Waves in composites and metamaterials/Bloch waves and the quasistatic limit

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[edit] Bloch Theorem

In the previous lecture we showed that Maxwell's equations at fixed frequency can be formulated in terms of the fields \mathbf{D} and \mathbf{B} as [1]

 \text{(1)} \qquad 
  \boldsymbol{\nabla} \cdot \mathbf{D} = 0 ~;~~ \boldsymbol{\nabla} \cdot \mathbf{B} = 0 ~;~~
  i~\boldsymbol{\nabla} \times \left(\cfrac{\mathbf{D}}{\epsilon}\right) = \omega~\mathbf{B} ~;~~
  -i~\boldsymbol{\nabla} \times \left(\cfrac{\mathbf{B}}{\mu}\right) = \omega~\mathbf{D} ~.

Equations (1) suggest that we should look for solutions \mathbf{D} and \mathbf{B} in the space of divergence-free fields such that

 \text{(2)} \qquad 
  \mathcal{L}\begin{bmatrix} \mathbf{D} \\ \mathbf{B} \end{bmatrix} = 
  \omega~\begin{bmatrix} \mathbf{D} \\ \mathbf{B} \end{bmatrix}
  \qquad \text{or} \qquad
   {
   (\mathcal{L} - \omega~\boldsymbol{1})\begin{bmatrix}\mathbf{D} \\ \mathbf{B} \end{bmatrix} = 
   \boldsymbol{0} 
   }

where the operator \mathcal{L} is given by

 \text{(3)} \qquad 
  {
  \mathcal{L} := \begin{bmatrix}
       0 & -i~\boldsymbol{\nabla} \times \mu^{-1} \\
       i~\boldsymbol{\nabla} \times \epsilon^{-1} & 0 
       \end{bmatrix} ~.
  }

If the medium is such that the permittivity \epsilon(\mathbf{x}) and the permeability \mu(\mathbf{x}) are periodic, i.e.,


   \epsilon(\mathbf{x}) = \epsilon(\mathbf{x} + \mathbf{R}) ~;~~
   \mu(\mathbf{x}) = \mu(\mathbf{x} + \mathbf{R})

where \mathbf{R} is a lattice vector (see Figure 1) then the operator \mathcal{L} has the same periodicity as the medium.

Figure 1. Lattice vector in a periodic medium.

Also recall the translation operator \mathcal{T}_R defined as


  {
  \mathcal{T}_R\begin{bmatrix} \mathbf{D}(\mathbf{x}) \\ \mathbf{B}(\mathbf{x}) \end{bmatrix} = 
  \begin{bmatrix} \mathbf{D}(\mathbf{x}+\mathbf{R}) \\ \mathbf{B}(\mathbf{x}+\mathbf{R}) \end{bmatrix} ~.
  }

Periodicity of the medium implies that \mathcal{T}_R commutes with \mathcal{L}, i.e.,


  {
  \mathcal{T}_R~\mathcal{L} = \mathcal{L}~\mathcal{T}_R ~.
  }

[2] The translation operator is unitary, i.e.,


  {
  \mathcal{T}_R~\mathcal{T}_R^T = \mathcal{T}_R~\mathcal{T}_{-R} = \boldsymbol{1} ~.
  }

This means that the adjoint operator \mathcal{T}_R^T is equal to the inverse operator \mathcal{T}_{-R}.

