OPTI6105/8505
Optical Properties of Materials I
                       Spring Semester 2005
                   TH 12:30-1:50, Rm 116 Burson
                    Instructor: Vasily Astratov
                       Office: 141 Burson
                      Phone: 704 687 4513
                    Email: astratov@uncc.edu
            Office Hours: 4:00-5:00 T and 3:00-5:00 W
One semester introductory core course for M.S. and Ph.D. programs in Opt. Sci.
 and Engineering: propagation, absorption, reflection, transmission, scattering,
                luminescence, birefringence in various materials.
  We thank Dr. Angela Davies for providing teaching materials for this course
                Welcome to Spring Semester 2005!
Text:
Main: Mark Fox, Optical Properties of Solids, Oxford University Press, 2001
Suppl: B.E.A. Saleh and M.C. Teich, Fundamentals of Photonics, John
  Wiley&Sons, 1991
Suppl:N.W. Ashcroft and N.D. Mermin, Solid State Physics, Thomson
  Learning, 1976
Suppl: Charles Kittel, Introduction to Solid State Physics, John Wiley&Sons,
  8th Ed., 2005
Suppl: J.H. Simmons, Optical Materials, Acad. Press, 2000
Suppl: E. Hecht, Optics, Addison Wesley 1998
Grading:
Homeworks (~7, assigned occasionally)       25%
Student Presentations                       15%
Take Home Midterm Exam                      30%
Take Home Final Exam                         30%
Grades will be assigned using a 10-point grading scale:
A = 90-100, B=80-89, etc.
Syllabus
Will be posted on the physics webpage, changes are possible!
Course Content
Ist part: Fox: intoduction, opt constants, E&M review, complex refractive
index, January 11-25
2nd part: AM: crystal structure, reciprocal lattice, electron band structure,
phonons, January 25-Mid February
3rd part: Fox: dispersion relations, Kramers-Kroenig relations, free electron
model, Mid February- Spring Break (March 8-10)
4th part: Fox: interaction of light with phonons, elastic, Raman and Brillouin
scattering and glasses, March 15-end of March
5th part: Fox: birefringence, interband absorption, excitons, luminescence,
metals, molecular materials, April
               Lecture 1: lntroduction
Classification of
optical processes
                    • Refraction causes the light to propagate at smaller velocities
                    • Absorption occurs if frequency is resonant with electronic
                    transitions
                    • Luminescence is a spontaneous emission of light by atoms,
                    depends on radiative/nonradiative lifetimes
                    • Scattering is associated with changing direction, the total
                    number of photons is unchanged:
                    Elastic (Example: Rayleigh)
                    Inelastic (Example: Raman, Brillouin)
   EM Radiation can be any frequency
    HeNe laser,
                                       Note: Frequency rarely if ever
λ =633 nm     ~2eV
                                       changes. Would need to change the
                                       energy of the photons to do that.
  1 eV. photon has
 λ of 1.24 µ (in near IR)              Velocity set by properties of material.
                                       This then sets the wavelength
        Optical coefficients
   • Will be using a simple plane wave propagaton
   • Will be normal incidence
   • Will restrict ourselves to non-magnetic materials
• Reflectivity at a surface is described by the coefficient of reflectivity
• Coefficient of transmission or Transmissivity
    In the absence of scattering or
    absorption at the interface,
• The power reflection (R) and transmission (T) on each interface:
                                                 n1                                n1
                  n1 − n2 2                                       n2
              R=(         )                                T1                 T2
                  n1 + n2
                                                      R1                 R2
                 R +T =1
• The absorption of light by the medium is quantified by its absorption coefficient, α
               dI = −αdz × I (z )                          I(z)           I(z+dz)
           Beer’s Law:
                 I ( z ) = I 0 e −α z
                                                                     l
     Attenuation due to total thickness l:
                   I (l ) = I 0 e −αl
 • The refractive index depends on frequency, dispersion
 • The absorption coefficient is also a function frequency
 Responsible for the distinct color of some materials.
  Transmission through absorbing medium:
The absorption can be described in terms of the optical density, O.D. Called the
absorbance.
This can be written in terms of α
Will see OD as a specification for filters but not very useful as a general characterization of a material
because the value depends on thickness.
