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Light is an electromagnetic wave. We
have an electrical field that oscillates with some frequency (around
1015 Hz as you should now know by heart). If it impinges on a
dielectric material (= no free electrons), it will jiggle the charges inside
(bound electrons) around a bit. We looked at this in detail in
chapter 3.
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An electrical field caused some polarization of the dielectric material. This lead
straight to the dielectric constant
er. |
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| Attention! |
The word "polarization" above and in chater 3
has nothing to do with the
"polarization" of light! |
Attention! |
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Since the word "light" is synonymous to
"oscillating electrical field", it is no surprise that er is linked to the index of refraction n =
er½. |
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For oscillating electrical fields we needed to
look at the frequency dependence of the
polarization and that lead straight to the complex
dielectric
function er(w) = e'(w) + ie''(w) instead of the simple dielectric constant
er. Go back to
chapter
3.3.2 if you don't quite recall all of this. |
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The dielectric function, after some
getting used to, made life much easier and provided for new insights not easily
obtainable otherwise. In particular, it encompassed the "ideal"
dielectric losses and losses resulting from
non-ideality. i.e. from a finite conductivity in its imaginary part. |
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So it's logical to do exactly the
same thing for the index of refraction. We replace n by a
complex index of refraction
n* defined as |
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We don't use n' and n'' as symbols
for the real and imaginary part but denote the real part by the (old) symbol
n and the imaginary part by k.
This is simply to keep up with tradition and has no special meaning. |
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We use the old relation between the index of
refraction and the dielectric constant but now write it as |
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With n = n(w); k = k(w), since e' and e'' are
frequency dependent as discussed before. |
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Re-arranging for n
and k yields somewhat unwieldy
equations: |
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| n2 |
= |
1
2 |
æ
ç
è |
æ
è |
e' 2 + e'' 2 |
ö
ø |
½ |
+ e' |
ö
÷
ø |
| k2 |
= |
1
2 |
æ
ç
è |
æ
è |
e' 2 + e'' 2 |
ö
ø |
½ |
e' |
ö
÷
ø |
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Anyway - That is all. Together with the
Fresnel equations we now have a lot of
optics covered. Example of a real
complex indexes of
refraction are shown in the link. |
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So lets see how this works, and what k, the so far unspecified imaginary part of
n*, will give us. |
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First, lets get some easier formula.
In order to do this,
we remember
that e'' was connected to the
"dielectric" and static (ohmic) conductivity of the material and
express e'' in terms of the (total)
conductivity sDK as |
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Note that in contrast to the definition of e''
given before in
the context of the dielectric function, we have an e0 in the e'' part. We had, for the sake of simplicity,
made a
convention that the e in the dielectric
function contain the e0, but here
it is more convenient to write it out, because then e' = e0 ·
er is reduced to er and directly relates to the
"simple" index of refraction n |
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Using that in the expression (n + ik)2 gives |
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| (n + ik)2 |
= |
n2 k2 + i
· 2nk |
= e' + i
· |
sDK
e0 · w |
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We have a complex number on both sides of the
equality sign, and this demands that the real and imaginary parts must be the
same on both sides, i.e. |
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| n2 k2 |
= |
e' |
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| nk |
= |
sDK
2e0w |
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Separating n and k finally gives |
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| n2 |
= |
1
2 |
æ
ç
è |
e' |
+ |
æ
è |
e' 2 + |
sDK2
4e02w2 |
ö
ø |
½ |
ö
÷
ø |
| k2 |
= |
1
2 |
æ
ç
è |
e' |
+ |
æ
è |
e' 2 + |
sDK2
4e02w2 |
ö
ø |
½ |
ö
÷
ø |
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Similar to what we had above,
but now with basic quantities like the "relative dielectric constant"
since e' = er
and the total conductivity sDK.
