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General form of Faradays Lawb
b aba b a
a
U UV V V E ds
q
! | !
r rg
So the electromotive force around a closed path is:
E ds!I r rgAnd Faradays Law becomes:
BdE ds dt*! ! I r
rgA changing magnetic flux produces an electric field.
This electric field is necessarily non-conservative.
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Eproduced by changing B
dd
dt
*! ! I
rrg l
2d B
E 2 r r dt
T ! Trr
d BrE2 dt
!
r
r
How about outside ro ?
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Problems with Amperes Law
o enclCd I ! Q
rrl
o2 r I! Qr
oI2 rQ!
Tr
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But what if..
o enclCB d I ! Q
rrl
oB 2 r 0T ! Qr
B 0!r
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Maxwells correction to Amperes Law
Q V!
oAd
I! V Ed!
o
o o E
A
Q Ed AEd
I ! ! I ! I *
Eo
dQ dI
dt dt
*! ! I alled displacement current, Id
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Maxwells Equations
Gauss's law electric
0 Gauss's law in magnetism
Faraday's law
Ampere-Maxwell lawI
oS
S
B
Eo o o
qd
d
dd
dt
dd
dt
!
!
* !
* !
E A
B A
E s
B s
The two Gausss laws are symmetrical, apart from the absence of the term formagnetic monopoles in Gausss law for magnetismFaradays law and the Ampere-Maxwell law are symmetrical in that the lineintegrals ofE and B around a closed path are related to the rate of change of
the respective fluxes
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Gausss law (electrical): The total electric flux through any
closed surface equals the net chargeinside that surface divided by Io
This relates an electric field to thecharge distribution that creates it
Gausss law (magnetism): The total magnetic flux through
any closed surface is zero This says the number of field lines
that enter a closed volume mustequal the number that leave that
volume This implies the magnetic fieldlines cannot begin or end at anypoint
Isolated magnetic monopoles havenot been observed in nature
oS
qd
! E A
0S
d !
B A
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Faradays law of Induction: This describes the creation of an electric field by a
changing magnetic flux The law states that the emf, which is the line
integral of the electric field around any closedpath, equals the rate of change of the magnetic fluxthrough any surface bounded by that path
One consequence is the current induced in aconducting loop placed in a time-varying B
The Ampere-Maxwell law is a generalization ofAmperes law
It describes the creation of a magnetic field by anelectric field and electric currents
The line integral of the magnetic field around anyclosed path is the given sum
Bdddt
* ! E s
I Eo o o dd dt* ! B s
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The Lorentz Force Law Once the electric and magnetic fields are known at
some point in space, the force acting on a particle
of charge q can be calculated F =qE +qv x B This relationship is called the Lorentz force law Maxwells equations, together with this force law,
completely describe all classical electromagneticinteractions
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Maxwells Equations in integral form
A Vo o
Q 1E dA dV ! ! VI I
rr
A dA 0
!
rr
Gausss Law
Gausss Law forMagnetism
A
d dE d dA
dt dt
* ! !
r rr rl
Eo encl o o o oA
d dEd I J dA
dt dt
* ! Q Q I ! Q I
rr rr rl
Faradays Law
Amperes Law
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Maxwells Equations in free space(no charge or current)
AE dA 0 !
rr
AdA 0 ! rr
Gausss Law
Gausss Law forMagnetism
A
d d
E d dAdt dt
*
! !
r rr r
lE
o o o o A
d dd E dA
dt dt
* ! Q I ! Q I
r rr rl
Faradays Law
Amperes Law
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Hertzs Experiment An induction coil is connected to a
transmitter The transmitter consists of two spherical
electrodes separated by a narrow gap The discharge between the electrodes
exhibits an oscillatory behavior at a veryhigh frequency
Sparks were induced across the gap of thereceiving electrodes when the frequency ofthe receiver was adjusted to match that ofthe transmitter
In a series of other experiments, Hertz alsoshowed that the radiation generated by thisequipment exhibited wave properties Interference, diffraction, reflection, refraction
and polarization He also measured the speed of the radiation
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Implication A magnetic field will be produced in empty space if thereis a changing electric field. (correction to Ampere)
This magnetic field will be changing. (originally therewas none!)
