Ellipsometry
Ellipsometry
Ellipsometry
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(1)<br />
<strong>Ellipsometry</strong><br />
(how to measure the dielectric constant ~<br />
directly and very accurately)<br />
Setup:<br />
ellipt.<br />
pol. light<br />
<br />
E <br />
lin. pol. light<br />
E s<br />
A<br />
nˆ<br />
E p<br />
P<br />
monochromator or<br />
interferometer<br />
analyzer<br />
<br />
detector: measures I ~ E<br />
2<br />
polarizer<br />
light<br />
source<br />
<br />
ip<br />
E E e , E e<br />
p<br />
is<br />
s<br />
<br />
coordinate system defined by plane of incidence of light<br />
2<br />
E <br />
p<br />
tan <br />
2<br />
<br />
i<br />
E <br />
tan e<br />
, : ellipsometric angles<br />
s<br />
<br />
p<br />
<br />
<br />
~<br />
<br />
~<br />
, , <br />
s<br />
1 i 2 <br />
<br />
measure the change of the polarization state of light upon non-normal incidence<br />
reflection on surface of a sample<br />
obtain the complex dielectric function ~<br />
Reflection of polarized light<br />
<br />
ikr i<br />
t<br />
plane wave : E E0e<br />
<br />
k E<br />
B <br />
k<br />
Dispersion relation<br />
n<br />
<br />
k <br />
c<br />
<br />
n<br />
magn. permeability 1 (non-magn. medium)<br />
= dielectric function
z<br />
<br />
k <br />
(2)<br />
'<br />
n,<br />
<br />
n <br />
<br />
''<br />
k <br />
nˆ<br />
<br />
k <br />
boundary condition at z = 0<br />
the same spatial and temporal evolution of the el. field on both sides<br />
equal phase factors<br />
<br />
n <br />
k<br />
r<br />
z<br />
0<br />
k<br />
r<br />
z<br />
0<br />
k<br />
r<br />
z<br />
0<br />
<br />
(projection of k , k and k on x-y plane)<br />
all the wave vectors must lie in the same plane<br />
k sin<br />
ksin<br />
k sin<br />
since k k <br />
and<br />
sin<br />
k<br />
n<br />
<br />
sin<br />
k n<br />
Snell' s law<br />
dynamical aspects from boundary conditions for Maxwell equations<br />
(see previous lectures)<br />
<br />
tang. comp. of E and H are continuous<br />
<br />
normal components of D and B are continuous<br />
<br />
<br />
<br />
<br />
E E<br />
<br />
0 0 <br />
<br />
<br />
E<br />
<br />
0 nˆ<br />
0<br />
<br />
<br />
<br />
<br />
k E0<br />
k E0<br />
k E <br />
0 nˆ<br />
0<br />
<br />
<br />
<br />
<br />
E0<br />
E0<br />
E <br />
0 nˆ<br />
0<br />
<br />
<br />
<br />
<br />
<br />
(1) D<br />
(2) B<br />
k<br />
E0<br />
k E0<br />
<br />
<br />
<br />
<br />
<br />
k E<br />
<br />
0 <br />
nˆ<br />
0 (4) Ht<br />
n<br />
(3) E<br />
t<br />
n<br />
<br />
D E<br />
<br />
B H<br />
n ˆ<br />
<br />
<br />
unit vector,<br />
ˆ1 <br />
nˆ<br />
nˆ<br />
1
(3)<br />
s-component: perpendicular (senkrecht) to plane of incidence<br />
B<br />
<br />
<br />
E<br />
'<br />
n<br />
n<br />
B <br />
<br />
E <br />
<br />
nˆ<br />
’'<br />
<br />
E <br />
<br />
B <br />
<br />
E<br />
s<br />
nˆ<br />
(1),(2) are satisfied<br />
(3) E E <br />
E<br />
<br />
0<br />
s s s<br />
<br />
<br />
(4) n E E <br />
cos<br />
nE<br />
<br />
cos0<br />
