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Journal of Natural Sciences Research                                                          www.iiste.org
ISSN 2224-3186 (Paper) ISSN 2225-0921 (Online)
Vol.1, No.2, 2011
   The Optical Constants of Highly Absorbing Films Using the
        Spectral Reflectance Measured By Double Beam
                      Spectrophotometer
                                           ElSayed Moustafa1*
           1. Faculty of science , El-Azhar university, physics department, Assuit, 71511, Egypt
          * e-mail of the corresponding author: Sayed19652000@yahoo.com

Abstract
  The optical constants of the metal thin films of Rhodium have been determined, the phase angles was
determined using the measured spectral reflectance R(λ) by Kramers-Kronig relations. Then, the real part
of the refractive index is calculated by the approach of Heavens when the film is highly absorbing, in that
range the real refractive was found to be in order of the extinction coefficient k.
The interference reflectance spectra at normal incidence for different thicknesses of amorphous metal films
deposited by thermal evaporation have been obtained in the spectral range 400–800 nm. We propose a
method for determination of the refractive index and extinction coefficients of highly absorbing films. This
method is based on measurements of reflectance of the film at normal incidence alone, simulations of the
theoretical accuracy and the effect of the error of the spectral reflectance measurements in the
determination of the optical constants of the film are analyzed.
Keywords: optical constants , refractive index , thin film ,reflectance and absorption coefficient .
1. Introduction

The determination of the optical properties of thin films is a topic of fundamental and technological
importance ( Jyh-Jian Chen, et al ,1999 ). Most of the optical applications of metal coating are based on the
knowledge of the optical constants. For the metal coating (Rh) film which was used, this metal is inert , so
changes due to oxidations should be minimal. The optical constants are important parameters for predicting
the performance of an optical system. The optical constants are sensitive to the microstructure, which is
effected by the deposition conditions.

A good knowledge of film parameters is necessary for the design and manufacture of new optical coatings
and devices such as multilayers coatings and regulate filters[ Manifacier.J.C, et al 1976]. An optical
constant is sometimes called a complex refractive index and is described by the expression of (n-ik), where
n and k are the refractive index and the extinction coefficient respectively of the film. Measurements of
the optical constants of highly absorbing thin films on transparent or slightly absorbing substrates have
been extensively investigated. Especially the method based on only a single measurements of the
transmission spectrum at normal incidence is widely used to determine the refractive index and extinction
coefficient of a film( Swanepoel. R, 1984). Also, there are the method of interference of the spectral
transmittance and reflectance ( Özcan Bazkir,2007 ).

2.Theoretical considerations

In the highly absorbing films, according to the notation of Heaven, the reflectance can
approach to the following formula :

                              (n − 1) 2 − k 2
                       Rf =                                       (1)
                              (n + 1) 2 + k 2

In the above approach the sample is considered to be in air so n0=1, the refractive index
of vacuum and practically the incident rays are quasi-parallel.



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Journal of Natural Sciences Research                                                          www.iiste.org
ISSN 2224-3186 (Paper) ISSN 2225-0921 (Online)
Vol.1, No.2, 2011
In the fundamental absorption region (i.e., αf ≥ 105 cm-1 or αfdf ≥ 1), transmission
measurements become impractical and the optical constants have to be determined from
reflectivity measurements alone. This is possible, in principle, when the amplitude r and phase angle θ of
the complex reflectivity are both determined as a function of hω as follows:

                                 r (ω ) = r (ω )e iθ
                                 ˆ                                             (2)

It is achieved in ellipsometry where the polarization state of a light beam impinging at non-normal
incidence onto the specimen surface is a analyzed ( J.D .Joannopoulos & G.Lucovsky, 1984). Since
ellipsometry is very surface sensitive, it has so far been applied to study the growth and the oxidation of
plasma deposited amorphous films. An ε2 spectrum of HF etched a-SiH is given in (J.D .Joannopoulos &
G.Lucovsky ,1984). It is possible to derive both r(ω) and θ(ω) from measurements of |r2|2 at normal
incidence alone using the Kramers-Kronig dispersion relationship between r and θ (Özcan Bazkir,2007 ), as
follows:

                                         ω0            ln r (ω )
                           θ (ω0 ) = −         ∫
                                                   ∞
                                                                 dω                  (3)
                                         π     0
                                                       ω 2 − ω02

On the other hand the phase angle θ = 2π/λ( n - ik ).d                           ( 4)

d is the film thickness.




