Upload
hedia
View
76
Download
5
Embed Size (px)
DESCRIPTION
- PowerPoint PPT Presentation
Citation preview
I have decided on a change in the grading policy. I did not want to take up class time with extra quizzes so we only had 4 of the planned 6-7 quizzes. I feel that having 10% of the grade based on just 4 (really 2 since I drop the 2 lowest) quiz grades is too much. Therefore the homework will count for 30% of the grade instead of 25% and the quizzes will only count for 5%
I will be skipping Chapters 30 and 31 so that I may cover electromagnetic waves and optics as these will be covered on the MCAT. In Chapters 32 -34, I will be focusing only on those topics covered in the MCAT.
I have put some practice problems on line.
I will not be here next week. The last lecture will be given by Professor Rasmussen. However, you may email me with questions.
The final is Dec 13 at 2 PM. Remember that it will be 40% comprehensive and 60% on material covered since the last exam. You will be allowed two 8 ½ X 11 sheets of paper for notes (both sides) and it is open book.
Your grades will be available by Dec 16. You may email me or come by my office in WSTC if you want to know your grade on your final. I leave Dec 18, so you must contact me by Dec 16 if you want to talk about your grade.
I will have a review session in FN 2.212 the day before the final starting at noon and going until ????. You need to have studied for the exam prior to the session for it to do any good as you need to know what you don’t understand so I can review it.
Eddy Currents
When magnetic field is on, currents (eddy currents) are induced in conductors so that the pendulum slows down or stops
Displacement Current
0 enclB dl I 0
0 0( ) EA
q C Ed EAd
0E
cddq
idt dt
0 displacement currentEd
di
dt
tcc
Ej
Bj
B0
2
0
2
1
20
0 c
“displacement current” of the electric field
flux as opposed to conduction
current
!fields! magnetic gcirculatin torise give
toofields electric changingbut currentsonly Not
:tiongeneraliza sMaxwell'
esconsequenc reaching-farwith
result ain gculminatin theory ofy consistenc theof
analysis oreticalpurely the a of examplegreat a is
equations Maxwell theof one tion togeneraliza Its
currentssteady -non toapplied once
orycontradict becomes
:currents varying-for time Law sAmpere' of Inadequacy
000
0
tId
Id
E
sB
sB
The Reality of Displacement Current
D ci i
2
0 2
02
0
2
inside the capacitor2
outside capacitor2
D
c
c
rB dl rB i
Rr
B iR
B ir
Field in the region outside of the capacitor existsas if the wire were continuous within the capacitor
0
2 20
1
0
t
tc c
E
BE
j EB
B
0
0 0
0
S
c
S
Qd
dl dt
dl I dt
B d
E A
E B A
B E A
A
Maxwell equations in all their consistency and beauty
differential form integral form
12
00 c
Gauss’s Law for E
Gauss’s Law for B
Ampere’s Law
Faraday’s Law
How are these equivalent?
Special cases of the more general Stokes' theorem
The Divergence theorem relates the flow (flux) of a vector field through a surface to the behavior of the vector field inside the surface.
More precisely: the outward flux of a vector field through a closed surface is equal to the volume integral of the divergence of the region inside the surface.
the sum of all sources minus the sum of all sinks gives the net flow out of a region.
€
(∇ ⋅F)dV = F ⋅ndSS
∫V
∫
The left side is a volume integral over the volume V, the right side is the surface integral over the boundary of the volume V.
The Curl Theorem relates the surface integral of the curl of a vector field over a surface S to the line integral of the vector field over its boundary,
Use Divergence and Curl Theorems
The left side is a surface integral and the right side is a line integral
€
(∇ × F) ⋅dA = F ⋅ds∫S
∫
€
E ⋅dA =Qenc
ε0S
∫
€
Q = ρdVV
∫
E ⋅dA =S
∫ ρ
ε0
dVV
∫
€
E⋅ dAS
∫ = E⋅ndSS
∫ = (∇⋅E)dVV
∫
€
(∇ ⋅E)dVV
∫ =ρ
ε0
dVV
∫
€
∇⋅E =ρ
ε0
Equivalence of integral and differential forms of Gauss’s law for electric fields
If is the charge density (C/m3), the total charge in a volume is the integral over that volume of
But from the divergence theorem:
It is often written as
€
∇⋅D = ρ where D=ε0E
Q j
0
: with timechanges inside charge the
surface, closed rough thecurrent th theof Because
onconservati Charge
j
jnj
t
dVdAdVt
It
Q
Something very fundamental
!!! 01
1
0)(
:yconsistenc restoreson modificati sMaxwell'
?? t
s Where'- 1
0)(
:onconservati chargewith
nt inconsiste be wouldlaw sAmpere'Just
00
0
2
0
2
tt
tc
c
jEj
EjB
jB
0
E
So the next (?) time you see a shirt that looks like this:
You will know what it means!