The translation operator also commutes, i.e.,


  {
  \mathcal{T}_R~\mathcal{T}_{R'} = \mathcal{T}_{R'}~\mathcal{T}_R = \mathcal{T}_{R+R'} ~.
  }

[3] Also, since \mathcal{L} and \mathcal{T}_R commute, the operators \mathcal{L}-\omega\boldsymbol{1} and \mathcal{T}_R must also commute. This implies that


  \mathcal{T}_R~(\mathcal{L} - \omega~\boldsymbol{1})
    ~\begin{bmatrix}\mathbf{D}(\mathbf{x}) \\ \mathbf{B}(\mathbf{x})\end{bmatrix} = \boldsymbol{0}
  = (\mathcal{L} - \omega~\boldsymbol{1})~\mathcal{T}_R
    ~\begin{bmatrix}\mathbf{D}(\mathbf{x}) \\ \mathbf{B}(\mathbf{x})\end{bmatrix}
  = (\mathcal{L} - \omega~\boldsymbol{1})~
    ~\begin{bmatrix}\mathbf{D}(\mathbf{x}+\mathbf{R}) \\ \mathbf{B}(\mathbf{x}+\mathbf{R})\end{bmatrix} ~.

Hence the eigenstates of \mathcal{L} - \omega~\boldsymbol{1} and the eigenstates of \mathcal{T}_R lie in the same space. Therefore, any solution can be expressed in fields which are simultaneously eigenstates of all the \mathcal{T}_R, i.e., these eigenstates have the property

 \text{(4)} \qquad 
  {
  [\mathcal{T}_R - c(\mathbf{R})~\boldsymbol{1}]\begin{bmatrix} \mathbf{D}(\mathbf{x}) \\ \mathbf{B}(\mathbf{x}) 
    \end{bmatrix} = \boldsymbol{0} ~.
  }

Since \mathcal{T}_R~\mathcal{T}_{R'} = \mathcal{T}_{R+R'}, we have


  c(\mathbf{R})~c(\mathbf{R}') = c(\mathbf{R} + \mathbf{R}') ~.

So it suffices to know c(\mathbf{R}) when \mathbf{R} = \mathbf{a}_1, \mathbf{a}_2 , \mathbf{a}_3 where the \mathbf{a}_i's are the primitive vectors of the lattice, i.e.,


  \epsilon(\mathbf{x} + \mathbf{a}_j) = \epsilon(\mathbf{x}) ~;~~
  \mu(\mathbf{x} + \mathbf{a}_j) = \mu(\mathbf{x}) ~.

Let us assume that


  c(\mathbf{a}_j) = e^{2\pi~i~\alpha_j} \qquad j = 1, 2, 3

for a suitable choice of αj.

Then for any lattice vector


  \mathbf{R} = n_1~\mathbf{a}_1 + n_2~\mathbf{a}_2 + n_3~\mathbf{a}_3

we have


  \begin{align}
  c(\mathbf{R}) & = c(n_1~\mathbf{a}_1 + n_2~\mathbf{a}_2 + n_3~\mathbf{a}_3)
   = c(n_1~\mathbf{a}_1)~c(n_2~\mathbf{a}_2)~c(n_3~\mathbf{a}_3) \\
   & = c\left(\sum_{i=1}^{n_1}\mathbf{a}_1\right)~
     c\left(\sum_{i=1}^{n_2}\mathbf{a}_2\right)~c\left(\sum_{i=1}^{n_3}\mathbf{a}_3\right)
   = [c(\mathbf{a}_1)]^{n_1}~[c(\mathbf{a}_2)]^{n_2}~[c(\mathbf{a}_3)]^{n_3} \\
   & = e^{2\pi i \alpha_1~n_1}~e^{2\pi i \alpha_2~n_2}~e^{2\pi i \alpha_3~n_3}
     = e^{2\pi i (\alpha_1~n_1 + \alpha_2~n_2 + \alpha_3~n_3)} 
  \end{align}

or,


  c(\mathbf{R}) = e^{2\pi i (\alpha_1~n_1 + \alpha_2~n_2 + \alpha_3~n_3)} ~.

Define a vector


  \mathbf{k} := \alpha_1~\mathbf{b}_1 + \alpha_2~\mathbf{b}_2 + \alpha_3~\mathbf{b}_3

where the vectors \mathbf{b}_i are the reciprocal lattice vectors satisfying


  \mathbf{b}_i\cdot\mathbf{a}_j = 2\pi~\delta_{ij} ~.