                                              df        nf film       nf = (n -ik)

                                          n1 ≡ ns             substrate

                                      no =1                               d2

 Figure ( 1 ) demonstrates the optical constants used in the calculation of thin highly absorbing
                                               film

 The Kramers-Kronig relationship links the value of θ at a particular frequency ω0 to an integral over
reflectivities extending over all energies hω. The latter is, however, only known over a limited region in ω
and methods have therefore been developed to extrapolate r(ω) to very low or very high frequencies in a
physically reasonable way.

The sum rules relations are considerable help in this procedure. The most useful of these in the present
work is that which relates ε∞, the long wavelength dielectric constant to an integral over ε2 (ω) .




24 | P a g e
www.iiste.org
Journal of Natural Sciences Research                                                             www.iiste.org
ISSN 2224-3186 (Paper) ISSN 2225-0921 (Online)
Vol.1, No.2, 2011
 The advantage of the methods that use the envelope of transmittance or reflectance measurements is that
the dispersion of the complex refractive index of the index of a thin film is obtained easily. The
disadvantage. However, is that the thin film must be thick (J.M.Gonzalez-leal et al, 2004 ). Here there is no
new method for n and k determination of the film . But an improvement to obtain the accurate values of
the optical constants by comparing two methods, one of them is the interference method and the other is a
method depends on the spectral reflectance of the film involved the correction of the multi-reflections
inside the substrate.

The theoretical idea of this work is the determination of the optical constants nf and kf for the highly
absorbing films using the measured reflectance Rf at normal incidence using KK relations.

3.Results and discussions

The reflectance of the samples has been measured by double beam spectrophotometer with high accuracy
± 1% as shown in figure ( 2 ). To obtain the accurate values of the optical constants by comparing two
methods, one of them is the interference method which depends on the maxima and minima of the
transmittance and reflectance (Yanfi Zheng & Kazuo kikuchi,1997), the other is a method depends on the
spectral reflectance of the film involved the correction of the multi-reflections inside the substrate. Figures
( 2 ) shows the experimental spectral reflectance of Rh film, by applying equation (3),we calculated the
values of the phase angle using the measured reflectance data, the value of θ has been found to be 1.8435 .
Then by substitution in equation ( 2 ) and computing the Fresnel coefficients, the real refractive index n
and k have been determined, it is noted that the values of n and k are nearly equal as the thickness of the
film decreases and the wavelength λ increases.

In this work the values of θ have been calculated from the integral ( 3 ) over the range from 1.55 - 4.14
eV. By solving equations ( 1 ) and ( 4 ), the real refractive index n can be determined , then the extinction
coefficient k can be estimated by equation ( 1 ). Where d is the film thickness and λ is the incidence
wavelength.

ω0 in the calculations has been taken to be around 0.75*1015 Hz , and the interval dω was 1 Hz. As the
extrapolation of the reflectance increases , this means more accuracy.

The integral ( 3 ) has been estimated numerically using a computerizing program, the uncertainty of
estimation within ± 2%.

Table (1) illustrates the values of the calculated refractive index nkk and the extinction coefficient kkk of the
absorbing film comparing them with that determined by interference method of R(λ) and T(λ). It is clear
that the error between the two values is acceptable with respect to this type of measurements around ± 5%.
The advantage of this method its accuracy because the optical constants directly determine from the
measured spectral reflectance R(λ) of the film especially the metal films at normal incidence.

5. Conclusions

-From the previous analysis it was conclude that the optical constants of film depend on the method of
calculation. The accuracy of the suggested method depends on the extrapolation of the curve of the
spectral reflectance of the sample.

-It is preferable to use the spectral reflectance measured by the spectrophotometer at normal incidence as
the film is highly absorbing and the thickness is thin.

-Table ( 1 ) are very important in the calculation of the optical constants of the highly absorbing films.

References:

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www.iiste.org
Journal of Natural Sciences Research                                                          www.iiste.org
ISSN 2224-3186 (Paper) ISSN 2225-0921 (Online)
Vol.1, No.2, 2011
Arndt.D.P, Borgongo.J.P.,Azzam.R.M & Bennett.J.P,(1984), "Multiple determination of the optical
constants of thin-film coating materials ", Applied Optics,vol.23,No.20,3571-3580.

Borgongo . J. P , Lazarides . B, & Pelletier . E,(1982), "Automatic determination of the optical constants
of inhomogeneous thin films", Applied optics , vol . 21, No. 22, 4020.