0
0 0 0
0
t
t
E
BE
EB j
B
0
0 0
0
S
c
S
Qd
dl dt
dl I dt
B d
E A
E B A
B E A
A
Maxwell equations and electromagnetic waves
differential form integral form
12
00 c
Gauss’s Law for E
Gauss’s Law for B
Ampere’s Law
Faraday’s Law
Electromagnetic disturbances in free space
With a complete set of Maxwell equations, a remarkable new phenomenon occurs:
Fields can leave the sources and travel alone through space.
The bundle of electric and magnetic fields maintains itself:
If B were to disappear, this would produce E;
if E tries to go away, this would create B.
So they propagate onward in space.
0
0
2
B
EB
BE
E
tc
t
No charges and no currents!
Generating Electromagnetic Radiation
Heinrich Hertz was the first person to produceelectromagnetic waves intentionally in the lab
Oscillating charges in the LC circuit were sources of electromagnetic waves
Marconi – first radio communication.Radio transmitter- electric charges oscillate along the antennae
and produce EM waves. Radio receiver – incoming EM waves inducecharge oscillations and those are detected
Plane EM waves
A simple plane EM wave
Wavefront – boundary plane between the regions with and without EM disturbance
We will first show that such a planeEM wave satisfies Maxwell equations
First, we will see if it satisfies Gauss’s laws for E and B fields
Consider Faraday’s Law
Bddl
dt
E
Circulation of vector E around loop efgh equals to -Ea
dl Ea
E
Rate of change of flux through the surfacebounded by efgh is d=(Ba)(cdt)
BdBac
dt
Hence –Ea=-Bac, and
E cB
Now consider Ampere’s Law
0 0Ed
dldt
B
Circulation of vector B around loop efgh equals to Ba
B dl Ba
Rate of change of flux through the surfacebounded by efgh is d=(Ea)(cdt)
EdEac
dt
0 0B cE
0 0
1c
299,792,458 /c m s
Key Properties of EM Waves
The EM wave in vacuum is transverse; both E and B are perpendicular to the direction of propagation of the wave, and to each other.
Direction of propagation and fields are related by
There is definite ratio between E and B; E=cB
The wave travels in vacuum with definite and unchanging speed c
Unlike mechanical waves, which need oscillating particles of a medium to transmit a disturbance, EM waves require no medium.
k E B
Plane waves
wavestransverse -n propagatio of
direction thelar toperpendicu are fields The
:fields dependent)-( dynamicfor 0
10
0
0
0
),( ),,(
:direction-in only
spacein change that fields varying)-(time
dynamicin interested now be wouldWe
2
tBE
t
E
cz
B
y
B
t
B
z
E
y
E
x
B
x
E
z
E
y
E
x
E
txtx
x
xx
xyz
xyz
x
xzyx
B
E
BBEE
0
0
2
B
EB
BE
E
tc
t
EM Wave Equation
0
0
2
B
EB
BE
E
tc
t
t
E
cx
B
x
B
z
B
BBt
t
B
x
E
y
E
x
Et
B
x
E
z
E
EE
BEtxtx
yzzx
zyxy
yzx
zy
xx
2
yz
1
other!each lar toperpendicu are and
0 ,0 dependent)-( Dynamic
0
0
0 ,0 choose usLet
0 ),,( ),,(
BE
BBEE
Plane waves
01
:for same theand
01
:for equation wave thederive we
1
1
equations twoCombining
2
2
22
2
2
2
22
2
2
2
t
B
cx
B
Bt
E
cx
E
Et
E
tc
x
B
tt
B
xx
E
x
t
E
cx
B
t
B
x
E
zz
z
yy
y
y
zzy
yz
zy
sinusoidal waves
General (one-dimensional) wave equation
01
)( ),(
)( ),(
2
2
22
2
22
2
2
2
t
y
vx
y
vtxfvt
yvtxfv
t
y
vtxfx
yvtxf
x
y
direction- negative in the propagates
direction- positive in the propagates
functions) arbitrary are and (
)()(
: wavesgpropagatin are solutions General
npropagatio wave theof speed theis
motion) wavestring in thent displaceme (e.g.
function wave theis Here
direction- along
npropagatio wavegeneral a describes
01
2
2
22
2
xg
xf
gf
ctxgvtxfy
v
y
x
t
y
vx
y
waveneticelectromagan isLight
in vacuumlight of speed theis This
m/s1031
speedwith
wavesEM ofn propagatio thedescribe
01
01
equationsour So
8
00
2
2
22
2
2
2
22
2
c
t
B
cx
B
t
E
cx
E
zz
yy