Scattering causes attenuation in the same way as absorption and can be
described similarly:
             I ( z ) = I 0 e − Nσ s z
                                                  Rayleigh scattering:
                                                                    1
                                                         σ s (λ ) ∝ 4
                                                                                           λ
Lecture 2: E&M Review
B.E.A. Saleh & M.C. Teich, Fundamentals of Photonics, John Wiley & Sons (1991)
Fox: Appendix A
                                                         Quantum optics
                                                         Semiclassical
                                                         E&M optics
                                                         Wave optics
                                                Ray optics
Quantum optics treats light and matter quantum mechanically
Semiclassical – treat light classically, but apply QM to atoms
E&M optics – treats both light and material classically
Wave optics is the scalar approximation of E&M
Ray optics is the limit of wave optics when λ is very short
  Goals: Maxwell’s Equations
  What determines phase velocity?
   Waves on strings                                 Sound Waves
          τ    elastic                                       B
    v=      =                                         v=
          µ   inertial                                       ρ
Require medium
For “tight” and “light” media v is higher
           EM wave doesn’t require medium!
           Maxwell’s Equations in Free Space
               ∂E
     ∇× H = ε0        (1)     Displacement current in a capacitor
               ∂t
                    ∂H
     ∇ × E = − µ0         (2)          Faraday Law+Lenz’s Rule
                     ∂t
         ∇⋅E = 0          (3)          No electric charges
         ∇⋅H = 0          (4)          No magnetic charges
         ε0 = 8.85 10-12 F/m, µ0 = 1.26 10-6 Tm/A
                              The Wave Equation:
                   1 ∂ 2u                               c0 =
                                                                    1
                                                                               = 3 × 108 m / s
              ∇ u− 2 2 =0
                2
                                           Where:
                  c0 ∂t                                        (ε 0 µ 0 )
                                                                        1/ 2
 • EM waves are transverse waves (like string waves).
                                                                     Unit vector in propagation direction
                    Polarization
                    information
• For isotropic materials we can ignore the polarization and use
scalar wave theory:
                        What is different in the medium?
                        (Microscopic picture of polarization)
Simplistic model of an atom in an electric field:
                                                          +
                                                                  x       p=qx, x~E
                +                                          -
                                E
                -                               p =αE            α - atomic polarizability
For a collection of atoms:
                                =
                                                               “The dipole             # atoms/vol.
                                                               moment per unit
                                                               volume”
    So, P~E
                                           Electric permittivity of   Electric susceptibility
                                           free space                 of the material
              Continuing macroscopic discussion…
  D = ε0 E + P                In free space, P=M=0, so that D=ε0E
                              and B=µ0H, and (1-4) recovers
  B = µ0 H + µ0 M
D – electric displacement     Intensity and Power
P – polarization density      Poynting vector: S = E × H
B – magnetic flux density     represents the flow of EM power.
M – magnetization density     The optical intensity (power flow
                              across a unit area): I = <S>
            ∂D
   ∇× H =                     Boundary Conditions
            ∂t                At the boundary between two dielectric
                              media and in the absence of free charges
              ∂B
   ∇× E = −                   and currents:
              ∂t              • Tangential components of E and H
                              • Normal components of D and B
    ∇⋅D = 0                   Must be continuous
                                 E                         D             B
    ∇⋅B = 0                                     H
    Dielectric Media
E(r, t)            Medium                 P(r, t)
Input                                    Output
Linear:
P(r, t) is linearly related to E(r, t)
Nondispersive:
P(r, t) is determined by E(r, t) at the same time ‘t’, instantaneous response
Homogeneous:
Relation between P(r, t) and E(r, t) is independent of r.
Isotropic:
Relation between P(r, t) and E(r, t) is independent of the direction of E.
Spatially nondispersive:
Relation between P(r, t) and E(r, t) is local.