Then,


  \mathbf{k}\cdot\mathbf{R} = 
    (\alpha_1~\mathbf{b}_1 + \alpha_2~\mathbf{b}_2 + \alpha_3~\mathbf{b}_3) \cdot
    (n_1~\mathbf{a}_1 + n_2~\mathbf{a}_2 + n_3~\mathbf{a}_3)
    = \alpha_1~n_1~2~\pi + \alpha_2~n_2~2~\pi + \alpha_3~n_3~2~\pi

or,


  \mathbf{k}\cdot\mathbf{R} 
    = 2\pi (\alpha_1~n_1 + \alpha_2~n_2 + \alpha_3~n_3) ~.

Therefore, we have


  c(\mathbf{R}) = e^{i \mathbf{k}\cdot\mathbf{R}} ~.

Plugging this expression into (4), we get


  [\mathcal{T}_R - e^{i \mathbf{k}\cdot\mathbf{R}}~\boldsymbol{1}]
  \begin{bmatrix} \mathbf{D}(\mathbf{x}) \\ \mathbf{B}(\mathbf{x}) \end{bmatrix} 
  = \boldsymbol{0}

or,

 \text{(5)} \qquad 
  {
  \begin{bmatrix} \mathbf{D}(\mathbf{x}+\mathbf{R}) \\ \mathbf{B}(\mathbf{x}+\mathbf{R}) \end{bmatrix}  = 
  e^{i \mathbf{k}\cdot\mathbf{R}}~
  \begin{bmatrix} \mathbf{D}(\mathbf{x}) \\ \mathbf{B}(\mathbf{x}) \end{bmatrix} ~.
  }

Equation (5) is called the Bloch condition.

In summary, the solutions to the electromagnetic equations in a periodic medium can be expressed in Bloch waves where each Bloch wave is a time harmonic solution to the electromagnetic equations which in addition satisfies the Bloch condition for all lattice vectors \mathbf{R} and for some appropriate choice of \mathbf{k}.

Note that for any vector \mathbf{x}, the Bloch condition implies that


  e^{-i \mathbf{k}\cdot(\mathbf{x}+\mathbf{R})}
  \begin{bmatrix} \mathbf{D}(\mathbf{x}+\mathbf{R}) \\ \mathbf{B}(\mathbf{x}+\mathbf{R}) \end{bmatrix}  = 
  e^{i \mathbf{k}\cdot\mathbf{R} - i \mathbf{k} \cdot\mathbf{R} - i \mathbf{k} \cdot \mathbf{x}}~
  \begin{bmatrix} \mathbf{D}(\mathbf{x}) \\ \mathbf{B}(\mathbf{x}) \end{bmatrix} =
  e^{- i \mathbf{k} \cdot \mathbf{x}}~
  \begin{bmatrix} \mathbf{D}(\mathbf{x}) \\ \mathbf{B}(\mathbf{x}) \end{bmatrix} ~.

Therefore the quantity


  e^{- i \mathbf{k} \cdot \mathbf{x}}~
  \begin{bmatrix} \mathbf{D}(\mathbf{x}) \\ \mathbf{B}(\mathbf{x}) \end{bmatrix}

is periodic.

[edit] Quasistatic Limit

Let us now consider the solution of Maxwell's equation in periodic media in the quasistatic limit. [4] Consider the periodic medium shown in Figure 2. The lattice spacing is η.

Figure 2. Periodic medium with x and y spaces.

Define


  \epsilon_\eta(\mathbf{x}) := \epsilon\left(\cfrac{\mathbf{x}}{\eta}\right) 
    = \epsilon(\mathbf{y})~;~~
  \mu_\eta(\mathbf{x}) := \mu\left(\cfrac{\mathbf{x}}{\eta}\right)
    = \mu(\mathbf{y}) ~.

