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Ординатура / Офтальмология / Английские материалы / Optics Learning by Computing with Examples using MATLAB_Dieter Moller_2007

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320

8. OPTICAL CONSTANTS

polarized and has an effect on the oscillator under consideration. The local field at the oscillator must be corrected. This is called the Lorentz correction and the effective field at the site of the charges is

E + (1/3ε0)P .

(8.24)

Using P ε0NαE we have

 

Py ε0{Ey + (Py /3ε0)}.

(8.25)

Similar to the low density case, using Eq. (8.9), the square of the refractive index for the denser medium is

n2 1

+ Nα/(1 (Nα/3)).

(8.26)

This equation may also be written as

 

3(n2

1)/(n2 + 2)

(8.27)

and is called the Clausius–Mossotti equation, or with the parameters of our model,

n2 1 + 3ε0ωp2 /{3(ω02 ω2 iγ ω) ωp2 }.

(8.28)

We have in a solid that the interaction between the oscillators becomes very strong. The oscillation frequencies are modified and the damping constants become large. In addition, in crystals the periodicity must be taken into account.

8.3 DETERMINATION OF OPTICAL CONSTANTS

8.3.1 Fresnel’s Formulas and Reflection Coefficients

The determination of the two parts n and K of the complex refractive index may be accomplished by using reflection measurements. In Chapter 5 we found that Fresnel’s formulas relate the reflection coefficients of the p- and s-polarization cases to the real index of refraction. In a similar way to that of Chapter 5, one can show that the complex reflection coefficients are related to complex refractive indices through Fresnel’s formulas. Replacing n2 by n2 n2 iK2 we have for the reflection coefficients

r

 

(n2

iK2) cos θ n1 cos θ

 

(8.29)

(n2

iK2) cos θ + n1 cos θ

 

 

 

r

 

 

n1 cos θ (n2

iK2) cos θ

.

(8.30)

n1 cos θ + (n2

 

 

 

iK2) cos θ

 

In order to represent r and r depending on the angle of incidence. We need the law of refraction in complex terms (see FileFig 8.4 (M4SNELL) of Chapter 5). The law of refraction is

n1 sin θ (n2 iK2) sin θ .

(8.31)

8.3. DETERMINATION OF OPTICAL CONSTANTS

321

The angle θ must be a complex quantity since the left side of Eq. (8.31) is real. Introduction of Eq. (8.31) into Eqs. (8.29) and (8.30) gives us

r

 

(n2

iK2) cos θ n1

1 − {(n1 sin θ)/(n2

iK2)}2

 

(8.32)

 

 

 

 

 

 

 

(n2

iK2) cos θ + n1

1 − {(n1 sin θ)/(n2

iK2)}2

 

 

 

 

 

n1 cos θ (n2

iK2)

 

 

.

 

r

 

 

 

1 − {(n1 sin θ)/(n2

iK2)}2

(8.33)

n1 cos θ + (n2

 

 

 

 

 

iK2)

1 − {(n1 sin θ)/(n2

iK2)}2

 

In FileFig 8.1 we have graphs of the absolute value and the argument for reflected amplitudes of the parallel (zrp) and perpendicular (zrs) cases depending on n and K. For K 0 we see from the first graph that for the parallel case the minimum corresponding to the Brewster angle is not zero. The angle at the minimum is called the principal angle. The second graph shows the phase jump at the Brewster angle, which is now a smooth transition. In the application of FileFig 8.1, Section 3, we plot the parallel (zrp) and perpendicular (zrs) cases for several different values of n and K on the same graph.

FileFig 8.1 (O1FRNKPSS)

Graphs are shown for reflected amplitudes of the parallel (zrp) and perpendicular (zrs) cases depending on n and K for n1 1. For both cases the absolute value of the reflected amplitudes and the phase angle are plotted for n1 1, n2 1.5, and K 2.

O1FRNKPSS is only on the CD.

Application 8.1.

1.Make a graph and find the values of the principal angle for one value of n and three values of K.

2.Make a graph and find the values of the principal angle for one value of K and three values of n.

3.Observe that the curve of arg(zrp(θ)) is not continuously approaching the curve of arg(zrs(θ)) when K is going from 0.01 to zero. What is the remaining phase difference?