Minkov. D. A, (1989) , " Calculation of the optical constants of a layer upon a transparent substrate from
the reflection spectra ", J.Phys.D:Appl.Phys.22,1157.

Manifacier. J.C, Gasiot. J & Fillard. J.P, (1976 ), " A simple method for the determination of the optical
constants and thickness of weakly absorbing films ", J. Phys. E., 9, 1002-1004 .

Joannopoulos. J.D and Lucovsky. G, (1984)," The physics of hydrogenated amorphous silicon II ",
Springer- Verlag ,Berlin Heidelberg.

Jyh-Jian Chen, Jenn- Der Lin, & Long-Jye Sheu, (1999), " Simultaneous measurements of spectral optical
properties and thickness of an absorbing thin films on a substrate ",Thin Solid Films, 354, 176 -186.

Gonzalez-Leal. J.M, Pr ieto-Alcon. R, Stuchlik. M, Vlcek. M, Elliott. S.R, and Marquez. E,(2004),
"Determination of the surface roughness and refractive index of amorphous As40S60 films deposited by
spin coating," Opt. Mater. 27, 147-154 .

Özcan Bazk,ir, (2007), " Determination of optical constants of silicon photodiode from reflectivity
measurements at normal incidence of light ",Optics and Laser engineering , vol.45,issue 1,245-246.

  Swanepoel. R , (1983), "Determination of the thickness and optical constants of amorphous silicon",
J.Phys.E.Sci.Instrum.16, 1214.

Swanepoel. R , (1984)," Determination of the thickness and optical constants of the films using
transmission spectrum ", J.Phys.E:Sci.Instrum.,17,896.

Yanfi Zheng and Kazuo kikuchi,(1997), "Analytical method of determining optical constants of weakly
absorbing thin film ", Applied optics, vol,36,No.25,6325-6326.




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Journal of Natural Sciences Research                                                                                                  www.iiste.org
ISSN 2224-3186 (Paper) ISSN 2225-0921 (Online)
Vol.1, No.2, 2011




*The Author had been born in 1965, Egypt ,and has BSc in 1986 in physics, Msc in experimental physics
1993, and the ph.D in solid state and optical properties of films in 2000. Associated prof. in physics in 2006
,the field of research is the optical and electrical properties of solids ( glasses , coating films, solar cells ).
My institution is Faculty of science , El-Azhar university, physics department, Assuit, 71511, Egypt.




                                            0              2                4                 6                 8              10
                                     0.44                                                                                        10


                                                                                                           Rh-film 14 nm
                                                                                                                                8
                    reflectaance %




                                                                                                                                6

                                     0.43

                                                                                                                                4




                                                                                                                                2




                                     0.42                                                                                       0
                                                400               500               600              700               800
                                                                                 wavelength λ
                                                Figure ( 2a) illustrates the spectral reflectance of Rh film (14nm ) meaured
                                                                           by the spectrophotometer




27 | P a g e
www.iiste.org
Journal of Natural Sciences Research                                                                                                        www.iiste.org
ISSN 2224-3186 (Paper) ISSN 2225-0921 (Online)
Vol.1, No.2, 2011

                                           0                 2                 4                 6                8                10
                                                                                                                                     10

                                    0.59
                                                                                               Rh-27.1 nm
                                                                                                                                     8
                                    0.58
                    Reflectance %



                                    0.57                                                                                             6



                                    0.56                                                                                             4


                                    0.55
                                                                                                                                     2


                                    0.54

                                                                                                                                     0
                                           350      400       450      500         550     600        650      700       750       800
                                                                                    wavelength λ
                                                 Figure ( 2b) illustrates the spectral reflectance of Rh film (27.1 nm ) meaured
                                                                              by the spectrophotometer



 Table. ( 1 ) : A comparison between the calculated and reported values of the refractive index n and the
                                 extinction coefficient K for the Rh films

Material    Wavelength                           Thickness             Measured                Refractive             Extinction
                λ                                    t                 reflectivity            index nkk              coefficient          nf     Kf
               nm                                                           R                                             k kk
   Rh          450                                                       0.4367                      2.550              2.551              2.4   3.28
               500                                                       0.4322                      2.500              2.522              2.6   3.40
               550                                  14.2                 0.4311                      2.50                2.51             2.78   3.53
               600                                                       0.4294                      2.50                2.51             2.95   3.65
               650                                                       0.4284                      2.50                2.50             3.11   3.77
               700                                                       0.4282                      2.497               2.50             3.23   3.91



                 450                                                       0.5597                    2.50                  3.54           2.27   3.25
                 500                                                       0.5649                    2.56                  3.58           2.39   3.41
  Rh             550                                 27.1                  0.5698                    2.60                  3.62           2.51   3.58
                 600                                                       0.5745                    2.62                  3.69           2.62   3.74
                 650                                                       0.5770                    2.65                  3.70           2.75   3.88
                 700                                                       0.5797                    2.70                  3.76           2.78   4.03



*Reported n and k according to ( Arndt D.P, Borgongo . J. P. et al,1984).