These are periodic functions, i.e.,


  \epsilon(\mathbf{y} + \mathbf{a}_i) = \epsilon(\mathbf{y}) ~;~~
  \mu(\mathbf{y} + \mathbf{a}_i) = \mu(\mathbf{y})

where \mathbf{a}_i are the primitive lattice vectors. We may also write these periodicity conditions as


  \epsilon_\eta(\mathbf{x} + \eta\mathbf{a}_i) = \epsilon_\eta(\mathbf{x}) ~;~~
  \mu_\eta(\mathbf{x} + \eta\mathbf{a}_i) = \mu_\eta(\mathbf{x}) ~.

Similarly, define


  \mathbf{D}_\eta(\mathbf{x}) := \mathbf{D}(\mathbf{y}) ~;~~
  \mathbf{B}_\eta(\mathbf{x}) := \mathbf{B}(\mathbf{y}) ~;~~
  \mathbf{E}_\eta(\mathbf{x}) := \mathbf{E}(\mathbf{y}) ~;~~
  \mathbf{H}_\eta(\mathbf{x}) := \mathbf{H}(\mathbf{y}) ~.

Then Maxwell's equations can be written as

 \text{(6)} \qquad 
  \boldsymbol{\nabla} \cdot \mathbf{D}_\eta = 0 ~;~~
  \boldsymbol{\nabla} \cdot \mathbf{B}_\eta = 0 ~;~~
  \boldsymbol{\nabla} \times \mathbf{E}_\eta - i\omega~\mathbf{B}_\eta = \boldsymbol{0} ~;~~
  \boldsymbol{\nabla} \times \mathbf{H}_\eta + i\omega~\mathbf{D}_\eta = \boldsymbol{0} ~.

Let us look for Bloch wave solutions of the form


  \mathbf{E}_\eta(\mathbf{x}) = e^{i\mathbf{k}\cdot\mathbf{x}}~\mathbf{e}_\eta(\mathbf{x}) ~;~~
  \mathbf{D}_\eta(\mathbf{x}) = e^{i\mathbf{k}\cdot\mathbf{x}}~\mathbf{d}_\eta(\mathbf{x}) ~;~~
  \mathbf{H}_\eta(\mathbf{x}) = e^{i\mathbf{k}\cdot\mathbf{x}}~\mathbf{h}_\eta(\mathbf{x}) ~;~~
  \mathbf{B}_\eta(\mathbf{x}) = e^{i\mathbf{k}\cdot\mathbf{x}}~\mathbf{b}_\eta(\mathbf{x})

where \mathbf{e}_\eta, \mathbf{d}_\eta, \mathbf{h}_\eta, \mathbf{b}_\eta have the same periodicity as ε and μ, i.e.,


  \mathbf{e}_\eta(\mathbf{x} + \eta~\mathbf{a}_i) = \mathbf{e}(\mathbf{x}) ~;~~
  \mathbf{d}_\eta(\mathbf{x} + \eta~\mathbf{a}_i) = \mathbf{d}(\mathbf{x}) ~;~~
  \mathbf{h}_\eta(\mathbf{x} + \eta~\mathbf{a}_i) = \mathbf{h}(\mathbf{x}) ~;~~
  \mathbf{b}_\eta(\mathbf{x} + \eta~\mathbf{a}_i) = \mathbf{b}(\mathbf{x}) ~.

From the constitutive relations, we get


  \mathbf{d}_\eta(\mathbf{x}) = \epsilon_\eta(\mathbf{x})~\mathbf{e}_\eta(\mathbf{x}) ~;~~
  \mathbf{b}_\eta(\mathbf{x}) = \mu_\eta(\mathbf{x})~\mathbf{h}_\eta(\mathbf{x}) ~.

Recall that, for periodic media, Maxwell's equations may be expressed as


  (\mathcal{L} - \omega~\boldsymbol{1})\begin{bmatrix}\mathbf{D} \\ \mathbf{B} \end{bmatrix} = 
   \boldsymbol{0} ~.