8.3.2 Ratios of the Amplitude Reflection Coefficients

Equations (8.32) and (8.33) give the dependence of the reflection coefficients on n and K. We have the general problem that we cannot represent n and K as functions of rs and rp. This is only possible for approximations, (see Appendix 8.1), and other methods have to be considered.

322

8. OPTICAL CONSTANTS

One method is to apply reflection measurements at several angles of incidence to determine the absolute values of the ratio rs /rp. The ratio rs /rp is calculated similarly to that done by Born and Wolf (1964, p.617).

From Chapter 5 the ratio r /r from Fresnel’s formulas is

r /r [(n1 cos θ n2 cos θ

)/(n1 cos θ + n2 cos θ

)]/

(8.34)

[(n2 cos θ n1 cos θ

)/(n2 cos θ + n1 cos θ

)].

(8.35)

Using the law of refraction and the trigonometric formula for the sum of angles

cos(a ± b) cos a cos b ± sin a sin b

(8.36)

we get

 

| rs /rp | | cos(θ θ )/ cos(θ + θ ) | .

(8.37)

In FileFig 8.2 we show graphs of the real parts of rp and rs for various values of n and K. The third graph shows the ratio rp/rs and the fourth rs /rp. From these two graphs it appears that the ratio rp/rs is much more useful for the determination of optical constants than the ratios rs /rp, because they are smooth and do not show a resonance, related to the appearance of the Brewster angle. The optical constants may be obtained by measuring values of |rp/rs | for two different angles of θ, and solving the two equations for the unknowns n and K.

FileFig 8.2 (O2FRSOPS)

Graphs are shown for the real part of the ratios rs /rp and rp/rs , calculated with the expressions used in FileFig 8.1, for n1 1, n2 1.5, nn2 1.5, K 0.1, and K 0.01, KK 0.5, KKK 2.

O2FRSOPS is only on the CD.

8.3.3 Oscillator Expressions

8.3.3.1 One Oscillator

To fit experimental data of a narrow frequency range, in which we have a resonance feature, one may use for n + iK a similar expression derived in Eq. (8.23) but extended to four parameters,

n + iK A + S/[1 (ν/ν0)2 γ (ν/ν0)],

(8.38)

where A is a general constant, S the oscillator strength, γ the damping constant, and ν0 ω0/2π the resonance frequency. An example is shown in Figure 8.2 and a calculation given in FileFig 8.3.

8.3. DETERMINATION OF OPTICAL CONSTANTS

323

FIGURE 8.2 Optical constants of bone charcoal powder. Resonance of vibrations of Ca, P , and O atoms against each other. (From Tomasecli et al., infrared optical constants of black powders determined from measurements, Applied Optics, 1981, 20, 3961–3967.)

FileFig 8.3 (O3OSTINS)

Graphs are shown of Eq. (8.37) for A 20, S1 0.09, γ 1 0.002, and v01 1050 cm1. An analytical approximation for n close to 1 and small K is also presented.

O3OSTINS is only on the CD.

Application 8.3.

1.Change γ and observe the change in resonance wavenumber and the height of the imaginary part.

2.Change S and observe the change in resonance wavenumber and the height of the imaginary part.

3.Modify the graphs by plotting in addition a graph using S2 0.19, γ 2 0.03, and ν02 1150 cm1. Change parameters and study the effect on n and K.

4.Modify the graphs of the thin medium by also plotting a graph using different values of a2 and c2. Change a1, a2 and c1 and cc and compare the effect on n and K.

8.3.3.2 Many Oscillator Terms

The dependence of the electrical polarization on the frequency over a large range suggests that one uses more than one oscillator term in the formula for the

324

8. OPTICAL CONSTANTS

FIGURE 8.3 The dependence of the polarizability on frequency for the microwave, infrared, and ultraviolet regions.

representation of n and K (schematically shown in Figure 8.3). Having measured n and K over a large range of frequencies, the experimental data are fit to formulas such as

n2 K2

1 +

fj ωp2 (ωoj2 ω2)/((ωoj2 ω2)2 + (γj ω)2)

(8.39)

 

 

j

 

2nK

j

ωp2 fj γj ω/((ωoj2 ω2)2 + (γj ω)2),

(8.40)

 

 

 

where fj , γj , and ωoj are empirical constants. The constants in these expressions are determined by a “best fit" calculation over a large range of frequencies with respect to the measured values of n and K

8.3.4 Sellmeier Formula

Similarly to what has been discussed for the oscillator expression, one may fit experimental data to represent the dependence of n and K on the wavelength by using a polynomial approach of the type

j N

 

n2 c1 + c2λ4/(λ2 c3) + aj λ2/(λ2 bj ).

