Page 73 - Chalcogenide Glasses for Infrared Optics
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Chalcogenide Glasses      51

              component glasses and will yield the harmonic oscillator frequency
              for the dominant pair which in this case comprises Si-Te and Ge-Te.
              The other bond pairs absorb but not with the intensity required to
              produce a reflection band. Also, the intensity is affected by the con-
              centration of the element in the glass composition.
                 The optical constants are interdependent. That is, the refractive
              index is really a complex number N = n – ik, where n is the real part of
              the refractive index and k is the imaginary part of the refractive index,
              sometimes called the extinction coefficient. The bulk absorption coef-
              ficient α can be calculated from α = 4πk/λ,  where λ = wavelength in
              centimeters. Reflectivity R is calculated from

                                 R =  ( n− )1  2 +  k 2
                                     ( n+ )1  2  +  k  2
                    In the transparent region, k is very small and is omitted in the
              calculation. However, in the region of the Restrahlen band, it becomes
              large, even the dominant term. The curves in Fig. 2.18 show the
              expected shape. The peak of reflectivity, the maximum absorption
              wavelength, and the wavelength for the harmonic oscillator do not
              coincide because of the interrelationship of the optical constants. The
              wavelength of the harmonic oscillator for each bond pair and the
              maximum absorption were determined, when possible, by using
                                                37
              the inspection method described by Moss.  The values needed for the
              calculation are the magnitude of maximum reflectivity, the wave-
              length of maximum and minimum reflection, and the short wave-
              length refractive index. The calculated results found from the curves
              in Fig. 2.18 and for a number of other samples are shown in Table 2.9.
              In some cases only absorption results were available. From the results,
              we see that binary glasses are straightforward, yielding their oscilla-
              tor frequency, As-S, Ge-S, Ge-Se, As-Se. A small change is observed
              when a third element is present. The absorption of the third element
              is not intense enough to produce a second band whether due to the
              concentration or the ionic character of the bond. At the very least, the
              different mass of the atom when coupled to the primary structure
              produces a frequency change. As an example, compare the oscillator
              frequency for the Ge-S binary and in the ternary Ge-S-Te.
                 Tellurium is an atom much heavier than sulfur which lowers the
              frequency of vibration. The force constant for each atom pair may be
              calculated from

                                           κ  
                                              /
                                  ν =  1  ×   12
                                           µ
                                  o  2 πC  
              where  ν = wave number of harmonic oscillator frequency
                     o
                    C = speed of light
                    κ = force constant
                    µ = reduced mass
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