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The optical constants of highly absorbing films using the spectral reflectance measured by double beam spectrophotometer

  • 1. Journal of Natural Sciences Research www.iiste.org ISSN 2224-3186 (Paper) ISSN 2225-0921 (Online) Vol.1, No.2, 2011 The Optical Constants of Highly Absorbing Films Using the Spectral Reflectance Measured By Double Beam Spectrophotometer ElSayed Moustafa1* 1. Faculty of science , El-Azhar university, physics department, Assuit, 71511, Egypt * e-mail of the corresponding author: Sayed19652000@yahoo.com Abstract The optical constants of the metal thin films of Rhodium have been determined, the phase angles was determined using the measured spectral reflectance R(λ) by Kramers-Kronig relations. Then, the real part of the refractive index is calculated by the approach of Heavens when the film is highly absorbing, in that range the real refractive was found to be in order of the extinction coefficient k. The interference reflectance spectra at normal incidence for different thicknesses of amorphous metal films deposited by thermal evaporation have been obtained in the spectral range 400–800 nm. We propose a method for determination of the refractive index and extinction coefficients of highly absorbing films. This method is based on measurements of reflectance of the film at normal incidence alone, simulations of the theoretical accuracy and the effect of the error of the spectral reflectance measurements in the determination of the optical constants of the film are analyzed. Keywords: optical constants , refractive index , thin film ,reflectance and absorption coefficient . 1. Introduction The determination of the optical properties of thin films is a topic of fundamental and technological importance ( Jyh-Jian Chen, et al ,1999 ). Most of the optical applications of metal coating are based on the knowledge of the optical constants. For the metal coating (Rh) film which was used, this metal is inert , so changes due to oxidations should be minimal. The optical constants are important parameters for predicting the performance of an optical system. The optical constants are sensitive to the microstructure, which is effected by the deposition conditions. A good knowledge of film parameters is necessary for the design and manufacture of new optical coatings and devices such as multilayers coatings and regulate filters[ Manifacier.J.C, et al 1976]. An optical constant is sometimes called a complex refractive index and is described by the expression of (n-ik), where n and k are the refractive index and the extinction coefficient respectively of the film. Measurements of the optical constants of highly absorbing thin films on transparent or slightly absorbing substrates have been extensively investigated. Especially the method based on only a single measurements of the transmission spectrum at normal incidence is widely used to determine the refractive index and extinction coefficient of a film( Swanepoel. R, 1984). Also, there are the method of interference of the spectral transmittance and reflectance ( Özcan Bazkir,2007 ). 2.Theoretical considerations In the highly absorbing films, according to the notation of Heaven, the reflectance can approach to the following formula : (n − 1) 2 − k 2 Rf = (1) (n + 1) 2 + k 2 In the above approach the sample is considered to be in air so n0=1, the refractive index of vacuum and practically the incident rays are quasi-parallel. 23 | P a g e www.iiste.org
  • 2. Journal of Natural Sciences Research www.iiste.org ISSN 2224-3186 (Paper) ISSN 2225-0921 (Online) Vol.1, No.2, 2011 In the fundamental absorption region (i.e., αf ≥ 105 cm-1 or αfdf ≥ 1), transmission measurements become impractical and the optical constants have to be determined from reflectivity measurements alone. This is possible, in principle, when the amplitude r and phase angle θ of the complex reflectivity are both determined as a function of hω as follows: r (ω ) = r (ω )e iθ ˆ (2) It is achieved in ellipsometry where the polarization state of a light beam impinging at non-normal incidence onto the specimen surface is a analyzed ( J.D .Joannopoulos & G.Lucovsky, 1984). Since ellipsometry is very surface sensitive, it has so far been applied to study the growth and the oxidation of plasma deposited amorphous films. An ε2 spectrum of HF etched