    Lecture 3: Complex Index, K-vector and ε
     Linear, Nondispersive, Homogeneous, and Isotropic Media
P = ε0χE, χ - electric
susceptibility                  Since D and E are parallel:
E                         P     D = ε E, where ε = ε0(1 + χ)= ε0 εr - electric
             χ                  permittivity of the medium,
Under these conditions:         εr = ε/ε0 = (1 + χ) – relative dielectr. constant
                 ∂E             By analogy with the free space case:
     ∇× H = ε
                 ∂t
                                   1 ∂ 2u                      c0 =
                                                                           1
                                                                                      = 3 × 108 m / s
                 ∂H           ∇ u− 2 2 =0
                                 2
    ∇ × E = − µ0                  v ∂t                                (ε 0 µ 0 )
                                                                               1/ 2
                  ∂t
                               Where v = c/n – speed of light in a Medium
      ∇⋅E = 0
                                        1/ 2
                                   ⎛ε ⎞
                              n = ⎜⎜ ⎟⎟        = ε r1/ 2 = (1 + χ )1/ 2    - Refractive Index
      ∇⋅H = 0                      ⎝ ε0 ⎠
Magnetic phenomena were neglected
B = µ0H + µ0M, M = χmH
B = µH, where µ = µ0(1+χm), χm - magnetic susceptibility
Magnitization can be classified as:
•Diagmagnetic (due to interaction of external
Field with orbital motion of electrons, causes B to decrease)
•Paramagnetism (due to interactions of spin of unpaired
electrons with field, causes B to increase
•Ferromagnitism: Material with a large internal
magnetization (e.g. Iron, cobalt, nickel)
Will not be dealing with ferromagnetic material in this class. For
most materials, paramagnetic and diagmetic affects lead to:
 χm~ 10-8 – 10-5, hence µr ≅ 1, µ ≅ µ0
            Complex Refractive Index and Conductivity
The origin of imaginary part can be traced down to the conductivity of material.
In a conductor: j = σE.
Real current is included in a full Ampere-Maxwell law:
                  ∂D
     ∇× H = j +         By substituting j and eliminating D, B, and H we have:
                  ∂t
          ∂E 1 ∂2 E
∇ E − σµ0
 2
            − 2 2 =0              Substituting   E ( z , t ) = E 0 ei ( kz −ωt )   gives:
          ∂t v ∂t
k2 = iσµ0ω + (ω/v)2           On the other hand: k = nω/c. If k-complex, why
                              don’t we introduce complex n?
n2 = iσ/(ε0ω) + εr
    Behavior at a boundary: Reflection and Transmission
Boundary Conditions:
  E xi + E xr = E xt   (1)   i,r,t – incident, reflected and transmitted beams.
                             The sign “-” for reflected H component is due to
  H yi − H yr = H yt   (2)   opposite directions of Si = E × H and Sr.
Taking into account the relationship between the magnitudes of E and H vectors:
   H yi = cε 0 n1 E xi               H yt = cε 0 n2 E xt         H yr = cε 0 n1 E xr
   Assuming n1 = 1, and n2 = n we can represent (2):
              E xi − E xr = n~E xt                         (3)
    By soliving (1) and (3) together we obtain:
        E xr n~ − 1
             =~                 That can be rearranged to obtain the result:
        Ex n + 1
           i
                      2
              E   r         ~
                            n −1
                                 2
       R=         x
                          = ~
              E   i
                  x         n +1
       Complex Refractive Index and Dielectric Constant
                           K - extinction coefficient. Since n=√εr and
     n~ = n + iK           n – complex we can introduce
                           εr = ε1 + i ε2
The link between ε1, iε2 from one side and n, K from another side:
                                                                   1 1
                                          1
   ε1 = n 2 − K 2                      n=    (ε 1 + (ε 12 + ε 22 ) 2 ) 2
                                           2
                                                                   1 1
                                         1
    ε 2 = 2nK                         K=    (−ε 1 + (ε 12 + ε 22 ) 2 ) 2
                                          2
               Lecture 4: Crystal Structure
               Features of Optical Physics in Solid State
       Free Atoms            Gases, Liquids, Glasses               Solids
   Atomic or Molecular      No translational symmetry     Translational symmetry
         Physics                 Weak interaction           Stronger interaction
  Spherically symmetric            High density
Aspects of the solid particularly relevant to the optical properties:
• crystal symmetry
• electronic bands (conservation of E and k-vector will dictate allowed transitions).
• Vibronic bands, phonons. Small energy, play a critical role in scattering and in k-
vector conservation.
• The density of states (directly related to the absorption coefficient).
• Delocalized states and collective states: excitons, plasmon, polaritons.
