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Bloch's theorem

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(Redirected from Bloch waves) Fundamental theorem in condensed matter physics This article is about a theorem in quantum mechanics. For the theorem used in complex analysis, see Bloch's theorem (complex variables).
Isosurface of the square modulus of a Bloch state in a silicon lattice
Solid line: A schematic of the real part of a typical Bloch state in one dimension. The dotted line is from the factor e. The light circles represent atoms.

In condensed matter physics, Bloch's theorem states that solutions to the Schrödinger equation in a periodic potential can be expressed as plane waves modulated by periodic functions. The theorem is named after the Swiss physicist Felix Bloch, who discovered the theorem in 1929. Mathematically, they are written

Bloch function

ψ ( r ) = e i k r u ( r ) {\displaystyle \psi (\mathbf {r} )=e^{i\mathbf {k} \cdot \mathbf {r} }u(\mathbf {r} )}

where r {\displaystyle \mathbf {r} } is position, ψ {\displaystyle \psi } is the wave function, u {\displaystyle u} is a periodic function with the same periodicity as the crystal, the wave vector k {\displaystyle \mathbf {k} } is the crystal momentum vector, e {\displaystyle e} is Euler's number, and i {\displaystyle i} is the imaginary unit.

Functions of this form are known as Bloch functions or Bloch states, and serve as a suitable basis for the wave functions or states of electrons in crystalline solids.

The description of electrons in terms of Bloch functions, termed Bloch electrons (or less often Bloch Waves), underlies the concept of electronic band structures.

These eigenstates are written with subscripts as ψ n k {\displaystyle \psi _{n\mathbf {k} }} , where n {\displaystyle n} is a discrete index, called the band index, which is present because there are many different wave functions with the same k {\displaystyle \mathbf {k} } (each has a different periodic component u {\displaystyle u} ). Within a band (i.e., for fixed n {\displaystyle n} ), ψ n k {\displaystyle \psi _{n\mathbf {k} }} varies continuously with k {\displaystyle \mathbf {k} } , as does its energy. Also, ψ n k {\displaystyle \psi _{n\mathbf {k} }} is unique only up to a constant reciprocal lattice vector K {\displaystyle \mathbf {K} } , or, ψ n k = ψ n ( k + K ) {\displaystyle \psi _{n\mathbf {k} }=\psi _{n(\mathbf {k+K} )}} . Therefore, the wave vector k {\displaystyle \mathbf {k} } can be restricted to the first Brillouin zone of the reciprocal lattice without loss of generality.

Applications and consequences

Applicability

The most common example of Bloch's theorem is describing electrons in a crystal, especially in characterizing the crystal's electronic properties, such as electronic band structure. However, a Bloch-wave description applies more generally to any wave-like phenomenon in a periodic medium. For example, a periodic dielectric structure in electromagnetism leads to photonic crystals, and a periodic acoustic medium leads to phononic crystals. It is generally treated in the various forms of the dynamical theory of diffraction.

Wave vector

A Bloch wave function (bottom) can be broken up into the product of a periodic function (top) and a plane-wave (center). The left side and right side represent the same Bloch state broken up in two different ways, involving the wave vector k1 (left) or k2 (right). The difference (k1k2) is a reciprocal lattice vector. In all plots, blue is real part and red is imaginary part.

Suppose an electron is in a Bloch state ψ ( r ) = e i k r u ( r ) , {\displaystyle \psi (\mathbf {r} )=e^{i\mathbf {k} \cdot \mathbf {r} }u(\mathbf {r} ),} where u is periodic with the same periodicity as the crystal lattice. The actual quantum state of the electron is entirely determined by ψ {\displaystyle \psi } , not k or u directly. This is important because k and u are not unique. Specifically, if ψ {\displaystyle \psi } can be written as above using k, it can also be written using (k + K), where K is any reciprocal lattice vector (see figure at right). Therefore, wave vectors that differ by a reciprocal lattice vector are equivalent, in the sense that they characterize the same set of Bloch states.

The first Brillouin zone is a restricted set of values of k with the property that no two of them are equivalent, yet every possible k is equivalent to one (and only one) vector in the first Brillouin zone. Therefore, if we restrict k to the first Brillouin zone, then every Bloch state has a unique k. Therefore, the first Brillouin zone is often used to depict all of the Bloch states without redundancy, for example in a band structure, and it is used for the same reason in many calculations.

When k is multiplied by the reduced Planck constant, it equals the electron's crystal momentum. Related to this, the group velocity of an electron can be calculated based on how the energy of a Bloch state varies with k; for more details see crystal momentum.

Detailed example

For a detailed example in which the consequences of Bloch's theorem are worked out in a specific situation, see the article Particle in a one-dimensional lattice (periodic potential).