a-SiH is given in (J.D .Joannopoulos & G.Lucovsky ,1984). It is possible to derive both r(ω) and θ(ω) from measurements of |r2|2 at normal incidence alone using the Kramers-Kronig dispersion relationship between r and θ (Özcan Bazkir,2007 ), as follows: ω0 ln r (ω ) θ (ω0 ) = − ∫ ∞ dω (3) π 0 ω 2 − ω02 On the other hand the phase angle θ = 2π/λ( n - ik ).d ( 4) d is the film thickness. df nf film nf = (n -ik) n1 ≡ ns substrate no =1 d2 Figure ( 1 ) demonstrates the optical constants used in the calculation of thin highly absorbing film The Kramers-Kronig relationship links the value of θ at a particular frequency ω0 to an integral over reflectivities extending over all energies hω. The latter is, however, only known over a limited region in ω and methods have therefore been developed to extrapolate r(ω) to very low or very high frequencies in a physically reasonable way. The sum rules relations are considerable help in this procedure. The most useful of these in the present work is that which relates ε∞, the long wavelength dielectric constant to an integral over ε2 (ω) . 24 | P a g e www.iiste.org
  • 3. Journal of Natural Sciences Research www.iiste.org ISSN 2224-3186 (Paper) ISSN 2225-0921 (Online) Vol.1, No.2, 2011 The advantage of the methods that use the envelope of transmittance or reflectance measurements is that the dispersion of the complex refractive index of the index of a thin film is obtained easily. The disadvantage. However, is that the thin film must be thick (J.M.Gonzalez-leal et al, 2004 ). Here there is no new method for n and k determination of the film . But an improvement to obtain the accurate values of the optical constants by comparing two methods, one of them is the interference method and the other is a method depends on the spectral reflectance of the film involved the correction of the multi-reflections inside the substrate. The theoretical idea of this work is the determination of the optical constants nf and kf for the highly absorbing films using the measured reflectance Rf at normal incidence using KK relations. 3.Results and discussions The reflectance of the samples has been measured by double beam spectrophotometer with high accuracy ± 1% as shown in figure ( 2 ). To obtain the accurate values of the optical constants by comparing two methods, one of them is the interference method which depends on the maxima and minima of the transmittance and reflectance (Yanfi Zheng & Kazuo kikuchi,1997), the other is a method depends on the spectral reflectance of the film involved the correction of the multi-reflections inside the substrate. Figures ( 2 ) shows the experimental spectral reflectance of Rh film, by applying equation (3),we calculated the values of the phase angle using the measured reflectance data, the value of θ has been found to be 1.8435 . Then by substitution in equation ( 2 ) and computing the Fresnel coefficients, the real refractive index n and k have been determined, it is noted that the values of n and k are nearly equal as the thickness of the film decreases and the wavelength λ increases. In this work the values of θ have been calculated from the integral ( 3 ) over the range from 1.55 - 4.14 eV. By solving equations ( 1 ) and ( 4 ), the real refractive index n can be determined , then the extinction coefficient k can be estimated by equation ( 1 ). Where d is the film thickness and λ is the incidence wavelength. ω0 in the calculations has been taken to be around 0.75*1015 Hz , and the interval dω was 1 Hz. As the extrapolation of the reflectance increases , this means more accuracy. The integral ( 3 ) has been estimated numerically using a computerizing program, the uncertainty of estimation within ± 2%. Table (1) illustrates the values of the calculated refractive index nkk and the extinction coefficient kkk of the absorbing film comparing them with that determined by interference method of R(λ) and T(λ). It is clear that the error between the two values is acceptable with respect to this type of measurements around ± 5%. The advantage of this method its accuracy because the optical constants directly determine from the measured spectral reflectance R(λ) of the film especially the metal films at normal incidence. 5. Conclusions -From the previous analysis it was conclude that the optical constants of film depend on the method of calculation. The accuracy of the suggested method depends on the extrapolation of the curve of the spectral reflectance of the sample. -It is preferable to use the spectral reflectance measured by the spectrophotometer at normal incidence as the film is highly absorbing and the thickness is thin. -Table ( 1 ) are very important in the calculation of the optical constants of the highly absorbing films. References: 25 | P a g e www.iiste.org