The changing magnetic field will produce an electric field.(Faraday)
This changes the electric field.
This produces a new magnetic field.
This is a change in the magnetic field.
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An antenna
We have changed the magneticfield near the antenna
Hook up anA source
An electric field results! This isthe start of a radiation field.
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Look at the cross section
E and B are perpendicular (transverse)We say that the waves are polarized.
E and B are in phase (peaks and zeros align)
alled:Electromagnetic Waves
Accelerating
electric charges
give rise to
electromagneticwaves
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Angular Dependence of Intensity
This shows the angulardependence of the radiationintensity produced by a dipole
antenna The intensity and power
radiated are a maximum in aplane that is perpendicular tothe antenna and passingthrough its midpoint
The intensity varies as(sin2 /r2
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Active Figure 34.3
(SLIDESHOW MODE ONLY)
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Harmonic Plane Waves
x
At t=
0
At x = 0
P
P!spatial period orwavelength
88!temporal period
phase velocity
2v
T T 2 k
P T P [! ! P ! !
T
t
r
r
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Applying Faraday to radiation
BdE ddt
* !
rrl
E d E dE y E y dE y ! ( ( ! (rr
lBd dB dx y
dt dt
*! (
dBdE y dx ydt
( ! (
dE dB
dx dt!
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Applying Ampere to radiation
Eo o
dB d
dt
* ! Q I
rrl
B d B z B dB z dB z ! ( ( ! ( rr lEd dE dx z
dt dt
*! (
o odEdB z dx zdt
( ! Q I (
o o
dB dE
dx dt
! Q I
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Fields are functions of bothposition (x) and time (t)
o od ddx dt
! Q I
d d
dx dt!
x t
x x!
x x
o ox tx x! Q Ix x
2
2x x t
x x x! x x x
2
o o 2t x t
x x x
! Q Ix x x
Partial derivatives
are appropriate
2 2
o o2 2
x t
x x! Q I
x x
This is a waveequation!
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The Trial Solution The simplest solution to the partial differential
equations is a sinusoidal wave:
E=Emax cos (kxt)B =Bmax cos (kxt)
The angular wave number is k= 2/ is the wavelength
The angular frequency is = 2 is the wave frequency
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The trial solution
y oE E E sin kx t! ! [2 2
o o2 2
E E
x t
x x! Q I
x x
2
2o2
EE sin kx t
t
x! [ [
x
22
o2
Ek E sin kx t
x
x! [
x
2 2o o o ok E sin kx t E sin kx t [ ! Q I [ [2
2
o o
1
k
[!
Q I
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The speed of light(or any other electromagnetic radiation)
o o
1v c
k
[! ! !
Q I
2v f
T T 2 k
P T P [! ! P ! !
T
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3. The speed of an electromagnetic wave traveling in a transparentnonmagnetic substance is , where is the dielectric constant of the substance.Determine the speed of light in water, which has a dielectric constant at opticalfrequencies of 1.78.
5. Figure 34.3 shows a plane electromagnetic sinusoidal wave propagatingin thex direction. Suppose that the wavelength is 50.0 m, and the electric fieldvibrates in thexyplane with an amplitude of 22.0 V/m. alculate (a) thefrequency of the wave and (b) the magnitude and direction ofB when the electricfield has its maximum value in the negativey direction. (c) Write an expressionforB with the correct unit vector, with numerical values forBmax, k, and , andwith its magnitude in the form
6. Write down expressions for the electric and magnetic fields of asinusoidal plane electromagnetic wave having a frequency of 3.00 GHz andtraveling in the positivex direction. The amplitude of the electric field is 300V/m.
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The electromagnetic spectrum
2v
T T 2 k
P T P [! ! P ! !