                                 Crystal Symmetry
Lifting of degeneracies by reduction of the symmetry.
Optical anisotropy (Neumann’s Principle):
Macroscopic physical properties must have at least the symmetry of the crystal structure
                            Bravais Lattice
Bravais Lattice, Unit Cell and Basis
A 3-D Bravais lattice consists of all points with position vectors R of the form:
R = n1a1 + n2a2 + n3a3
    Coordination #: Number of nearest neighbors
    e.g. for S.C. structure, c# is 6
        What defines a legitimate pair?
                                          2-D Examples:
                        The parallelogram (primitive unit cell) defined
                        by the pair must enclose only 1 lattice site…
Homeycomb lattice
Not a Bravais Lattice
 Need to define this as a lattice with a basis
                 Body-Centered Cubic (BCC) Lattice
BCC Lattice: e.g. Fe, Cr, Cs, …
Is it Bravais Lattice?
What is the coordination number?
               Face-Centered Cubic (FCC) Lattice
FCC Lattice: e.g. Au, Ag, Al, Cu…
                                              R = a2 + a3
Is it Bravais Lattice?
What is the coordination number?              L = a1 + a2 + a3
                                              Q = 2a2
                                   Primitive Unit Cell
   A volume that, when translated in a Bravais lattice, fills all of space without
   overlapping itself or leaving voids.
A primitive cell must contain precisely one lattice point: nv = 1 where n – density of
points, v – volume of the primitive cell.
                       Primitive Unit Cell (Continued)
        Obvious primitive cell:
        r = x1a1 + x2a2+ x3a3, where 0 < xi < 1
Conventional unit cell – large cube
Primitive cell – figure with six parallelogram faces, ¼ v and less symmetry
     Disadvantage: doesn't display the full symmetry of the Bravais lattices.
                          Wigner-Seitz Primitive Cell
  Region around a lattice point such that the area
  enclosed is closest the enclosed point than to
  any other lattice point.
The surrounding cube in not the conventional FCC cell, but a shifted one
 Not all periodic structures are equivalent to a Bravais Lattice with a
                           single-point basis
   Honeycomb lattice in 2-D:
                                         Can be considered as a 2-D triangular
                                         Bravais lattice with a two-point basis
   Diamond structure in 3-D:                 Hexagonal Close-Packed (HCP):
Can be regarded as a FCC lattice with          Can be regarded as a hexagonal
the two-point basis 0 and (a/4)(x+y+z)         lattice with the two-point basis
                     Lecture 5: The Reciprocal Lattice
        This is an important concept:
        • Theory of crystal diffraction
        • Study of functions with the periodicity of Bravais lattice
        • Laws of momentum conservation in periodic structures
Definition:
Consider Bravais lattice with points represented by R(n1, n2, n3) and a plane wave, eikr.
For certain K the plane waves will have the periodicity of a given Bravais lattice:
        ei K ( r + R ) = ei K r       ei K R = 1    Should be held for all R’s
    Simplest example 1-D:
                                      The direct lattice: R = na, the reciprocal lattice: k = kb.
    •     •      •       •   •        Let us require ba = 2π, then kR = 2πk1n which means
                                  x
                                      that k1 = 0,1,2,…
                     a                Thus the reciprocal lattice is a Bravais lattice where b
                                      can be taken as a primitive vector.
                             Reciprocal Lattice in a 3-D case
   Can be generated by the three primitive vectors:
               a2 × a3
    b1 = 2π
            a1 ⋅ (a 2 × a3 )               This leads to bi aj = 2πδij, where δij is
                                           the Kronecker delta symbol
                     a3 × a1               For any k = k1b1 + k2b2 + k3b3 and
    b2 = 2π
                 a1 ⋅ (a 2 × a3 )
                                           R=n1a1 + n2a2 + n3a3 we have:
                     a1 × a2               kR = 2π(k1n1 + k2n2 + k3n3)
    b3 = 2π
                 a1 ⋅ (a 2 × a3 )
Thus     e = 1 is satisfied by those k-vectors, and the reciprocal lattice as a
          iK R
Bravais lattice and bi – are primitive vectors.