(8.41)

j 1

 

8.3. DETERMINATION OF OPTICAL CONSTANTS

325

This is called a Sellmeier-type equation and has been used, for example, to fit the data for potassium bromide in the spectral region from .2 to 42 microns using 11 empirical constants.1 An example is given in FileFig 8.4.

When fitting experimental data one has to keep in mind that n and K are not independent. They are related by the Kramer–Kroning model.2 In some spectral regions, for example in the x-ray region, one obtains the K value from absorption measurements and calculates the corresponding n value with the Kramer–Kroning model.

FileFig 8.4 (O4SELMRS)

A graph of a Sellmeier expression n(λ) for fused quartz is shown for the range of λ from 4000 to 8000 Angstrom using parameters ci with i 1 to 3.

O4SELMRS

Graph for Demonstration of the Sellmeier Presentation of the Refractive Index

For fused quartz we have

 

 

 

 

 

 

 

 

c1 : 1.448

c2 : 3.3 · 105

 

 

c3

: 1.23 · 1011

 

λ : 4000, 4001 . . . 8000

 

n(λ) : c1 +

c2

+

c3

 

 

 

 

 

 

.

 

 

λ2

λ4

 

l

l

Application 8.4. Determination (backward) of the constants c1, c2, and c3. Read from the graph three values of λi and the corresponding value of n(λi ). Consider c1 to c3 as unknown and formulate a system of linear equations. One

1E. D. Palik, Handbook of Optical Constants of Solids II, Academic Press, New York, 1991.

2Charles Kittel, Introduction to Solid State Physics, John Wiley & Sons, New York, 1967.

326

8. OPTICAL CONSTANTS

would be n(λi ) c1 + c22i + c34i . Solve the system of these inhomogeneous linear equations with one of the available computer programs. Make an estimate of the error.

8.4 OPTICAL CONSTANTS OF METALS

8.4.1 Drude Model

In Section 8.2 we discussed the optical constants of dielectrics and in Section 8.3 their determination. We now discuss metals and how their optical constants are also described by a complex refractive index. The determination of the n and K values for metals is similar to what has been discussed before, but the model representing the material is different.

Metals show high reflectivity in the visible and infrared spectral regions and their attenuation increases with lower frequencies. The values of real and imaginary parts of the refractive index of metals are in the lower frequency region which is much higher than one usually finds for dielectrics.

The interaction of the electromagnetic wave with the metal is described by the Drude model. The electrons are assumed to move almost freely in the metal and there is no restoring force to make the electrons vibrate, as discussed for the dielectric. For an isotropic medium with free conducting charges we write Maxwell’s equations as

× E B/∂t

 

c2 × B E/∂t + j0

(8.42)

· E 0

 

· B 0.

 

This is similar to Eq. (8.1). For the current density vector j we take

 

j Nevj ,

(8.43)

where vj is called the drift velocity. The electrical field of the light and the current density in the material are related by the wave equation. We assume E and j are vibrating in the y direction and propagating in the x direction and from Eq. (8.41) we get for the wave equation

2Ey /∂x2 (1/c2)2Ey /∂t2 [1/(c2ε0)]∂jy /∂t.

(8.44)

As in Section 8.2, we now find an expression for jy in terms of the parameters of the damped oscillator model and the vibrating electrical field E0. The differential equation of the model is now without the force term,

md2u/dt2 + mγ du/dt eE0eiωt .

(8.45)

8.4. OPTICAL CONSTANTS OF METALS

327

The general solution of Eq. (8.44) is the sum of the solutions of the homogeneous and inhomogeneous equations. For the homogeneous equation,

md2u/dt2 + mγ du/dt 0.

(8.46)

Using the trial solution u u0et/τ , we get for γ τ 1. Typically one has a value of 1013 for τ and we neglect this solution.

The inhomogeneous equation may be rewritten, using v du/dt, as

 

mdv/dt + mγ v eE0eiωt ,

(8.47)

Using the trial solution v v0eiωt one obtains

 

v0 E0(e/m)/(γ ).

(8.48)

The current density j0 Nev0 can be expressed as

 

j0 (τ E0)(Ne2/m)/(1 iωτ ) (σ E0)/(1 iωτ ),

(8.49)

where we used j0 Nev0, γ τ 1, and the static conductivity

 

σ τ Ne2/m.