s s s<br />
with ncos n cos n n sin n<br />
n<br />
sin<br />
2 2 2 2 2 2 2 2<br />
<br />
Snell's law<br />
<br />
Es<br />
2n<br />
cos<br />
<br />
E<br />
2 2 2<br />
s n cos<br />
n<br />
n<br />
sin <br />
<br />
2 2 2<br />
E n cos<br />
n<br />
n<br />
sin <br />
s<br />
<br />
E<br />
2 2 2<br />
s n cos<br />
n<br />
n<br />
sin <br />
Fresnel equations for s -pol. light
(4)<br />
p-component: parallel to plane of incidence<br />
<br />
E <br />
p<br />
<br />
<br />
B<br />
‘<br />
n<br />
n<br />
E <br />
p<br />
<br />
B <br />
’'<br />
nˆ<br />
<br />
B <br />
<br />
<br />
E p<br />
(1)<br />
(2)<br />
cos<br />
E p E<br />
<br />
p <br />
cos<br />
E<br />
<br />
n E p E p nE<br />
<br />
<br />
<br />
<br />
<br />
p 0<br />
<br />
p<br />
<br />
0<br />
(E<br />
t<br />
)<br />
(B )<br />
t<br />
E<br />
E<br />
<br />
p<br />
p<br />
<br />
n<br />
2<br />
2n<br />
ncos<br />
cos<br />
n<br />
n<br />
2<br />
n<br />
2<br />
sin<br />
E<br />
E<br />
<br />
p<br />
p<br />
n<br />
<br />
n<br />
2<br />
2<br />
cos<br />
n<br />
cos<br />
n<br />
n<br />
n<br />
2<br />
2<br />
n<br />
n<br />
2<br />
2<br />
sin<br />
sin<br />
2<br />
2<br />
<br />
<br />
Fresnel equations for<br />
p -pol. light
(5)<br />
Brewster-angle:<br />
2 2 2<br />
for ncos<br />
<br />
B<br />
n n n<br />
sin B<br />
0<br />
n<br />
Ep<br />
0<br />
at this angle the refl. wave has no p-component<br />
purely s-polarized one can make so - called Brewster -polarizers)<br />
n<br />
<br />
B<br />
arctan <br />
n <br />
n 1.5 (glass) B<br />
56.3<br />
n<br />
the larger n the closer is to 90<br />
B<br />
total internal reflection:<br />
n<br />
sin<br />
for n n<br />
<br />
n sin<br />
<br />
90<br />
if<br />
<br />
<br />
<br />
B<br />
n<br />
<br />
arcsin<br />
<br />
n <br />
refracted wave propagates along the interface<br />
no energy transport across interface; total internal reflection.
(6)<br />
Glas / amb.<br />
r s , r p 1<br />
n 1.5<br />
n<br />
~ r<br />
s,<br />
p<br />
r<br />
s,<br />
p<br />
e<br />
i s,<br />
p<br />
Es<br />
rs<br />
<br />
E<br />
s<br />
r s<br />
r<br />
p<br />
<br />
E<br />
E<br />
p<br />
p<br />
r p<br />
0<br />
45° 90°<br />
B<br />
<br />
s<br />
p<br />
reflected wave<br />
0<br />
Reflectance<br />
1<br />
E <br />
R <br />
2<br />
2<br />
E<br />
R s<br />
R s<br />
R P
define complex reflection coeff.<br />
2 2 2<br />
rp<br />
n sin tan n<br />
n<br />
sin <br />
<br />
<br />
r 2 2 2<br />
s n sin tan n<br />
n<br />
sin <br />
(7)<br />
take<br />
n 1, n<br />
2<br />
2<br />
2 1<br />
<br />
2 2<br />
<br />
sin tan sin<br />
<br />
1<br />
<br />
<br />
It is important to note that <br />
and <br />
are complex quantities<br />
<br />
i<br />
1 2<br />
Rp<br />
e<br />
<br />
1i<br />
2<br />
<br />
R e<br />
Rp<br />
i( ps)<br />
e<br />
<br />
R<br />
s<br />
s<br />
i<br />
p<br />
i<br />
s<br />
relative attenuation<br />
relative phase shift<br />
R<br />
R<br />
<br />
p<br />
s<br />
p<br />
tan <br />
<br />
s<br />