Statement

Bloch's theorem — For electrons in a perfect crystal, there is a basis of wave functions with the following two properties:

  • each of these wave functions is an energy eigenstate,
  • each of these wave functions is a Bloch state, meaning that this wave function ψ {\displaystyle \psi } can be written in the form ψ ( r ) = e i k r u ( r ) , {\displaystyle \psi (\mathbf {r} )=e^{i\mathbf {k} \cdot \mathbf {r} }u(\mathbf {r} ),} where u(r) has the same periodicity as the atomic structure of the crystal, such that u k ( x ) = u k ( x + n a ) . {\displaystyle u_{\mathbf {k} }(\mathbf {x} )=u_{\mathbf {k} }(\mathbf {x} +\mathbf {n} \cdot \mathbf {a} ).}

A second and equivalent way to state the theorem is the following

Bloch's theorem — For any wave function that satisfies the Schrödinger equation and for a translation of a lattice vector a {\displaystyle \mathbf {a} } , there exists at least one vector k {\displaystyle \mathbf {k} } such that: ψ k ( x + a ) = e i k a ψ k ( x ) . {\displaystyle \psi _{\mathbf {k} }(\mathbf {x} +\mathbf {a} )=e^{i\mathbf {k} \cdot \mathbf {a} }\psi _{\mathbf {k} }(\mathbf {x} ).}

Proof

Using lattice periodicity

Being Bloch's theorem a statement about lattice periodicity, in this proof all the symmetries are encoded as translation symmetries of the wave function itself.

Proof Using lattice periodicity

Source:

Preliminaries: Crystal symmetries, lattice, and reciprocal lattice

The defining property of a crystal is translational symmetry, which means that if the crystal is shifted an appropriate amount, it winds up with all its atoms in the same places. (A finite-size crystal cannot have perfect translational symmetry, but it is a useful approximation.)

A three-dimensional crystal has three primitive lattice vectors a1, a2, a3. If the crystal is shifted by any of these three vectors, or a combination of them of the form n 1 a 1 + n 2 a 2 + n 3 a 3 , {\displaystyle n_{1}\mathbf {a} _{1}+n_{2}\mathbf {a} _{2}+n_{3}\mathbf {a} _{3},} where ni are three integers, then the atoms end up in the same set of locations as they started.

Another helpful ingredient in the proof is the reciprocal lattice vectors. These are three vectors b1, b2, b3 (with units of inverse length), with the property that ai · bi = 2π, but ai · bj = 0 when ij. (For the formula for bi, see reciprocal lattice vector.)

Lemma about translation operators

Let T ^ n 1 , n 2 , n 3 {\displaystyle {\hat {T}}_{n_{1},n_{2},n_{3}}} denote a translation operator that shifts every wave function by the amount n1a1 + n2a2 + n3a3 (as above, nj are integers). The following fact is helpful for the proof of Bloch's theorem:

Lemma — If a wave function ψ is an eigenstate of all of the translation operators (simultaneously), then ψ is a Bloch state.

Proof of Lemma

Assume that we have a wave function ψ which is an eigenstate of all the translation operators. As a special case of this, ψ ( r + a j ) = C j ψ ( r ) {\displaystyle \psi (\mathbf {r} +\mathbf {a} _{j})=C_{j}\psi (\mathbf {r} )} for j = 1, 2, 3, where Cj are three numbers (the eigenvalues) which do not depend on r. It is helpful to write the numbers Cj in a different form, by choosing three numbers θ1, θ2, θ3 with e = Cj: ψ ( r + a j ) = e 2 π i θ j ψ ( r ) {\displaystyle \psi (\mathbf {r} +\mathbf {a} _{j})=e^{2\pi i\theta _{j}}\psi (\mathbf {r} )} Again, the θj are three numbers which do not depend on r. Define k = θ1b1 + θ2b2 + θ3b3, where bj are the reciprocal lattice vectors (see above). Finally, define u ( r ) = e i k r ψ ( r ) . {\displaystyle u(\mathbf {r} )=e^{-i\mathbf {k} \cdot \mathbf {r} }\psi (\mathbf {r} )\,.} Then u ( r + a j ) = e i k ( r + a j ) ψ ( r + a j ) = ( e i k r e i k a j ) ( e 2 π i θ j ψ ( r ) ) = e i k r e 2 π i θ j e 2 π i θ j ψ ( r ) = u ( r ) . {\displaystyle {\begin{aligned}u(\mathbf {r} +\mathbf {a} _{j})&=e^{-i\mathbf {k} \cdot (\mathbf {r} +\mathbf {a} _{j})}\psi (\mathbf {r} +\mathbf {a} _{j})\\&={\big (}e^{-i\mathbf {k} \cdot \mathbf {r} }e^{-i\mathbf {k} \cdot \mathbf {a} _{j}}{\big )}{\big (}e^{2\pi i\theta _{j}}\psi (\mathbf {r} ){\big )}\\&=e^{-i\mathbf {k} \cdot \mathbf {r} }e^{-2\pi i\theta _{j}}e^{2\pi i\theta _{j}}\psi (\mathbf {r} )\\&=u(\mathbf {r} ).\end{aligned}}} This proves that u has the periodicity of the lattice. Since ψ ( r ) = e i k r u ( r ) , {\displaystyle \psi (\mathbf {r} )=e^{i\mathbf {k} \cdot \mathbf {r} }u(\mathbf {r} ),} that proves that the state is a Bloch state.

Finally, we are ready for the main proof of Bloch's theorem which is as follows.

