physics 2112 lecture 23 electricity & magnetism lecture 23, slide 1
TRANSCRIPT
Physics 2112Lecture 23
Electricity & Magnetism Lecture 23, Slide 1
First…..two comments
E&M waves like sounds waves (in many ways)
So I’m going to say “Recall from Physics 2111….” a lot
Slide 2
The animations in the pre-lectures are really nice for this topic.
There are just some things that are tough to draw on the board.
Creating an Electromagnetic Wave
Slide 3
E
Dipole Antenna
Signal Generator
What does this Create?
Electric Field changing in magnitude and direction
with time and spaceEx = Eo sin (kx – wt)
Key Point!!!
Slide 4
Not just single sine wave!
Same value of E
z
Plane wave!
Ampere’s Law / Faraday’s Law
Slide 5
dAdt
dEldB oo
dAdt
dBldE
Ampere’s Law – Changing Electric Field causes Magnetic Field
Faraday’s Law – Changing Magnetic Field causes Electric Field
Ex = Eo sin (kx – wt) By = Bo sin (kx – wt)
t
B
x
E
Eo k cos (kx – wt) = Bo w cos (kx – wt)
Eo/Bo = /w k = wave velocity
Eo = c Bo = B/(moeo)1/2 for wave only
Plane Waves from Last Time
E and B are perpendicular and in phase
Oscillate in time and space
Direction of propagation given by E X B
E0 = cB0
Argument of sin/cos gives direction of propagation
Electricity & Magnetism Lecture 23, Slide 6
Ex
By
Not Really
Slide 7
The Electromagnetic Spectrum
Clickers: f =24Ghz l ~ 12.5cm
Recall from 2111:v = fl = c
Waves Carry Energy
Electricity & Magnetism Lecture 23, Slide 8
Recall: Energy Density for E field = uE = ½ eo E2
Energy Density for B field = uB = ½ 1/mo B2
Average Total Energy Density = <u> = ½ (uE + uB) = EB/cmo
Recall from 2111:Intensity = Power/Area = Average Energy hitting a surface per unit time
Intensity = <u> c = EB/mo
Define:Poynting Vector
o
BES
Example 23.1: Sunshine Poynting Vector
Slide 9
Sunlight puts an average of1000 Joules of energy every second into each square meter of the earth around the equator.
What is the magnitude of the average Poynting vector for this light?
a) |Savg| = 1000 Watts/m2
b) |Savg| = 1000/ Watts/m2
c) |Savg| = 1000 Watts/m2
22
What is Emax and Bmax for these E&M waves?
Just another way to keep track of all this:Its magnitude is equal to IIts direction is the direction of propagation of the wave
Comment on Poynting Vector
Electricity & Magnetism Lecture 23, Slide 10
td
dp
m
p
td
dE
2
2
Light has Momentum!
Electricity & Magnetism Lecture 23, Slide 11
If it has energy and its moving, then it also has momentum:
Analogy from mechanics:
td
dp
m
mv
pressureA
F
c
I
m
pE
2
2
vF
IAtd
dU
td
dEFor E - M waves:
cFIA
cv
Radiation pressure
c
IP
Example 23.2: Pressure from Sunshine
Slide 12
Sunlight puts an average of 1000 Joules of energy every second into each square meter of the earth around the equator.
What is the pressure this sunlight puts on the earth assuming it is all absorbed?
What is the total force exerted on the earth by this sunlight?
What is the pressure of this sunlight if it reflected back?
Doppler Shift
The Big IdeaAs source approaches:Wavelength decreasesFrequency Increases
Electricity & Magnetism Lecture 23, Slide 13
Recall for sound from 2111:
If source is moving wrt to air:)/1/( soundsso vvff
If observer is moving wrt to air: )/1( soundoso vvff
)/1(
)/1(
sounds
soundoso vv
vvff
If observer is moving wrt to air:
What’s Different from Sound or Water Waves ?
Sound /Water Waves : You can calculate (no relativity needed)
BUTResult is somewhat complicated: is source or observer moving wrt medium?
Electromagnetic Waves : You need relativity (time dilation) to calculate
BUTResult is simple: only depends on relative motion of source & observer
b > 0 if source & observer are approaching
b < 0 if source & observer are separating
b = v/c
Doppler Shift for E-M Waves
Electricity & Magnetism Lecture 23, Slide 14
2
1
1
1'
ff
v
or f’f
v
ff’
Doppler Shift for E-M Waves
Electricity & Magnetism Lecture 23, Slide 15
The Doppler Shift is the SAME for both cases! f ’/f only depends on the relative velocity
2
1
1
1'
ff
A Note on Approximations
why?
Doppler Shift for E-M Waves
Electricity & Magnetism Lecture 23, Slide 16
2
1
1
1'
ff if b <<< 1 1' ff
Taylor Series: Expand around b = 0 2
1
1
1
F
2
!2
)0(
!1
)0(')0( FF
FF
Evaluate:1)0( F
1)0( F 1)(F
NOTE:2/1)1()( F
2
11)( F
A police k-band radar gun emits radio waves at a frequency of 24GHz which is reflected off an approaching car and received back at the gun.
Which car will provide a higher reflected frequency?a) A car approaching at 67 mphb) A car approaching at 69mphc) Both will provide the same
Electricity & Magnetism Lecture 23, Slide 17
Example 23.3: Police Radar
What are the reflected frequencies for these two speeds?
Our Sun Star in a distant galaxy
wav
elen
gth
Wavelengths appear shifted higher lengths
Red Shift
Frequencies appear shifted lower(c = lf)
Star separating from us(Expanding Universe)
Electricity & Magnetism Lecture 23, Slide 18
Light from distant stars
Red Shift (the whole story!)
Electricity & Magnetism Lecture 23, Slide 19
Two additional effects can cause frequency shifts from distant stars.
Gravity - Extreme case is a black hole. You can think of a black hole a “redshifting” light until l = infinity and f = 0 Expanding Universe - Can take so long to reach Earth that universe expanded during flight, stretching the wavelength
Exact mixture depends – How long was wave in flight, how large was object emitting the wave and how fast was it moving wrt Earth.
We believe the energy in an e-m wave is carried by photons
Question: What are Photons?Answer: Photons are Photons.
Photons possess both wave and particle propertiesParticle:
Energy and Momentum localized Wave:
They have definite frequency & wavelength ( fl = c)
Question: How can something be both a particle and a wave?Answer: It can’t (when we observe it)What we see depends on how we choose to measure it!The mystery of quantum mechanics: More on this in PHYS 2115 (one cool class!)
h = 6.63e-34 J - s Planck’s constant
Connections seen in equations:E = hfp = h/l
Photons
Electricity & Magnetism Lecture 23, Slide 20