• determines of force exerted by EM wave on
charged particles (Lorentz force)• linear,circular, eliptical
Evolution of electric field vector
linear polarization
Evolution of electric field vector
circular polarization
You are encouraged to solve all problems in the textbook (Pedrotti3).
The following may be covered in the werkcollege on 8 September 2010:
Chapter 4:3, 5, 7, 13, 14, 17, 18, 24
Exercises