  • 4. Journal of Natural Sciences Research www.iiste.org ISSN 2224-3186 (Paper) ISSN 2225-0921 (Online) Vol.1, No.2, 2011 Arndt.D.P, Borgongo.J.P.,Azzam.R.M & Bennett.J.P,(1984), "Multiple determination of the optical constants of thin-film coating materials ", Applied Optics,vol.23,No.20,3571-3580. Borgongo . J. P , Lazarides . B, & Pelletier . E,(1982), "Automatic determination of the optical constants of inhomogeneous thin films", Applied optics , vol . 21, No. 22, 4020. Minkov. D. A, (1989) , " Calculation of the optical constants of a layer upon a transparent substrate from the reflection spectra ", J.Phys.D:Appl.Phys.22,1157. Manifacier. J.C, Gasiot. J & Fillard. J.P, (1976 ), " A simple method for the determination of the optical constants and thickness of weakly absorbing films ", J. Phys. E., 9, 1002-1004 . Joannopoulos. J.D and Lucovsky. G, (1984)," The physics of hydrogenated amorphous silicon II ", Springer- Verlag ,Berlin Heidelberg. Jyh-Jian Chen, Jenn- Der Lin, & Long-Jye Sheu, (1999), " Simultaneous measurements of spectral optical properties and thickness of an absorbing thin films on a substrate ",Thin Solid Films, 354, 176 -186. Gonzalez-Leal. J.M, Pr ieto-Alcon. R, Stuchlik. M, Vlcek. M, Elliott. S.R, and Marquez. E,(2004), "Determination of the surface roughness and refractive index of amorphous As40S60 films deposited by spin coating," Opt. Mater. 27, 147-154 . Özcan Bazk,ir, (2007), " Determination of optical constants of silicon photodiode from reflectivity measurements at normal incidence of light ",Optics and Laser engineering , vol.45,issue 1,245-246. Swanepoel. R , (1983), "Determination of the thickness and optical constants of amorphous silicon", J.Phys.E.Sci.Instrum.16, 1214. Swanepoel. R , (1984)," Determination of the thickness and optical constants of the films using transmission spectrum ", J.Phys.E:Sci.Instrum.,17,896. Yanfi Zheng and Kazuo kikuchi,(1997), "Analytical method of determining optical constants of weakly absorbing thin film ", Applied optics, vol,36,No.25,6325-6326. 26 | P a g e www.iiste.org
  • 5. Journal of Natural Sciences Research www.iiste.org ISSN 2224-3186 (Paper) ISSN 2225-0921 (Online) Vol.1, No.2, 2011 *The Author had been born in 1965, Egypt ,and has BSc in 1986 in physics, Msc in experimental physics 1993, and the ph.D in solid state and optical properties of films in 2000. Associated prof. in physics in 2006 ,the field of research is the optical and electrical properties of solids ( glasses , coating films, solar cells ). My institution is Faculty of science , El-Azhar university, physics department, Assuit, 71511, Egypt. 0 2 4 6 8 10 0.44 10 Rh-film 14 nm 8 reflectaance % 6 0.43 4 2 0.42 0 400 500 600 700 800 wavelength λ Figure ( 2a) illustrates the spectral reflectance of Rh film (14nm ) meaured by the spectrophotometer 27 | P a g e www.iiste.org
  • 6. Journal of Natural Sciences Research www.iiste.org ISSN 2224-3186 (Paper) ISSN 2225-0921 (Online) Vol.1, No.2, 2011 0 2 4 6 8 10 10 0.59 Rh-27.1 nm 8 0.58 Reflectance % 0.57 6 0.56 4 0.55 2 0.54 0 350 400 450 500 550 600 650 700 750 800 wavelength λ Figure ( 2b) illustrates the spectral reflectance of Rh film (27.1 nm ) meaured by the spectrophotometer Table. ( 1 ) : A comparison between the calculated and reported values of the refractive index n and the extinction coefficient K for the Rh films Material Wavelength Thickness Measured Refractive Extinction λ t reflectivity index nkk coefficient nf Kf nm R k kk Rh 450 0.4367 2.550 2.551 2.4 3.28 500 0.4322 2.500 2.522 2.6 3.40 550 14.2 0.4311 2.50 2.51 2.78 3.53 600 0.4294 2.50 2.51 2.95 3.65 650 0.4284 2.50 2.50 3.11 3.77 700 0.4282 2.497 2.50 3.23 3.91 450 0.5597 2.50 3.54 2.27 3.25 500 0.5649 2.56 3.58 2.39 3.41 Rh 550 27.1 0.5698 2.60 3.62 2.51 3.58 600 0.5745 2.62 3.69 2.62 3.74 650 0.5770 2.65 3.70 2.75 3.88 700 0.5797 2.70 3.76 2.78 4.03 *Reported n and k according to ( Arndt D.P, Borgongo . J. P. et al,1984). 28 | P a g e www.iiste.org