Here ω is an eigenvalue of \mathcal{L}. However, \mathcal{L} depends on ω via ε(ω) and μ(ω). {\bf Bloch wave solutions do not exists unless ω takes one of a discrete set of values.}

Let these discrete values be


  \omega = \omega_\eta^j(\mathbf{k})

where the superscript j labels the solution branches.

Let us see what the Bloch wave solutions reduce to as \eta\rightarrow 0. Following standard multiple scale analysis, let us assume that the periodic complex fields have the expansions

 \text{(7)} \qquad 
  \begin{align} 
    \mathbf{e}_\eta(\mathbf{x}) & = \mathbf{e}_0(\mathbf{y}) + \eta~\mathbf{a}_1(\mathbf{y}) + \eta^2~\mathbf{a}_2(\mathbf{y}) +
      \dots \\
    \mathbf{d}_\eta(\mathbf{x}) & = \mathbf{d}_0(\mathbf{y}) + \eta~\mathbf{d}_1(\mathbf{y}) + \eta^2~\mathbf{d}_2(\mathbf{y}) +
      \dots \\
    \mathbf{h}_\eta(\mathbf{x}) & = \mathbf{h}_0(\mathbf{y}) + \eta~\mathbf{h}_1(\mathbf{y}) + \eta^2~\mathbf{h}_2(\mathbf{y}) +
      \dots \\
    \mathbf{b}_\eta(\mathbf{x}) & = \mathbf{b}_0(\mathbf{y}) + \eta~\mathbf{b}_1(\mathbf{y}) + \eta^2~\mathbf{b}_2(\mathbf{y}) +
      \dots
  \end{align}

Let us also assume that the dependence of ω on η and \mathbf{k} has an expansion of the form

 \text{(8)} \qquad 
  \omega = \omega_\eta^j(\mathbf{k}) 
     = \omega_0^j(\mathbf{y}) + \eta~\omega_1^j(\mathbf{y}) + \eta^2~\omega_2^j(\mathbf{y}) +
      \dots

Plugging (8) and (7) into (6) gives

 \text{(9)} \qquad 
  \begin{align}
    \boldsymbol{\nabla} \cdot \left(e^{i\eta~\mathbf{k}\cdot\mathbf{y}}~[\mathbf{d}_0(\mathbf{y}) + \eta~\mathbf{d}_1(\mathbf{y}) + \dots]
         \right) & = 0 \\
    \boldsymbol{\nabla} \cdot \left(e^{i\eta~\mathbf{k}\cdot\mathbf{y}}~[\mathbf{b}_0(\mathbf{y}) + \eta~\mathbf{b}_1(\mathbf{y}) + \dots]
         \right) & = 0 \\
    \boldsymbol{\nabla} \times \left(e^{i\eta~\mathbf{k}\cdot\mathbf{y}}~[\mathbf{e}_0(\mathbf{y}) + \eta~\mathbf{e}_1(\mathbf{y}) + \dots]
          \right)
     - i [\omega_0^j + \eta~\omega_1^j + \dots]
         [\mathbf{b}_0(\mathbf{y}) + \eta~\mathbf{b}_1(\mathbf{y}) + \dots] & = \boldsymbol{0} \\
    \boldsymbol{\nabla} \times \left(e^{i\eta~\mathbf{k}\cdot\mathbf{y}}~[\mathbf{h}_0(\mathbf{y}) + \eta~\mathbf{h}_1(\mathbf{y}) + \dots]
          \right)
     + i [\omega_0^j + \eta~\omega_1^j + \dots]
         [\mathbf{d}_0(\mathbf{y}) + \eta~\mathbf{d}_1(\mathbf{y}) + \dots] & = \boldsymbol{0} ~.
  \end{align}

Define


  \boldsymbol{\nabla}_y := \left(\frac{\partial }{\partial y_1}, \frac{\partial }{\partial y_2}, \frac{\partial }{\partial y_3}\right)~.