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Now lets look at the physical meaning of n and k, i.e. the real and complex part of the complex index
of refraction, by looking at an electromagnetic wave traveling through a medium
with such an index. |
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For that we simply use the general formula for the electrical
field strength E of an electromagnetic wave traveling in a medium
with refractive index n*. For simplicities sake, we do it
one-dimensional in the x-direction (and use the index
"x" only in the first equation). In the most general terms we
have |
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| Ex |
= E0, x · exp i ·
(kx · x w · t) |
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With kx = component of
the wave vector in x-direction = k = 2p/l, w = circular frequency = 2pn. |
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There is no index of refraction in the formulas
but you know (I hope) what to do. |
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You must introduce the velocity v of the
electromagnetic wave in the material and use the relation between frequency,
wavelength, and velocity to get rid of k or l, respectively. In other words, we use |
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Of course, c is the speed of light in
vacuum. Insertion yields |
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| Ex |
= |
E0, x · exp i · |
æ
ç
è |
w · n*
c |
· x w
· t |
ö
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ø |
= |
E0, x · exp i · |
æ
ç
è |
w · (n + i ·
k)
c |
· x w ·
t |
ö
÷
ø |
| Ex |
= |
E0, x · exp · |
æ
ç
è |
i · w · n
· x
c |
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w · k ·
x
c |
i · w ·
t |
ö
÷
ø |
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The red expression is nothing but
the wavevector, so we get a rather simple result: |
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| Ex |
= |
exp |
w ·
k · x
c |
· exp[ i ·
(kx · x w · t)] |
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Decreasing
amplitude |
Plane wave |
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Spelt out: if we use a complex index of
refraction, the propagation of electromagnetic waves in a material is whatever
it would be for an ideal material with only a real index of refraction times a attenuation
factor that decreases the amplitude exponentially as a function of
depth x. |
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Obviously, at a depth often called
absorption length or
penetration depth W = c/w · k, the intensity
decreased by a factor 1/e. |
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The imaginary part k of the complex index of refraction thus describes
rather directly the attenuation of electromagnetic waves in the material
considered. It is known as damping
constant, attenuation
index, extinction
coefficient, or (rather misleading) absorption
constant. Misleading, because an absorption constant is usually the
a in some exponential decay law of the form
I = I0 · exp a · x or what we called W = c/w · k above. |
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Note: Words like "constant",
"index", or "coefficient" are also misleading - because
k is not constant, but depends on the
frequency just as much as the real and imaginary part of the dielectric
function. |
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The equations above go beyond just describing the
optical properties of (perfect) dielectrics because we can include all kinds of
conduction mechanisms into s, and all kinds
of dielectric polarization mechanisms into e'. |
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We can even use these equations for things like the
reflectivity of metals, as we shall see. |
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Keeping in mind that typical n's in
the visible region are somewhere between 1.5 - 2.5 (n
» 2.5 for diamond is one of the highest
values as your girl friend knows), we can draw a few quick conclusions: From
the simple but coupled equations for n and k follows: |
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For sDK = 0 (and,
as we would assume as a matter of course, er > 0 (but possibly < 1?)) we
obtain immediately n = (er)½ and k = 0 - the old-fashioned simple relation between just
er and n. Remember
that sDK = 0 applies only if
- the static conductivity sstat
is close to zero, and
- we have frequencies where e''
» 0, i.e well outside the
resonance
"peak" for optical frequencies.
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Generally, we would like k to be
rather small for "common" optical materials! |
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We also expect k to be rather small for "common" optical
materials, because optical materials are commonly insulators, i.e. so at least
sstatic » 0 applies. |
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Let's look at some numbers now. With
w »
1016 Hz and c = 3 · 1010
cm/s, we have a penetration depth W » 3 · 106/k. |
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If, for example, the penetration depth should be
in excess of 1 km (for optical communication, say), k < 3 · 1011 is needed. It
should be clear that this is quite a tough requirement on the material. How
does it translates into requiremetns for sDK or e''? |
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If we now look at the other extreme, materials
with large sDK values (e.g.
metals), both n and k will
become large. |
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Looking at the Fresnel
equations we see that for large n values the intensity of the
reflected beam approaches 100 %, and large k values mean that the little bit of light that is not
reflected will not go very deep. |
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Light that hits a good conductor thus will be mostly reflected
and does not penetrate. Well, that is exactly what happens when light hits a
metal, as we know from everyday experience. |
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© H. Föll (Advanced Materials B, part 1 - script)