T
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Another lookdE dB
dx dt!
y oE E E sin kx t! ! [
o od d
E sin kx t B sin kx tdx dt
[ ! [
o oE k cos kx t B cos kx t [ ! [ [
o
o o o
E 1c
B k
[! ! !
Q I
z oB B B sin kx t! ! [
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Energy in Waves
2 20
0
1 1u E B
2 2! I
Q
o
o o o
E 1c
B k
[! ! !
Q I
20u E! I
2
0
1u B!
Q0
0
u EBI
!Q
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Poynting Vector
Poynting vector points in the direction the wave moves Poynting vector gives the energy passing through a unit
area in 1 sec. Units are Watts/m2
0
1S E B! v
Q
r r r
S cu!r
! ! !2 2
o o o
E cBEBS c
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Intensity The wave intensity, I, is the time average of
S (the Poynting vector) over one or more
cycles When the average is taken, the time average
of cos2(kx - t) = is involved
! ! ! ! !2 2
max max max max
av2 2 2
I aveo o o
E E cS cu
c
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11. How much electromagnetic energy per cubic meter iscontained in sunlight, if the intensity of sunlight at the Earthssurface under a fairly clear sky is 1 000 W/m2?
16. Assuming that the antenna of a 10.0-kW radio stationradiates spherical electromagnetic waves, compute themaximum value of the magnetic field 5.00 km from the
antenna, and compare this value with the surface magneticfield of the Earth.
21. A lightbulb filament has a resistance of 110 . Thebulb is plugged into a standard 120-V (rms) outlet, and emits
1.00% of the electric power delivered to it by electromagneticradiation of frequencyf. Assuming that the bulb is coveredwith a filter that absorbs all other frequencies, find theamplitude of the magnetic field 1.00 m from the bulb.
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Radiation Pressure
Up
c
(( !
F 1 dpP
A A dt! !
ave1 dUP
Ac dt c! !
r
Maxwell showed: (Absorption of radiationby an object)
What if the radiation reflects off an object?
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Pressure and
Momentum
For a perfectly reflecting surface,p = 2U/c and P= 2S/c
For a surface with a reflectivity somewherebetween a perfect reflector and a perfect absorber,the momentum delivered to the surface will besomewhere in between U/c and 2U/c
For direct sunlight, the radiation pressure is about5 x 10-6N/m2
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26. A 100-mW laser beam is reflected back upon itself by amirror. alculate the force on the mirror.
27. A radio wave transmits 25.0 W/m2 of power per unitarea. A flat surface of area Ais perpendicular to the direction of
propagation of the wave. alculate the radiation pressure on it,assuming the surface is a perfect absorber.
29. A 15.0-mW heliumneon laser ( = 632.8 nm) emits a
beam of circular cross section with a diameter of 2.00 mm. (a)Find the maximum electric field in the beam. (b) What totalenergy is contained in a 1.00-m length of the beam? (c) Find themomentum carried by a 1.00-m length of the beam.
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Background for the superior
mathematics student!
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Harmonic Plane Waves
In general, We will only be concerned with the real part ofthe complex phasor representation of a plane wave.
Using Eulers formula:
Re cosT T
E E kx todi b! [
T T TE Ee E kx t i kx t o
i kx t
o! ! [ [ [b g b g b gcos sin
k! 2TP
= propagation number
[TX
!2
= angular frequency
(kx-[t)=
phase
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Phase Velocity - Another View
J [! kx t
ddt
kdxdt
kvJ [ [! ! ! 0
Since the plane waves remain plane waves,
the phase on a plane does not change with time
v
k!
[
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Vector alculus Theorems
T T T T T F dl F d S
C Az zz ! v
A VF dA FdV !
rr r r
And an Important Identity
Gauss Divergence Theorem
Stokes Theorem
T T T T T T v v ! F F F e j e j 2
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Maxwells Equations In Differential Form
T T !D V
T T
!B 0
Gausss Law
Gausss Law forMagnetism
T TT
v ! x
x
EB
tT T T
T
v ! xx
H Jt
Faradays Law
Amperes Law