                                 Important Examples
       Direct Lattice                          Corresponding Reciprocal
       Simple Cubic (SC):                      SC with b1 = (2π/a)x, …
       a1=ax, a2=ay, a3=az
       FCC with a cubic cell of side a         BCC with a cubic cell of side 4π/a
       BCC with a cubic cell of side a         FCC with a cubic cell of 4π/a
       Simple Hexagonal (SH) with              SH with 2π/c and 4π/(√3a)
       lattice constants a and c
 • The reciprocal of reciprocal lattice is nothing but the original direct lattice.
 • If v is the volume of a primitive cell in the direct lattice, then the primitive cell of the
 reciprocal lattice has volume (2π)3/v
 • The Wigner-Seitz primitive cell of the reciprocal lattice is known as the first Brillouin
 zone.
The first Brillouin zone                                              The first Brillouin zone
for the BCC lattice                                                   for the FCC lattice
                         Lattice Planes and their Miller Indices
          d                d’
                                                  • For any family of lattice planes
                                                  separated by d there are perpendicular
                                                  lattice vectors, with the shortest of
                                                  which have a length of 2π/d.
• The Miller indices of a lattice plane (h, k, l) are the coordinates of the shortest
reciprocal lattice vector normal to that plane
• Miller indices depend on the particular choice of primitive vectors. Plane with indices h,
k, l, is normal to the reciprocal lattice vector hb1 + kb2 + lb3.
• FCC and BCC Bravais lattices are described in terms of a conventional cubic cell, SC
with bases. In crystallography to determine the orientation of lattice planes in real space:
How to find Miller indices from the real space analysis?
h : k : l = (1/x1) : (1/x2) : (1/x3), where xi- intercepts of the plane along the crystal axes.
recipr.         direct
• Directions in a direct lattice can be specified by [n1 n2 n3] indices (not to be confused
with Miller indices): n1a1 + n2a2 + n3a3
 Crystallography of Photonic Crystals – Opals
                                         SEM of polished surface
      3-D FCC        K-space
Size of the spheres 0.2-0.5 micron ~ λ
                         Structural
Sedimentation            collapse
                          T=516K
                          P=6.4MPa
     Triangular packing for (111) planes – L point
                                     Conventional cubic cell:
                                     [001]     (111)
                                                           [010]
                                 [100]
• Represented ~10% of the total surface area of the samples
        Square Packing for (100) planes – X point
            SEM                       [001]      (100)
                                                         [010]
                                   [100]
• Represented at ~70% of the total surface area of the samples
         Rectangular packing for (110) – K point
              SEM
                                        [001]      (110)
                                                           [010]
                                    [100]
• Represented at ~20% of the total surface area of the samples
Lecture 6: Determination of Crystal Structures by
           X-ray or Optical Diffraction
        Formulation of Bragg and von Laue
        Ewald’s Construction
        Experimental methods: Laue, Rotating Crystal, Powder
        Geometrical Structure Factor and Atomic Form Factor
        Fascinating Example of Photonic Crystals
                                 Bragg Formulation
Assumption: diffraction is produced by specular reflections produced by lattice planes.
X-rays: Atomic Lattices                               Visible: Photonic Crystals
                              Differently defined θ
                                                             θ
                                  Different n
                                                                      n
                     n≈1                     n = 1.5-3.5
  Bragg Formula                                       Bragg Formula
  mλ = 2d sinθ, m=1, 2,…                              mλ = 2nd cosθ, m=1, 2,…
  Wavelength                                          Wavelength
  Longest for m = 1, θ = 900                          Longest for m = 1, θ = 00
  λ = 2d, d ~ 1Å = 10-8 cm ⇒ λ                        λ = 2nd, d ~ 0.1-1 µm ⇒ λ
  ~ 10-8 cm                                           ~ 0.3-3 µm
  or E = hν = hc/λ ~ 103-104 eV                       or E = hν = hc/λ ~ 1 eV
  Linewidth                                           Linewidth
  ∆ν/ν ~ ∆n/n                                         ∆ν/ν ~ ∆n/n
  ∆n/n ~ 10-5 ⇒ ∆ν/ν ~ 10-5                           ∆n/n ~ 0.1-3.5 ⇒ ∆ν/ν ~ 1
                                           More on Linewidths in Opals (FCC)
                                                                                                      Thickness dependency
                       ∆ν =(2/π)ν∆n/n – in 1-D case                                                 1.0
                                                                                                           Reflection Spectra for fixed refractive index (Toluene n=1.5)
                       In 3-D FCC opal structure:
                                                                                 Intensity (A.u.)
