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Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
John David Jackson
Dai-Sik Kim
Nano Optics Lab.
School of Physics and Astronomy
Seoul National University
Classical Electrodynamics I
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
Perfect conductor case
xtkzEE ˆ)(cos0
ytkzBB ˆ)(cos0
After normal incidence reflection:
tkzxEtkztkzxEE sinsinˆ2)](cos)([cosˆ00
tkzyBB coscosˆ2 0
22 k
Perfect conductor
x
y
z
E
B
k
0
8. Waveguides, Resonant Cavities, and Optical Fibers Day 21
못들어옴
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
Boundary condition for the perfect conductor
0// E KHn
ˆ
K
: Surface current
cf) previous lecture: Quasi-Static Magnetic Fields in Conductors (section 5.18),
z
etz
yHH
)(cosˆ0
z
etz
yHE
)4
(cos2
2ˆ
0
phase difference.
For the perfect conductor case,
0)(ˆ cEEn
0)(ˆ cBBn
Where cc BE
, are the fields inside the conductor.
8. Waveguides, Resonant Cavities, and Optical Fibers Day 21
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
BiE
EiB
0 B
0 E 022
B
E
Because of the cylindrical geometry it is useful to single out the spatial variation of
the fields in the z direction and to assume
tiikzeyxEtzyxE ),(),,,(
tiikzeyxBtzyxB ),(),,,(
In general,22 k
8.2 Cylindrical Cavities and Waveguides
8. Waveguides, Resonant Cavities, and Optical Fibers Day 21
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
Assuming propagation in the positive z direction and the nonvanishing of at
least one of Ez and Bz , the transverse fields are
ztztt BzEkk
iE
ˆ
)( 22
ztztt EzBkk
iB
ˆ
)( 22
pf) Suppose that the z dependence is given by
0)( 222
B
Ekt
2
222
zt
tiikzeyxEtzyxE ),(),,,(
tiikzeyxBtzyxB ),(),,,(
8. Waveguides, Resonant Cavities, and Optical Fibers Day 21
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
It is useful to separate the fields into components parallel to and transverse
to the z axis:
tz EEE
where
zz EzE ˆ
zEzEtˆ)ˆ(
The Maxwell equation can be written out in terms of transverse and parallel
components as
BiE
EiB
0 B
0 E
zttt EBzi
z
E
ˆ
zttt BEzi
z
B
ˆ
ztt BiEz
ˆ
ztt EiBz
ˆ
z
EE z
tt
z
BB z
tt
8. Waveguides, Resonant Cavities, and Optical Fibers Day 21
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
BiE
양변 x z tBziBziEz
ˆˆ)(ˆ
?)(ˆ Ez
)()()()()( abbaabbaba
)(ˆ,ˆ Ezz
EEEbzaLet z
tt
ztz Bziz
EE
z
EEEzTherefore
ˆ)(ˆ,
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
It is evident from the previous equations that if Ez and Bz are known the
transverse components of E and B are determined.
zttt EBzi
z
E
ˆtiikzeyxEtzyxE ),(),,,(
zttt EBziEik
ˆ
zttt BEziz
B
ˆzttt BEziBik
ˆ
zttztt EEziBik
ziEik
ˆ1
ˆ
tztt EziBik
B
ˆ1
tiikzeyxBtzyxB ),(),,,(
- ①
- ②
From ②
With ①,
8. Waveguides, Resonant Cavities, and Optical Fibers Day 21
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
The result, after some simplifications, is
ztztt BzEkk
iE
ˆ
)( 22
ztztt EzBkk
iB
ˆ
)( 22
ztztt Bzk
E
kiik
E
ˆ1
2
Likewise,
ztztt Bzk
Ek
iikE
ˆ
2
8. Waveguides, Resonant Cavities, and Optical Fibers Day 21
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
x
y
z
E
B
)(cosˆ0 tkzxEE
)(cosˆ0 tkzyBB
22 k
Ex) TEM mode
02 tE
02 tB
This means that ETEM is a solution of an electrostatic problem in two dimensions.
It is necessary to have two or more cylindrical surfaces to support the TEM mode.
An important property of the TEM mode is the absence of a cutoff frequency.
8. Waveguides, Resonant Cavities, and Optical Fibers Day 21
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
Transverse Magnetic (TM) waves
0zB everywhere; boundary condition, 0SzE
Transverse Electric (TE) waves
0zE everywhere; boundary condition: 0
S
z
n
Bn: surface normal
)( 22 k
EikE zt
t
)(
ˆ22 k
EziB zt
t
)(
ˆ22 k
BziE zt
t
)( 22 k
BikB zt
t
8. Waveguides, Resonant Cavities, and Optical Fibers Day 21
0
S
z
x
BCan be deduced from Ey =0 on y=0
surface plus Bn =0, in--------------------- zttt BEzi
z
B
ˆ
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
ztztt BzEkk
iE
ˆ
)( 22
ztztt EzBkk
iB
ˆ
)( 22
It is found from
that the transverse magnetic and electric fields for both TM and TE waves are
related by
tt EzZ
H ˆ1
8. Waveguides, Resonant Cavities, and Optical Fibers Day 21
8.3 Waveguides
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
TM waves
)( 22 k
EikE zt
t
)( 22 k
BikH zt
t
TE waves
)(
)(
0
0
TEk
k
k
TMk
kk
Z
Where Z is called the wave impedance and is given by
8. Waveguides, Resonant Cavities, and Optical Fibers Day 21
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
0)( 22
2
2
2
2
zHk
yx
TE mode
0)( 222
B
Ekt
0
S
z
n
Hat x=0, a and y=0, b
b
yn
a
xmHyxH z
coscos~),( 0
8. Waveguides, Resonant Cavities, and Optical Fibers Day 21
8.4 Modes in a Rectangular Waveguide
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
If a>b, the lowest cutoff frequency, that of the dominant TE mode, occurs for
m=1, n=0:
a
0,1
22
22
2
mnmnb
n
a
mk
Cutoff frequency
2/122
b
n
a
mmn
8. Waveguides, Resonant Cavities, and Optical Fibers Day 21
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
This corresponds to half of a free-space wavelength across the guide. The
explicit fields for this mode are
tiikz
z ea
xHH
cos0
tiikz
x ea
xH
ikaH
sin0
tiikz
y ea
xH
aiE
sin0
8. Waveguides, Resonant Cavities, and Optical Fibers Day 21
22
22
2
mnmnb
n
a
mk
ztztt BzEkk
iE
ˆ
)( 22
ztztt EzBkk
iB
ˆ
)( 22
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
We note that, for mn ,the wave number is real: waves of the mode can propagate in the guide.