Then, for a vector field \mathbf{v}(\mathbf{y}), using the chain rule we get

 \text{(10)} \qquad 
  \boldsymbol{\nabla} \cdot \mathbf{v}(\mathbf{y}) = \cfrac{1}{\eta}~\boldsymbol{\nabla}_y \cdot\mathbf{v}(\mathbf{y}) ~;~~ 
  \boldsymbol{\nabla} \times \mathbf{v}(\mathbf{y}) = \cfrac{1}{\eta}~\boldsymbol{\nabla}_y\times{\mathbf{v}(\mathbf{y})} ~.

Using definitions (10) in (9) and collecting terms of order 1 / η gives

 \text{(11)} \qquad 
  {
  \begin{align}
    \boldsymbol{\nabla}_y \cdot\mathbf{d}_0(\mathbf{y}) = 0 \\
    \boldsymbol{\nabla}_y \cdot\mathbf{b}_0(\mathbf{y}) = 0 \\
    \boldsymbol{\nabla}_y\times{\mathbf{e}_0(\mathbf{y})} = \boldsymbol{0} \\
    \boldsymbol{\nabla}_y\times{\mathbf{h}_0(\mathbf{y})} = \boldsymbol{0} 
  \end{align}
  }

These are the solutions in the quasistatic limit. Also, from the constitutive equations


  \mathbf{d}_0(\mathbf{y}) = \epsilon(\mathbf{y})~\mathbf{e}_0(\mathbf{y}) ~;~~
  \mathbf{b}_0(\mathbf{y}) = \mu(\mathbf{y})~\mathbf{h}_0(\mathbf{y}) ~.

Similarly, collecting terms of order 1 from the expanded Maxwell's equations (9) we get

 \text{(12)} \qquad 
  {
  \begin{align}
    i~\mathbf{k}\cdot\mathbf{d}_0(\mathbf{y}) + \boldsymbol{\nabla}_y \cdot\mathbf{d}_1(\mathbf{y}) = 0 \\
    i~\mathbf{k}\cdot\mathbf{b}_0(\mathbf{y}) + \boldsymbol{\nabla}_y \cdot\mathbf{b}_1(\mathbf{y}) = 0 \\
    i~\mathbf{k}\times\mathbf{e}_0(\mathbf{y}) + \boldsymbol{\nabla}_y\times{\mathbf{e}_1(\mathbf{y})} - i~\omega_0^j~\mathbf{b}_0(\mathbf{y})
       = \boldsymbol{0} \\
    i~\mathbf{k}\times\mathbf{h}_0(\mathbf{y}) + \boldsymbol{\nabla}_y\times{\mathbf{h}_1(\mathbf{y})} + i~\omega_0^j~\mathbf{d}_0(\mathbf{y})
       = \boldsymbol{0} ~.
  \end{align}
  }

Since \mathbf{d}_1(\mathbf{y}), \mathbf{b}_1(\mathbf{y}), \mathbf{e}_1(\mathbf{y}), \mathbf{h}_1(\mathbf{y}) are periodic, this implies that

 \text{(13)} \qquad 
  {
  \begin{align}
    \langle \boldsymbol{\nabla}_y \cdot\mathbf{d}_1(\mathbf{y})\rangle = 0 \\
    \langle \boldsymbol{\nabla}_y \cdot\mathbf{b}_1(\mathbf{y})\rangle = 0 \\
    \langle \boldsymbol{\nabla}_y \times{\mathbf{e}_1(\mathbf{y})}\rangle = \boldsymbol{0} \\
    \langle \boldsymbol{\nabla}_y \times{\mathbf{h}_1(\mathbf{y})}\rangle = \boldsymbol{0} ~.
  \end{align}
  }

where \langle \bullet \rangle is the volume average over the unit cell. So a necessary condition that equations (12) have a solution is that