As above, let T ^ n 1 , n 2 , n 3 {\displaystyle {\hat {T}}_{n_{1},n_{2},n_{3}}} denote a translation operator that shifts every wave function by the amount n1a1 + n2a2 + n3a3, where ni are integers. Because the crystal has translational symmetry, this operator commutes with the Hamiltonian operator. Moreover, every such translation operator commutes with every other. Therefore, there is a simultaneous eigenbasis of the Hamiltonian operator and every possible T ^ n 1 , n 2 , n 3 {\displaystyle {\hat {T}}_{n_{1},n_{2},n_{3}}\!} operator. This basis is what we are looking for. The wave functions in this basis are energy eigenstates (because they are eigenstates of the Hamiltonian), and they are also Bloch states (because they are eigenstates of the translation operators; see Lemma above).

Using operators

In this proof all the symmetries are encoded as commutation properties of the translation operators

Proof using operators

Source:

We define the translation operator T ^ n ψ ( r ) = ψ ( r + T n ) = ψ ( r + n 1 a 1 + n 2 a 2 + n 3 a 3 ) = ψ ( r + A n ) {\displaystyle {\begin{aligned}{\hat {\mathbf {T} }}_{\mathbf {n} }\psi (\mathbf {r} )&=\psi (\mathbf {r} +\mathbf {T} _{\mathbf {n} })\\&=\psi (\mathbf {r} +n_{1}\mathbf {a} _{1}+n_{2}\mathbf {a} _{2}+n_{3}\mathbf {a} _{3})\\&=\psi (\mathbf {r} +\mathbf {A} \mathbf {n} )\end{aligned}}} with A = [ a 1 a 2 a 3 ] , n = ( n 1 n 2 n 3 ) {\displaystyle \mathbf {A} ={\begin{bmatrix}\mathbf {a} _{1}&\mathbf {a} _{2}&\mathbf {a} _{3}\end{bmatrix}},\quad \mathbf {n} ={\begin{pmatrix}n_{1}\\n_{2}\\n_{3}\end{pmatrix}}} We use the hypothesis of a mean periodic potential U ( x + T n ) = U ( x ) {\displaystyle U(\mathbf {x} +\mathbf {T} _{\mathbf {n} })=U(\mathbf {x} )} and the independent electron approximation with an Hamiltonian H ^ = p ^ 2 2 m + U ( x ) {\displaystyle {\hat {H}}={\frac {{\hat {\mathbf {p} }}^{2}}{2m}}+U(\mathbf {x} )} Given the Hamiltonian is invariant for translations it shall commute with the translation operator [ H ^ , T ^ n ] = 0 {\displaystyle =0} and the two operators shall have a common set of eigenfunctions. Therefore, we start to look at the eigen-functions of the translation operator: T ^ n ψ ( x ) = λ n ψ ( x ) {\displaystyle {\hat {\mathbf {T} }}_{\mathbf {n} }\psi (\mathbf {x} )=\lambda _{\mathbf {n} }\psi (\mathbf {x} )} Given T ^ n {\displaystyle {\hat {\mathbf {T} }}_{\mathbf {n} }} is an additive operator T ^ n 1 T ^ n 2 ψ ( x ) = ψ ( x + A n 1 + A n 2 ) = T ^ n 1 + n 2 ψ ( x ) {\displaystyle {\hat {\mathbf {T} }}_{\mathbf {n} _{1}}{\hat {\mathbf {T} }}_{\mathbf {n} _{2}}\psi (\mathbf {x} )=\psi (\mathbf {x} +\mathbf {A} \mathbf {n} _{1}+\mathbf {A} \mathbf {n} _{2})={\hat {\mathbf {T} }}_{\mathbf {n} _{1}+\mathbf {n} _{2}}\psi (\mathbf {x} )} If we substitute here the eigenvalue equation and dividing both sides for ψ ( x ) {\displaystyle \psi (\mathbf {x} )} we have λ n 1 λ n 2 = λ n 1 + n 2 {\displaystyle \lambda _{\mathbf {n} _{1}}\lambda _{\mathbf {n} _{2}}=\lambda _{\mathbf {n} _{1}+\mathbf {n} _{2}}}

This is true for λ n = e s n a {\displaystyle \lambda _{\mathbf {n} }=e^{s\mathbf {n} \cdot \mathbf {a} }} where s C {\displaystyle s\in \mathbb {C} } if we use the normalization condition over a single primitive cell of volume V 1 = V | ψ ( x ) | 2 d x = V | T ^ n ψ ( x ) | 2 d x = | λ n | 2 V | ψ ( x ) | 2 d x {\displaystyle 1=\int _{V}|\psi (\mathbf {x} )|^{2}d\mathbf {x} =\int _{V}\left|{\hat {\mathbf {T} }}_{\mathbf {n} }\psi (\mathbf {x} )\right|^{2}d\mathbf {x} =|\lambda _{\mathbf {n} }|^{2}\int _{V}|\psi (\mathbf {x} )|^{2}d\mathbf {x} } and therefore 1 = | λ n | 2 {\displaystyle 1=|\lambda _{\mathbf {n} }|^{2}} and s = i k {\displaystyle s=ik} where k R {\displaystyle k\in \mathbb {R} } . Finally, T ^ n ψ ( x ) = ψ ( x + n a ) = e i k n a ψ ( x ) , {\displaystyle \mathbf {{\hat {T}}_{n}} \psi (\mathbf {x} )=\psi (\mathbf {x} +\mathbf {n} \cdot \mathbf {a} )=e^{ik\mathbf {n} \cdot \mathbf {a} }\psi (\mathbf {x} ),} which is true for a Bloch wave i.e. for ψ k ( x ) = e i k x u k ( x ) {\displaystyle \psi _{\mathbf {k} }(\mathbf {x} )=e^{i\mathbf {k} \cdot \mathbf {x} }u_{\mathbf {k} }(\mathbf {x} )} with u k ( x ) = u k ( x + A n ) {\displaystyle u_{\mathbf {k} }(\mathbf {x} )=u_{\mathbf {k} }(\mathbf {x} +\mathbf {A} \mathbf {n} )}

