1. Chapter 4: Wave equations
(condensed version)
Chapter 4: Wave equations
Features of today’s lecture:
55 slides
10 meters of rope
1 song

3. 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

4. Waves move A wave is… a disturbance in a medium
f(x) t0
t1 > t0
t2 > t1
t3 > t2 v x
A wave is…
a disturbance in a medium
-propagating in space with velocity v
-transporting energy
-leaving the medium undisturbed

5. let’s make some waves

6. 1D traveling wave f(x) v x 0 1 2 3
t1 > t0
t2 > t1
t3 > t2 v x
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.

7. works for anything that moves!
The wave equation
Let y = f (x'), where x' = x ± vt So and
Now, use the chain rule:
So Þ and Þ   
Combine to get the 1D differential wave equation:
works for anything that moves!

8. 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)

9. Snapshots of harmonic waves
at a fixed time:
at a fixed point: T A A
propagation constant: k = 2p/l
wave number: k = 1/l
frequency: n = 1/T
angular frequency: w = 2pn
n ≠ v
v = velocity (m/s)
n = frequency (1/s)
v = nl
Note:

10. The phase of a harmonic wave
The phase, j, is everything inside the sine or cosine (the argument).
y = A sin[k(x ± vt)]
j = k(x ± vt)
For constant phase, dj = 0 = k(dx ± vdt)
which confirms that v is the wave velocity.

11. Absolute phase y = A sin[k(x ± vt) + j0] A = amplitude
j0 = initial phase angle (or absolute phase) at x = 0 and t =0
y = A sin[k(x ± vt) + j0] p

12. How fast is the wave traveling?
The phase velocity is the wavelength/period: v = l/T
Since n = 1/T:
In terms of k, k = 2p/l, and
the angular frequency, w = 2p/T, this is:
v = ln
v = w/k

13. Phase velocity vs. Group velocity
Here, phase velocity = group velocity (the medium is non-dispersive).
In a dispersive medium, the phase velocity ≠ group velocity.

14. works for any periodic wave??

16. Complex numbers make it less complex!
P = (x,y)
x: real and y: imaginary
P = x + i y
= A cos(j) + i A sin(j)
where

17. “one of the most remarkable formulas in mathematics”
Euler’s formula
“one of the most remarkable formulas in mathematics”
Links the trigonometric functions and the complex exponential function
eij = cosj + i sinj
so the point, P = A cos(j) + i A sin(j), can also be written:
P = A exp(ij) = A eiφ
where
A = Amplitude
j = Phase

18. Harmonic waves as complex functions
Using Euler’s formula, we can describe the wave as
y = Aei(kx-wt)
so that y = Re(y) = A cos(kx – wt)
y = Im(y) = A sin(kx – wt) ~ ~ ~
Why?
Math is easier with exponential functions than with trigonometry.

19. Plane waves
A plane wave’s contours of maximum field, called wavefronts, are planes. They extend over all space.
The wavefronts of a wave sweep along at the speed of light.
equally spaced
separated by one wavelength apart
perpendicular to direction or propagation
Usually we just draw lines; it’s easier.

20. represents direction of propagation
Wave vector k
represents direction of propagation
Y = A sin(kx – wt)
Consider a snapshot in time, say t = 0:
Y = A sin(kx)
Y = A sin(kr cosq)
If we turn the propagation constant (k = 2p/l) into a vector, kr cosq = k · r
Y = A sin(k · r – wt)
wave disturbance defined by r
propagation along the x axis

21. General case Y = Aei(k·r - wt) k · r = xkx = yky + zkz = kr cosq  ks
arbitrary direction
In complex form:
Y = Aei(k·r - wt)
Substituting the Laplacian operator:

22. Spherical waves harmonic waves emanating from a point source
wavefronts travel at equal rates in all directions

23. Cylindrical waves

24. the wave nature of light

25. Electromagnetic waves

26. Derivation of the wave equation from Maxwell’s equations

27. E and B are perpendicular
Perpendicular to the direction of propagation:
I. Gauss’ law (in vacuum, no charges): so
II. No monopoles:
Always! so
Always!

28. E and B are perpendicular
Perpendicular to each other:
III. Faraday’s law: so
Always!

29. E and B are harmonic Also, at any specified point in time and space,
where c is the velocity of the propagating wave,

30. The 1D wave equation for light waves
where E is the light electric field
We’ll use cosine- and sine-wave solutions:
where:
E(x,t) = B cos[k(x ± vt)] + C sin[k(x ± vt)]
kx ± (kv)t
E(x,t) = B cos(kx ± wt) + C sin(kx ± wt)
The speed of light in vacuum, usually called “c”, is 3 x 1010 cm/s.

31. EM wave propagation in homogeneous media
The speed of an EM wave in free space is given by:
0 = permittivity of free space, 0 = 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)

32. Simple case— plane wave with E field along x, moving along z:y

33. General case— along any direction
which has the solution:
where
and

34. Arbitrary direction
= wave vector x
Plane of constant , constant E z y

35. Electromagnetic waves transmit energy
Energy density (J/m3) in an electrostatic field:
Energy density (J/m3) in an magnetostatic field:
Energy density (J/m3) in an electromagnetic wave is equally divided:

36. Rate of energy transport
Rate of energy transport: Power (W) A
cDt
Power per unit area (W/m2):
Poynting
Pointing vector

37. Poynting vector oscillates rapidly
Take the time average:
“Irradiance” (W/m2)

38. Light is a vector field
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.

39. Light is a 3D vector field
A light wave has both electric and magnetic 3D vector fields:
A 3D vector field assigns a 3D vector (i.e., an arrow having both direction and length) to each point in 3D space.

40. Polarization corresponds to direction of the electric field
determines of force exerted by EM wave on charged particles (Lorentz force)
linear,circular, eliptical

41. Evolution of electric field vector
linear polarization

42. Evolution of electric field vector
circular polarization

43. Exercises
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