                                                                                                    0.8
                                                                                                                                                       d= 0.70µm
                                                                                                                                                       d= 1.40µm
                                                                                                    0.6                                                d= 2.79µm
                                                                                                                                                       d= 5.58µm
                                                                                                                                                       d= 11.17µm
                                                                                                    0.4                                                d= 22.34µm
                      10            Index Matching                                                                                                     d= 44.68µm
                                                                                                    0.2
                      9
                                                                                                    0.0
                      8                                                                               60         62        64        66        68        70
FWHM Linewidth (nm)
                                                                                                      0          0        Wavelength
                                                                                                                          0        0 (nm)      0         0
                      7
                                                                             Experiment: V.N. Astratov et al., Nuovo Cimento17,
                      6                                                      1349 (1995)
                      5
                                                         Thickness (um)
                      4                                        22
                                                               45
                      3                                        89
                      2                                        179
                                                               357
                      1                                        715
                      0
                      1.20   1.25   1.30   1.35      1.40     1.45    1.50
                                      Refractive Index
Real Space Measurements can be Related to Directions in k-Space
                               Photonic Band Structure
              FCC
                              A.Blanko et al., Nature 405, 437 (2000)
Complete Photonic Band Gap and Control of Spontaneous Emission
     Pioneering Idea of Eli Yablonovitch, PRL58, 2059 (1987)
Complete photonic band gap is an overlap of partial stop bands for ALL
directions in space
Stop band frequency: ω = (c/nav)k,                [001]     (111)
where khkl = 2π / dhkl,
FCC lattice spacings dhkl are given:
d100= a/2, d111 = a/√3 ⇒
k100= 4π/a, k111= 2π √3 /a ⇒
ν100= (c/ 2π nav)k100 =2c/(anav)          a
ν111= (c/ 2π nav)k111 = √3c/(anav)
                                                                        [010]
(ν100 - ν111)/ ν100 = 1 – (√3)/2
                                              [100]
∆ν/ν =(2/π) ∆n/n – in 1-D case
                                                Spheres at the centers of the
∆n/n = 0.21 – Historical Interest               faces are removed for clarity
                 Von Laue Formulation of X-ray Diffraction
 No assumption of specular reflection by planes, but reradiation the incident
 radiation by individual atoms in all directions. Sharp peaks appear as a result of
 constructive interference.
                                                    Path difference:
                                                  dcosθ + dcosθ’ = d (n - n’)
                                                  Constructive interference:
                                                   d (n - n’) = m λ, m = 0,1,2,…
                                                  Multiplying by 2π/λ:
                                                  d (k - k’) = 2πm
                                                  For a Brave lattice:
                                                  R (k - k’) = 2πm
Laue condition: constructive interference occurs provided that the change in k-vector,
K = k - k’, is a vector of the reciprocal lattice
          Equivalence of the Bragg and Von Laue Formulations
                                                    It can be shown:
                                                    kK = (1/2)K, where K –
                                                    magnitude of the vector of the
                                                    reciprocal lattice
Equivalence of the von Laue and Bragg approaches means that the k-space lattice
plane associated with a diffraction peak in the Laue formulation is parallel to the
family of direct lattice planes responsible for peak in the Bragg formulation.
                             Ewald Construction
Given the incident k, a sphere of radius k is drawn about the point k. Diffraction
peaks corresponding to reciprocal lattice vectors K will be observed only if the
sphere intersects lattice points different from point O.
Need to vary parameters (λ, direction of propagation) to observe diffraction.
                            The Laue Method
By varying k from k0 to k1 we can expand Ewald sphere to fill the shaded
region. Bragg peaks will be observed corresponding to all reciprocal lattice
points in the shaded region.
                       The Rotating-Crystal Method
Evald sphere determined by the incident k-vector is fixed in k-space, while the
entire reciprocal lattice rotates about the axis of rotation of the crystal. The
Bragg reflection occur whenever these circles intersect the Ewald sphere.
Similarly we can introduce The Rotating-Crystal Method.
Topics for reading: Geometrical Structure Factor and Atomic Form Factor