Using group theory

Apart from the group theory technicalities this proof is interesting because it becomes clear how to generalize the Bloch theorem for groups that are not only translations. This is typically done for space groups which are a combination of a translation and a point group and it is used for computing the band structure, spectrum and specific heats of crystals given a specific crystal group symmetry like FCC or BCC and eventually an extra basis. In this proof it is also possible to notice how it is key that the extra point group is driven by a symmetry in the effective potential but it shall commute with the Hamiltonian.

Proof with character theory

All translations are unitary and abelian. Translations can be written in terms of unit vectors τ = i = 1 3 n i a i {\displaystyle {\boldsymbol {\tau }}=\sum _{i=1}^{3}n_{i}\mathbf {a} _{i}} We can think of these as commuting operators τ ^ = τ ^ 1 τ ^ 2 τ ^ 3 {\displaystyle {\hat {\boldsymbol {\tau }}}={\hat {\boldsymbol {\tau }}}_{1}{\hat {\boldsymbol {\tau }}}_{2}{\hat {\boldsymbol {\tau }}}_{3}} where τ ^ i = n i a ^ i {\displaystyle {\hat {\boldsymbol {\tau }}}_{i}=n_{i}{\hat {\mathbf {a} }}_{i}}

The commutativity of the τ ^ i {\displaystyle {\hat {\boldsymbol {\tau }}}_{i}} operators gives three commuting cyclic subgroups (given they can be generated by only one element) which are infinite, 1-dimensional and abelian. All irreducible representations of abelian groups are one dimensional.

Given they are one dimensional the matrix representation and the character are the same. The character is the representation over the complex numbers of the group or also the trace of the representation which in this case is a one dimensional matrix. All these subgroups, given they are cyclic, they have characters which are appropriate roots of unity. In fact they have one generator γ {\displaystyle \gamma } which shall obey to γ n = 1 {\displaystyle \gamma ^{n}=1} , and therefore the character χ ( γ ) n = 1 {\displaystyle \chi (\gamma )^{n}=1} . Note that this is straightforward in the finite cyclic group case but in the countable infinite case of the infinite cyclic group (i.e. the translation group here) there is a limit for n {\displaystyle n\to \infty } where the character remains finite.

Given the character is a root of unity, for each subgroup the character can be then written as χ k 1 ( τ ^ 1 ( n 1 , a 1 ) ) = e i k 1 n 1 a 1 {\displaystyle \chi _{k_{1}}({\hat {\boldsymbol {\tau }}}_{1}(n_{1},a_{1}))=e^{ik_{1}n_{1}a_{1}}}

If we introduce the Born–von Karman boundary condition on the potential: V ( r + i N i a i ) = V ( r + L ) = V ( r ) {\displaystyle V\left(\mathbf {r} +\sum _{i}N_{i}\mathbf {a} _{i}\right)=V(\mathbf {r} +\mathbf {L} )=V(\mathbf {r} )} where L is a macroscopic periodicity in the direction a {\displaystyle \mathbf {a} } that can also be seen as a multiple of a i {\displaystyle a_{i}} where L = i N i a i {\textstyle \mathbf {L} =\sum _{i}N_{i}\mathbf {a} _{i}}

This substituting in the time independent Schrödinger equation with a simple effective Hamiltonian H ^ = 2 2 m 2 + V ( r ) {\displaystyle {\hat {H}}=-{\frac {\hbar ^{2}}{2m}}\nabla ^{2}+V(\mathbf {r} )} induces a periodicity with the wave function: ψ ( r + i N i a i ) = ψ ( r ) {\displaystyle \psi \left(\mathbf {r} +\sum _{i}N_{i}\mathbf {a} _{i}\right)=\psi (\mathbf {r} )}

And for each dimension a translation operator with a period L P ^ ε | τ i + L i = P ^ ε | τ i {\displaystyle {\hat {P}}_{\varepsilon |\tau _{i}+L_{i}}={\hat {P}}_{\varepsilon |\tau _{i}}}

From here we can see that also the character shall be invariant by a translation of L i {\displaystyle L_{i}} : e i k 1 n 1 a 1 = e i k 1 ( n 1 a 1 + L 1 ) {\displaystyle e^{ik_{1}n_{1}a_{1}}=e^{ik_{1}(n_{1}a_{1}+L_{1})}} and from the last equation we get for each dimension a periodic condition: k 1 n 1 a 1 = k 1 ( n 1 a 1 + L 1 ) 2 π m 1 {\displaystyle k_{1}n_{1}a_{1}=k_{1}(n_{1}a_{1}+L_{1})-2\pi m_{1}} where m 1 Z {\displaystyle m_{1}\in \mathbb {Z} } is an integer and k 1 = 2 π m 1 L 1 {\displaystyle k_{1}={\frac {2\pi m_{1}}{L_{1}}}}

The wave vector k 1 {\displaystyle k_{1}} identify the irreducible representation in the same manner as m 1 {\displaystyle m_{1}} , and L 1 {\displaystyle L_{1}} is a macroscopic periodic length of the crystal in direction a 1 {\displaystyle a_{1}} . In this context, the wave vector serves as a quantum number for the translation operator.