For frequencies less than the cutoff frequency , the wave number is imaginary;
such modes cannot propagate and are called cutoff modes or evanescent modes.
n
c
kv
mnmn
p
1
1
1
2
2
Note that
Vp : phase velocity n: refractive index
8. Waveguides, Resonant Cavities, and Optical Fibers Day 21
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
pv
gvv
gpvvv 2
dkkd )2()2(
n
cvk
dk
dv mnmn
mn
g
11
12
2
vg : group velocity
8. Waveguides, Resonant Cavities, and Optical Fibers Day 21
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
Hollow cylinder case
TM
0zE 0)( 222 zt Ek
0)(1 22
2
2
2
2
k
d
d
d
dm
Solution: Bessel function
0)(1 22
2
2
2
2
k
d
d
d
dm
im
z eE )(~),(
Rz
8. Waveguides, Resonant Cavities, and Optical Fibers Day 21
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
222 k
0)(1
2
22
2
2
m
d
d
d
d
Assume m=0,
tiikz
z eJEE )(00
Boundary Condition 0)( rEz
...)654.8
(),520.5
(),405.2
(,0 000 R
JR
JR
Jm
.....654.8520.5405.2
030201RRR
8. Waveguides, Resonant Cavities, and Optical Fibers Day 21
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
tiikz
z eR
JEE )405.2
(00
tiikzeR
JHH )405.2
(ˆ10
Take the lowest zero,
1405.21,0
R
Cut off frequency
2
22 405.2
Rk
Dispersion relation
8. Waveguides, Resonant Cavities, and Optical Fibers Day 21
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
Because of reflections at the end surfaces, the z dependence of the fields is that
appropriate to standing waves:
zkBzkA cossin
end surfaces
z
0 d
The boundary conditions can be satisfied at each surface only if
...),2,1,0( pd
pk
8. Waveguides, Resonant Cavities, and Optical Fibers Day 21
8.7 Resonance Cavities
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
For TM fields the vanishing of Et at z=0 and z=d requires
...),2,1,0(cos),(
p
d
zpyxEz
8. Waveguides, Resonant Cavities, and Optical Fibers Day 21
From the cylinder waveguide result,
...),2,1,0(cos)(0
p
d
zp
R
xJeEE mn
m
im
z
mnxWhere are the n-th roots of 0)( xJm
2
22
2
21
d
p
R
xmnmnp
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
The lowest TM mode has m=0, n=1, p=0
R
405.2010
ti
z eR
JEE )405.2
(00
tieR
JEiH
)405.2
(10
8. Waveguides, Resonant Cavities, and Optical Fibers Day 21
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
earth
ionosphere
요사이의공명은아마도빛이지구를7바퀴반도는것과관련!?;
7.5 Hz?
http://sedonanomalies.weebly.com/schumann-resonance.html
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
이건조은데...; air index of refraction과관계된문제를내봐?
n_air=1.00029; cf) n_water=1.33
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
Eikonal equation
nn ||
Assume
t
BE
t
DH
)(x
0)();()(
ExDxx
EE
0))()(
()(2
2
22 x
x
EExn
cE
Slowly varying
8. Waveguides, Resonant Cavities, and Optical Fibers Day 21
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
0)(2
2
22 Exn
cE
0)(2
2
22
xn
c
If n is constant, xkn
ci
e
ˆ
For slowly varying n, )(xS
ci
e
Substitution gives,
0)( 22
2
2
Sc
iSSxnc
SSxn
)(2
)(ˆ)()( xkxnxS
)(ˆ xk
is a unit vector in the direction of )(xS
8. Waveguides, Resonant Cavities, and Optical Fibers Day 21
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
The form of is that of a plane wave with wave vector, ).(ˆ xk
)()( xSds
rdrn
ds
rdk
ˆ
ds
dSxS
ds
d
ds
rdrn
ds
d
)()(
But ,ˆ
kds
dso that )()(ˆˆ rnrnkk
ds
dS
Finally, we obtain
r
Cnrn
ds
rdrn
ds
d
4);()( 원운동
8. Waveguides, Resonant Cavities, and Optical Fibers Day 21
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim
Seoul National University Classical Electrodynamics I
Department of Physics & Astronomy Dai-Sik Kim