 \text{(14)} \qquad 
  {
  \begin{align}
    i~\mathbf{k}\cdot\langle \mathbf{d}_0(\mathbf{y}) \rangle = 0 \\
    i~\mathbf{k}\cdot\langle \mathbf{b}_0(\mathbf{y}) \rangle = 0 \\
    i~\mathbf{k}\times\langle \mathbf{e}_0(\mathbf{y}) \rangle - i~\omega_0^j~\langle \mathbf{b}_0(\mathbf{y}) \rangle
       = \boldsymbol{0} \\
    i~\mathbf{k}\times\langle \mathbf{h}_0(\mathbf{y}) \rangle + i~\omega_0^j~\langle \mathbf{d}_0(\mathbf{y}) \rangle
       = \boldsymbol{0} ~.
  \end{align}
  }

Note that the second pair of (14) implies the first pair.

[edit] Footnotes

  1. The following discussion is based on Ashcroft76 (p. 133-139).
  2. We can see that the two operators commute by working out the operations. Thus,
              
\mathcal{T}_R~\mathcal{L}~\begin{bmatrix}\mathbf{D} \\ \mathbf{B}\end{bmatrix} 
= \mathcal{T}_R~\begin{bmatrix} 
  -i~\boldsymbol{\nabla} \times [\mu^{-1}(\mathbf{x})~\mathbf{B}(\mathbf{x})] \\ 
  i~\boldsymbol{\nabla} \times [\epsilon^{-1}(\mathbf{x})~\mathbf{D}(\mathbf{x})]  
  \end{bmatrix} = \begin{bmatrix}          
  -i~\boldsymbol{\nabla} \times [\mu^{-1}(\mathbf{x}+\mathbf{R})~\mathbf{B}(\mathbf{x}+\mathbf{R})] \\             
  i~\boldsymbol{\nabla} \times [\epsilon^{-1}(\mathbf{x}+\mathbf{R})~\mathbf{D}(\mathbf{x}+\mathbf{R})]          
  \end{bmatrix}           
  = \mathcal{L}~\begin{bmatrix}\mathbf{D}(\mathbf{x}+\mathbf{R}) \\ 
     \mathbf{B}(\mathbf{x}+\mathbf{R})\end{bmatrix}          
  = \mathcal{L}~\mathcal{T}_R~\begin{bmatrix}\mathbf{D} \\ \mathbf{B}\end{bmatrix} ~.
  3. We can see that the translation operator commutes by working out the operations. Thus,
              
\mathcal{T}_R~\mathcal{T}_{R'}~
\begin{bmatrix} \mathbf{D}(\mathbf{x}) \\ \mathbf{B}(\mathbf{x}) \end{bmatrix}       
 = \mathcal{T}_R~
\begin{bmatrix}
\mathbf{D}(\mathbf{x}+\mathbf{R}') \\ 
\mathbf{B}(\mathbf{x}+\mathbf{R}')
\end{bmatrix}        
= \begin{bmatrix}
\mathbf{D}(\mathbf{x}+\mathbf{R}'+\mathbf{R}) \\ 
\mathbf{B}(\mathbf{x}+\mathbf{R}'+\mathbf{R})
\end{bmatrix}        
= \mathcal{T}_{R+R'}~
\begin{bmatrix}
\mathbf{D}(\mathbf{x}) \\ 
\mathbf{B}(\mathbf{x})
\end{bmatrix}        
= \mathcal{T}_{R'}~
\begin{bmatrix}
\mathbf{D}(\mathbf{x}+\mathbf{R}) \\ \mathbf{B}(\mathbf{x}+\mathbf{R})\end{bmatrix}       
 = \mathcal{T}_{R'}~\mathcal{T}_{R}~
\begin{bmatrix}\mathbf{D}(\mathbf{x}) \\ \mathbf{B}(\mathbf{x})\end{bmatrix}        ~.
  4. The following discussion is based on Milton02

[edit] References

  • N. W. Ashcroft and N. D. Mermin. Solid State Physics. Saunders, New York, 1976.
  • G. W. Milton. Theory of Composites. Cambridge University Press, New York, 2002.