We can generalize this for 3 dimensions χ k 1 ( n 1 , a 1 ) χ k 2 ( n 2 , a 2 ) χ k 3 ( n 3 , a 3 ) = e i k τ {\displaystyle \chi _{k_{1}}(n_{1},a_{1})\chi _{k_{2}}(n_{2},a_{2})\chi _{k_{3}}(n_{3},a_{3})=e^{i\mathbf {k} \cdot {\boldsymbol {\tau }}}} and the generic formula for the wave function becomes: P ^ R ψ j = α ψ α χ α j ( R ) {\displaystyle {\hat {P}}_{R}\psi _{j}=\sum _{\alpha }\psi _{\alpha }\chi _{\alpha j}(R)} i.e. specializing it for a translation P ^ ε | τ ψ ( r ) = ψ ( r ) e i k τ = ψ ( r + τ ) {\displaystyle {\hat {P}}_{\varepsilon |{\boldsymbol {\tau }}}\psi (\mathbf {r} )=\psi (\mathbf {r} )e^{i\mathbf {k} \cdot {\boldsymbol {\tau }}}=\psi (\mathbf {r} +{\boldsymbol {\tau }})} and we have proven Bloch’s theorem.

In the generalized version of the Bloch theorem, the Fourier transform, i.e. the wave function expansion, gets generalized from a discrete Fourier transform which is applicable only for cyclic groups, and therefore translations, into a character expansion of the wave function where the characters are given from the specific finite point group.

Also here is possible to see how the characters (as the invariants of the irreducible representations) can be treated as the fundamental building blocks instead of the irreducible representations themselves.

Velocity and effective mass

If we apply the time-independent Schrödinger equation to the Bloch wave function we obtain H ^ k u k ( r ) = [ 2 2 m ( i + k ) 2 + U ( r ) ] u k ( r ) = ε k u k ( r ) {\displaystyle {\hat {H}}_{\mathbf {k} }u_{\mathbf {k} }(\mathbf {r} )=\leftu_{\mathbf {k} }(\mathbf {r} )=\varepsilon _{\mathbf {k} }u_{\mathbf {k} }(\mathbf {r} )} with boundary conditions u k ( r ) = u k ( r + R ) {\displaystyle u_{\mathbf {k} }(\mathbf {r} )=u_{\mathbf {k} }(\mathbf {r} +\mathbf {R} )} Given this is defined in a finite volume we expect an infinite family of eigenvalues; here k {\displaystyle {\mathbf {k} }} is a parameter of the Hamiltonian and therefore we arrive at a "continuous family" of eigenvalues ε n ( k ) {\displaystyle \varepsilon _{n}(\mathbf {k} )} dependent on the continuous parameter k {\displaystyle {\mathbf {k} }} and thus at the basic concept of an electronic band structure.

Proof

E k ( e i k x u k ( x ) ) = [ 2 2 m 2 + U ( x ) ] ( e i k x u k ( x ) ) {\displaystyle E_{\mathbf {k} }\left(e^{i\mathbf {k} \cdot \mathbf {x} }u_{\mathbf {k} }(\mathbf {x} )\right)=\left\left(e^{i\mathbf {k} \cdot \mathbf {x} }u_{\mathbf {k} }(\mathbf {x} )\right)}