(8.50)

Equation (8.48) relates the current density j0 of our model to the electrical field E0 of the light, vibrating with angular frequency ω.

We now turn to the wave equation, (see Eq. (8.43)), using the trial solutions

Ey E0ei(kxωt) and jy j0ei(kxωt)

(8.51)

and introducing j0 from our model, Eq. (8.48), we obtain for the complex wave vector k

(k )2 1/c2{ω2 + (iσ ω/ε0)/(1 iωτ )}

(8.52)

and the complex refractive index n k c22,

 

(n )2 1 + iσ/{ωε0(1 iωτ )} 1 σ/{ωε0(i + ωτ )}.

(8.53)

Equation (8.52) relates the refractive index to the static conductivity of the metal σ , the frequency of light ω and the relaxation time τ , which is a parameter of our model and is related to the metal. In FileFig 8.5 we show graphs over a large frequency region of the real and imaginary parts of Eq. (8.52).

8.4.2 Low Frequency Region

For low frequencies, that is, when ωτ 1, we may neglect ωτ with respect to i (see Eq. (8.52)), and get

(n )2 1 + iσ/ωε0.

(8.54)

Since ω is small, which means iσ/ωε0 is large compared to 1, we write

 

 

 

 

 

 

n iK (

i

)( σ/ωε0).

(8.55)

328

8. OPTICAL CONSTANTS

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Using the identity

 

i (1 + i)/

 

2 one has

 

| n | | K | (

 

σ/2ωε0

);

(8.56)

that is, n and K have the same value and the wave is strongly attenuated in the medium. To find the frequency limit of Eq. (8.55), we have from ωτ 1,

that ω << 1, with τ mσ/Ne2. For copper we have σ 5.76 107 (ohm meter)1, N 8.5 1028 meter3, e 1.6 1019 coulomb, m 9.11 1031 kgm,

and obtain for 14.1 1013 1/sec. Therefore this approximation is valid for angular frequencies smaller than 1011 1012 Hz, which are lower frequencies than the far infrared. This approximation is plotted in FileFig 8.5 as the last graph. The light is strongly attenuated when entering metals in this spectral region and is therefore highly reflected (see also FileFig 8.7).

8.4.3 High Frequency Region

For high frequencies we have ωτ 1, and from Eq. (8.52) one has

n2

1

σ/ω2τ ε0.

(8.57)

Using Eq. (8.49) and the plasma frequency ωp Ne2/mε0 we have

 

n2

1

ωp2 2.

(8.58)

The plasma frequency ωp Ne2/mε0 has the value 1.6 1016 1/sec when using N 8.5 1028 meter3, e 1.6 1019 coulomb, ε0 8.85 1012 farad-meter1,

and m 9.11 1031 kg. Therefore the approximation of Eq. (8.57) is valid for angular frequencies larger than 1018, corresponding to the x ray region. This is also plotted in FileFig 8.5 on the third graph. In this region the refractive index n is real and less than 1 and light is penetrating the metal without being attenuated.

We see that the plasma frequency divides the frequency range into two parts. One for high frequencies when n is smaller than 1 and one for low frequencies when n is complex (see Eq. (8.53)).

FileFig 8.5 (O5METALS)

Graphs of the real and imaginary part of n n + iK of copper, for the general case and for the high and low frequency approximations.

O5METALS

Calculation of n and k for Copper Using the Drude Model

Calculation of real and imaginary parts. Expression for low and high frequencies depending on angular frequency.

8.4. OPTICAL CONSTANTS OF METALS

329

1. General Expression

c : 3 · 108m/s

σ : 6 · 107 (OHMm)1

 

εo : 8.85 · 1012

C2/Nm

 

τ

:

4.1

1

 

 

sec

 

i :

 

 

 

 

 

 

 

 

·

1011

 

 

 

1

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

ω : 1011, (2 · 10)11 . . . 1018.

 

 

 

 

 

 

 

 

Angular frequency for 1 mm wavelength is 2π 300 10 9; see below. The

general expression for n ik zm(ω)

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

zm(ω) :

 

1

+

i · σ

·

1

 

i

1

ω

 

.

 

 

 

 

 

 

 

 

εo

·

ω

·

·

τ

 

 

 

.

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

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