<br />
and <br />
ellipsometric angles<br />
<br />
<br />
1<br />
2<br />
sin<br />
<br />
~<br />
<br />
<br />
2<br />
<br />
<br />
<br />
2cos<br />
<br />
,<br />
<br />
<br />
2<br />
2<br />
2<br />
cos 2<br />
sin 2sin<br />
<br />
1<br />
2<br />
1<br />
sin2cos<br />
2<br />
2 2<br />
2sin<br />
2sin<br />
sin tan <br />
2<br />
1<br />
sin2cos<br />
<br />
, <br />
<br />
tan<br />
2<br />
<br />
<br />
<br />
How do we measure and :<br />
ellipt.<br />
pol. light<br />
<br />
E<br />
E p<br />
E s<br />
P<br />
FTIR<br />
nˆ<br />
A<br />
analyzer<br />
Ee<br />
E <br />
Ee<br />
i<br />
p<br />
p<br />
i<br />
s<br />
s
(8)<br />
We want to know<br />
I<br />
E<br />
2<br />
det<br />
as a function of<br />
A and P<br />
det ~ <br />
Jones matrix formalism :<br />
Polarizer<br />
1 0 <br />
change of coordinate system<br />
cos<br />
P sin P 1 0 cos<br />
P sin P <br />
<br />
<br />
<br />
0 0<br />
sin<br />
P cos P<br />
0 0<br />
sin P cos P<br />
sample<br />
r<br />
~<br />
p 0<br />
<br />
0<br />
~ rs<br />
<br />
cos<br />
A sin A1 0 cos<br />
A sin A<br />
r<br />
~<br />
p 0<br />
cos<br />
P sin P 1 0 cos<br />
P sin P <br />
E <br />
<br />
<br />
det<br />
<br />
<br />
<br />
sin<br />
A cos A<br />
<br />
0 0<br />
<br />
sin<br />
A cos A<br />
<br />
0<br />
r~<br />
s<br />
sin<br />
P cos P<br />
<br />
0 0<br />
<br />
<br />
sin P cos P<br />
<br />
analyzer<br />
sample<br />
polarizer<br />
<br />
E<br />
det<br />
<br />
<br />
~ r<br />
<br />
<br />
p<br />
cos P cos A ~ rs<br />
sin P sin A Ex<br />
<br />
<br />
0<br />
<br />
<br />
<br />
I<br />
det<br />
~<br />
~ 1<br />
E<br />
2<br />
det<br />
~ 2 2 2<br />
cos P sin P<br />
~ 2 2 2<br />
cos P sin P<br />
<br />
<br />
<br />
<br />
cos 2A<br />
<br />
<br />
Re<br />
~ sin2P<br />
~ 2 2 2<br />
cos P sin P<br />
<br />
<br />
<br />
<br />
sin 2A<br />
<br />
I<br />
I 0<br />
modulation of intensity as a function of<br />
Analyzer angle get , as second<br />
Fourier coefficient<br />
<br />
~<br />
tan cos<br />
i sin<br />
~ 2 2<br />
tan ;<br />
Re<br />
tan<br />
<br />
tan<br />
cos<br />
2<br />
2<br />
2<br />
cos<br />
2<br />
2<br />
<br />
<br />
~<br />
<br />
cos P sin P<br />
P<br />
P sin<br />
2<br />
2<br />
tan cos <br />
P<br />
2 2<br />
1tan<br />
sin P1<br />
<br />
<br />
<br />
2·A<br />
<br />
1<br />
tan <br />
1<br />
tan P<br />
analogous :<br />
cos <br />
<br />
1<br />
2
(9)<br />
modulation of I<br />
det<br />
A <br />
, tan<br />
,cos<br />
. Only cos is measured, not .<br />
<br />
<br />
2nd Fourier<br />
coefficients<br />
ambiguity with respect to shift by can be determined with retarder unit, i.e.<br />
introduce in addition to the sample a unit which leads to a known plane shift.<br />
Examples for applications<br />
1. Au + Semiconductors critical points in band structure<br />
2. Oxidation of a semiconductor surface thin film characterization<br />
3. Electrochemistry and biological systems. Radiation damage in solids<br />
4. High-T c -Superconductors