We remain with E k e i k x u k ( x ) = 2 2 m ( i k e i k x u k ( x ) + e i k x u k ( x ) ) + U ( x ) e i k x u k ( x ) E k e i k x u k ( x ) = 2 2 m ( i k ( i k e i k x u k ( x ) + e i k x u k ( x ) ) + i k e i k x u k ( x ) + e i k x 2 u k ( x ) ) + U ( x ) e i k x u k ( x ) E k e i k x u k ( x ) = 2 2 m ( k 2 e i k x u k ( x ) 2 i k e i k x u k ( x ) e i k x 2 u k ( x ) ) + U ( x ) e i k x u k ( x ) E k u k ( x ) = 2 2 m ( i + k ) 2 u k ( x ) + U ( x ) u k ( x ) {\displaystyle {\begin{aligned}E_{\mathbf {k} }e^{i\mathbf {k} \cdot \mathbf {x} }u_{\mathbf {k} }(\mathbf {x} )&={\frac {-\hbar ^{2}}{2m}}\nabla \cdot \left(i\mathbf {k} e^{i\mathbf {k} \cdot \mathbf {x} }u_{\mathbf {k} }(\mathbf {x} )+e^{i\mathbf {k} \cdot \mathbf {x} }\nabla u_{\mathbf {k} }(\mathbf {x} )\right)+U(\mathbf {x} )e^{i\mathbf {k} \cdot \mathbf {x} }u_{\mathbf {k} }(\mathbf {x} )\\E_{\mathbf {k} }e^{i\mathbf {k} \cdot \mathbf {x} }u_{\mathbf {k} }(\mathbf {x} )&={\frac {-\hbar ^{2}}{2m}}\left(i\mathbf {k} \cdot \left(i\mathbf {k} e^{i\mathbf {k} \cdot \mathbf {x} }u_{\mathbf {k} }(\mathbf {x} )+e^{i\mathbf {k} \cdot \mathbf {x} }\nabla u_{\mathbf {k} }(\mathbf {x} )\right)+i\mathbf {k} \cdot e^{i\mathbf {k} \cdot \mathbf {x} }\nabla u_{\mathbf {k} }(\mathbf {x} )+e^{i\mathbf {k} \cdot \mathbf {x} }\nabla ^{2}u_{\mathbf {k} }(\mathbf {x} )\right)+U(\mathbf {x} )e^{i\mathbf {k} \cdot \mathbf {x} }u_{\mathbf {k} }(\mathbf {x} )\\E_{\mathbf {k} }e^{i\mathbf {k} \cdot \mathbf {x} }u_{\mathbf {k} }(\mathbf {x} )&={\frac {\hbar ^{2}}{2m}}\left(\mathbf {k} ^{2}e^{i\mathbf {k} \cdot \mathbf {x} }u_{\mathbf {k} }(\mathbf {x} )-2i\mathbf {k} \cdot e^{i\mathbf {k} \cdot \mathbf {x} }\nabla u_{\mathbf {k} }(\mathbf {x} )-e^{i\mathbf {k} \cdot \mathbf {x} }\nabla ^{2}u_{\mathbf {k} }(\mathbf {x} )\right)+U(\mathbf {x} )e^{i\mathbf {k} \cdot \mathbf {x} }u_{\mathbf {k} }(\mathbf {x} )\\E_{\mathbf {k} }u_{\mathbf {k} }(\mathbf {x} )&={\frac {\hbar ^{2}}{2m}}\left(-i\nabla +\mathbf {k} \right)^{2}u_{\mathbf {k} }(\mathbf {x} )+U(\mathbf {x} )u_{\mathbf {k} }(\mathbf {x} )\end{aligned}}}

This shows how the effective momentum can be seen as composed of two parts, p ^ eff = i + k , {\displaystyle {\hat {\mathbf {p} }}_{\text{eff}}=-i\hbar \nabla +\hbar \mathbf {k} ,} a standard momentum i {\displaystyle -i\hbar \nabla } and a crystal momentum k {\displaystyle \hbar \mathbf {k} } . More precisely the crystal momentum is not a momentum but it stands for the momentum in the same way as the electromagnetic momentum in the minimal coupling, and as part of a canonical transformation of the momentum.

For the effective velocity we can derive

mean velocity of a Bloch electron

ε n k = 2 m d r ψ n k ( i ) ψ n k = m p ^ = v ^ {\displaystyle {\frac {\partial \varepsilon _{n}}{\partial \mathbf {k} }}={\frac {\hbar ^{2}}{m}}\int d\mathbf {r} \,\psi _{n\mathbf {k} }^{*}(-i\nabla )\psi _{n\mathbf {k} }={\frac {\hbar }{m}}\langle {\hat {\mathbf {p} }}\rangle =\hbar \langle {\hat {\mathbf {v} }}\rangle }

Proof

We evaluate the derivatives ε n k {\displaystyle {\frac {\partial \varepsilon _{n}}{\partial \mathbf {k} }}} and 2 ε n ( k ) k i k j {\displaystyle {\frac {\partial ^{2}\varepsilon _{n}(\mathbf {k} )}{\partial k_{i}\partial k_{j}}}} given they are the coefficients of the following expansion in q where q is considered small with respect to k ε n ( k + q ) = ε n ( k ) + i ε n k i q i + 1 2 i j 2 ε n k i k j q i q j + O ( q 3 ) {\displaystyle \varepsilon _{n}(\mathbf {k} +\mathbf {q} )=\varepsilon _{n}(\mathbf {k} )+\sum _{i}{\frac {\partial \varepsilon _{n}}{\partial k_{i}}}q_{i}+{\frac {1}{2}}\sum _{ij}{\frac {\partial ^{2}\varepsilon _{n}}{\partial k_{i}\partial k_{j}}}q_{i}q_{j}+O(q^{3})} Given ε n ( k + q ) {\displaystyle \varepsilon _{n}(\mathbf {k} +\mathbf {q} )} are eigenvalues of H ^ k + q {\displaystyle {\hat {H}}_{\mathbf {k} +\mathbf {q} }} We can consider the following perturbation problem in q: H ^ k + q = H ^ k + 2 m q ( i + k ) + 2 2 m q 2 {\displaystyle {\hat {H}}_{\mathbf {k} +\mathbf {q} }={\hat {H}}_{\mathbf {k} }+{\frac {\hbar ^{2}}{m}}\mathbf {q} \cdot (-i\nabla +\mathbf {k} )+{\frac {\hbar ^{2}}{2m}}q^{2}} Perturbation theory of the second order states that E n = E n 0 + d r ψ n V ^ ψ n + n n | d r ψ n V ^ ψ n | 2 E n 0 E n 0 + . . . {\displaystyle E_{n}=E_{n}^{0}+\int d\mathbf {r} \,\psi _{n}^{*}{\hat {V}}\psi _{n}+\sum _{n'\neq n}{\frac {|\int d\mathbf {r} \,\psi _{n}^{*}{\hat {V}}\psi _{n}|^{2}}{E_{n}^{0}-E_{n'}^{0}}}+...} To compute to linear order in q i ε n k i q i = i d r u n k 2 m ( i + k ) i q i u n k {\displaystyle \sum _{i}{\frac {\partial \varepsilon _{n}}{\partial k_{i}}}q_{i}=\sum _{i}\int d\mathbf {r} \,u_{n\mathbf {k} }^{*}{\frac {\hbar ^{2}}{m}}(-i\nabla +\mathbf {k} )_{i}q_{i}u_{n\mathbf {k} }} where the integrations are over a primitive cell or the entire crystal, given if the integral d r u n k u n k {\displaystyle \int d\mathbf {r} \,u_{n\mathbf {k} }^{*}u_{n\mathbf {k} }} is normalized across the cell or the crystal.

