chapter 4: wave equations

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

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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 Presentation

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Page 1: Chapter 4:  Wave equations

Chapter 4: Wave equations

Features of today’s lecture:55 slides10 meters of rope1 song

(condensed version)

Page 2: Chapter 4:  Wave equations
Page 3: Chapter 4:  Wave equations

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

Page 4: Chapter 4:  Wave equations

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

Page 5: Chapter 4:  Wave equations

let’s make some waves

Page 6: Chapter 4:  Wave equations

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

Page 7: Chapter 4:  Wave equations

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

Page 8: Chapter 4:  Wave equations

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)(

Page 9: Chapter 4:  Wave equations

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:

Page 10: Chapter 4:  Wave equations

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

Page 11: Chapter 4:  Wave equations

A = amplitude

0 = initial phase angle (or absolute phase) at x = 0 and t =0

Absolute phase

y = A sin[k(x ± vt) + 0]

Page 12: Chapter 4:  Wave equations

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

Page 13: Chapter 4:  Wave equations

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

Page 14: Chapter 4:  Wave equations

works for any periodic waveany ??

Page 15: Chapter 4:  Wave equations
Page 16: Chapter 4:  Wave equations

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

Page 17: Chapter 4:  Wave equations

“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

Page 18: Chapter 4:  Wave equations

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.

Page 19: Chapter 4:  Wave equations

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.

Page 20: Chapter 4:  Wave equations

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

Page 21: Chapter 4:  Wave equations

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

Page 22: Chapter 4:  Wave equations

Spherical waves

• harmonic waves emanating from a point source• wavefronts travel at equal rates in all directions

tkrier

Page 23: Chapter 4:  Wave equations

Cylindrical waves

tkieA

Ψ

Page 24: Chapter 4:  Wave equations

the wave nature of light

Page 25: Chapter 4:  Wave equations

Electromagnetic waves

Page 26: Chapter 4:  Wave equations

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:

Page 27: Chapter 4:  Wave equations

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:

Page 28: Chapter 4:  Wave equations

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

Page 29: Chapter 4:  Wave equations

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

Page 30: Chapter 4:  Wave equations

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

Page 31: Chapter 4:  Wave equations

x

z

y

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

Page 32: Chapter 4:  Wave equations

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

Page 33: Chapter 4:  Wave equations

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

Page 34: Chapter 4:  Wave equations

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

Page 35: Chapter 4:  Wave equations

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

Page 36: Chapter 4:  Wave equations

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

Page 37: Chapter 4:  Wave equations

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

Page 38: Chapter 4:  Wave equations

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:

Page 39: Chapter 4:  Wave equations

Polarization

• corresponds to direction of the electric field• determines of force exerted by EM wave on

charged particles (Lorentz force)• linear,circular, eliptical

Page 40: Chapter 4:  Wave equations

Evolution of electric field vector

linear polarization

Page 41: Chapter 4:  Wave equations

Evolution of electric field vector

circular polarization

Page 42: Chapter 4:  Wave equations

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