We can simplify over q to obtain ε n k = 2 m d r u n k ( i + k ) u n k {\displaystyle {\frac {\partial \varepsilon _{n}}{\partial \mathbf {k} }}={\frac {\hbar ^{2}}{m}}\int d\mathbf {r} \,u_{n\mathbf {k} }^{*}(-i\nabla +\mathbf {k} )u_{n\mathbf {k} }} and we can reinsert the complete wave functions ε n k = 2 m d r ψ n k ( i ) ψ n k {\displaystyle {\frac {\partial \varepsilon _{n}}{\partial \mathbf {k} }}={\frac {\hbar ^{2}}{m}}\int d\mathbf {r} \,\psi _{n\mathbf {k} }^{*}(-i\nabla )\psi _{n\mathbf {k} }}

For the effective mass

effective mass theorem

2 ε n ( k ) k i k j = 2 m δ i j + ( 2 m ) 2 n n n k | i i | n k n k | i j | n k + n k | i j | n k n k | i i | n k ε n ( k ) ε n ( k ) {\displaystyle {\frac {\partial ^{2}\varepsilon _{n}(\mathbf {k} )}{\partial k_{i}\partial k_{j}}}={\frac {\hbar ^{2}}{m}}\delta _{ij}+\left({\frac {\hbar ^{2}}{m}}\right)^{2}\sum _{n'\neq n}{\frac {\langle n\mathbf {k} |-i\nabla _{i}|n'\mathbf {k} \rangle \langle n'\mathbf {k} |-i\nabla _{j}|n\mathbf {k} \rangle +\langle n\mathbf {k} |-i\nabla _{j}|n'\mathbf {k} \rangle \langle n'\mathbf {k} |-i\nabla _{i}|n\mathbf {k} \rangle }{\varepsilon _{n}(\mathbf {k} )-\varepsilon _{n'}(\mathbf {k} )}}}

Proof

The second order term 1 2 i j 2 ε n k i k j q i q j = 2 2 m q 2 + n n | d r u n k 2 m q ( i + k ) u n k | 2 ε n k ε n k {\displaystyle {\frac {1}{2}}\sum _{ij}{\frac {\partial ^{2}\varepsilon _{n}}{\partial k_{i}\partial k_{j}}}q_{i}q_{j}={\frac {\hbar ^{2}}{2m}}q^{2}+\sum _{n'\neq n}{\frac {|\int d\mathbf {r} \,u_{n\mathbf {k} }^{*}{\frac {\hbar ^{2}}{m}}\mathbf {q} \cdot (-i\nabla +\mathbf {k} )u_{n'\mathbf {k} }|^{2}}{\varepsilon _{n\mathbf {k} }-\varepsilon _{n'\mathbf {k} }}}} Again with ψ n k = | n k = e i k x u n k {\displaystyle \psi _{n\mathbf {k} }=|n\mathbf {k} \rangle =e^{i\mathbf {k} \mathbf {x} }u_{n\mathbf {k} }} 1 2 i j 2 ε n k i k j q i q j = 2 2 m q 2 + n n | n k | 2 m q ( i ) | n k | 2 ε n k ε n k {\displaystyle {\frac {1}{2}}\sum _{ij}{\frac {\partial ^{2}\varepsilon _{n}}{\partial k_{i}\partial k_{j}}}q_{i}q_{j}={\frac {\hbar ^{2}}{2m}}q^{2}+\sum _{n'\neq n}{\frac {|\langle n\mathbf {k} |{\frac {\hbar ^{2}}{m}}\mathbf {q} \cdot (-i\nabla )|n'\mathbf {k} \rangle |^{2}}{\varepsilon _{n\mathbf {k} }-\varepsilon _{n'\mathbf {k} }}}} Eliminating q i {\displaystyle q_{i}} and q j {\displaystyle q_{j}} we have the theorem 2 ε n ( k ) k i k j = 2 m δ i j + ( 2 m ) 2 n n n k | i i | n k n k | i j | n k + n k | i j | n k n k | i i | n k ε n ( k ) ε n ( k ) {\displaystyle {\frac {\partial ^{2}\varepsilon _{n}(\mathbf {k} )}{\partial k_{i}\partial k_{j}}}={\frac {\hbar ^{2}}{m}}\delta _{ij}+\left({\frac {\hbar ^{2}}{m}}\right)^{2}\sum _{n'\neq n}{\frac {\langle n\mathbf {k} |-i\nabla _{i}|n'\mathbf {k} \rangle \langle n'\mathbf {k} |-i\nabla _{j}|n\mathbf {k} \rangle +\langle n\mathbf {k} |-i\nabla _{j}|n'\mathbf {k} \rangle \langle n'\mathbf {k} |-i\nabla _{i}|n\mathbf {k} \rangle }{\varepsilon _{n}(\mathbf {k} )-\varepsilon _{n'}(\mathbf {k} )}}}

The quantity on the right multiplied by a factor 1 2 {\displaystyle {\frac {1}{\hbar ^{2}}}} is called effective mass tensor M ( k ) {\displaystyle \mathbf {M} (\mathbf {k} )} and we can use it to write a semi-classical equation for a charge carrier in a band

Second order semi-classical equation of motion for a charge carrier in a band

M ( k ) a = e ( E + v ( k ) × B ) {\displaystyle \mathbf {M} (\mathbf {k} )\mathbf {a} =\mp e\left(\mathbf {E} +\mathbf {v} (\mathbf {k} )\times \mathbf {B} \right)}

where a {\displaystyle \mathbf {a} } is an acceleration. This equation is analogous to the de Broglie wave type of approximation

First order semi-classical equation of motion for electron in a band

k ˙ = e ( E + v × B ) {\displaystyle \hbar {\dot {k}}=-e\left(\mathbf {E} +\mathbf {v} \times \mathbf {B} \right)}

As an intuitive interpretation, both of the previous two equations resemble formally and are in a semi-classical analogy with Newton's second law for an electron in an external Lorentz force.

History and related equations

The concept of the Bloch state was developed by Felix Bloch in 1928 to describe the conduction of electrons in crystalline solids. The same underlying mathematics, however, was also discovered independently several times: by George William Hill (1877), Gaston Floquet (1883), and Alexander Lyapunov (1892). As a result, a variety of nomenclatures are common: applied to ordinary differential equations, it is called Floquet theory (or occasionally the Lyapunov–Floquet theorem). The general form of a one-dimensional periodic potential equation is Hill's equation: d 2 y d t 2 + f ( t ) y = 0 , {\displaystyle {\frac {d^{2}y}{dt^{2}}}+f(t)y=0,} where f(t) is a periodic potential. Specific periodic one-dimensional equations include the Kronig–Penney model and Mathieu's equation.

Mathematically Bloch's theorem is interpreted in terms of unitary characters of a lattice group, and is applied to spectral geometry.

See also

References

  1. Bloch, F. (1929). Über die quantenmechanik der elektronen in kristallgittern. Zeitschrift für physik, 52(7), 555-600.
  2. Kittel, Charles (1996). Introduction to Solid State Physics. New York: Wiley. ISBN 0-471-14286-7.
  3. Ziman, J. M. (1972). Principles of the theory of solids (2nd ed.). Cambridge University Press. pp. 17–20. ISBN 0521297338.
  4. Ashcroft & Mermin 1976, p. 134
  5. Ashcroft & Mermin 1976, p. 137
  6. ^ Dresselhaus, M. S. (2002). "Applications of Group Theory to the Physics of Solids" (PDF). MIT. Archived (PDF) from the original on 1 November 2019. Retrieved 12 September 2020.
  7. The vibrational spectrum and specific heat of a face centered cubic crystal, Robert B. Leighton
  8. Roy, Ricky (May 2, 2010). "Representation Theory" (PDF). University of Puget Sound.
  9. Group Representations and Harmonic Analysis from Euler to Langlands, Part II
  10. Ashcroft & Mermin 1976, p. 140
  11. ^ Ashcroft & Mermin 1976, p. 765 Appendix E
  12. Ashcroft & Mermin 1976, p. 228
  13. Ashcroft & Mermin 1976, p. 229
  14. Ashcroft & Mermin 1976, p. 227
  15. Felix Bloch (1928). "Über die Quantenmechanik der Elektronen in Kristallgittern". Zeitschrift für Physik (in German). 52 (7–8): 555–600. Bibcode:1929ZPhy...52..555B. doi:10.1007/BF01339455. S2CID 120668259.
  16. George William Hill (1886). "On the part of the motion of the lunar perigee which is a function of the mean motions of the sun and moon". Acta Math. 8: 1–36. doi:10.1007/BF02417081. This work was initially published and distributed privately in 1877.
  17. Gaston Floquet (1883). "Sur les équations différentielles linéaires à coefficients périodiques". Annales Scientifiques de l'École Normale Supérieure. 12: 47–88. doi:10.24033/asens.220.
  18. Alexander Mihailovich Lyapunov (1992). The General Problem of the Stability of Motion. London: Taylor and Francis. Translated by A. T. Fuller from Edouard Davaux's French translation (1907) of the original Russian dissertation (1892).
  19. Magnus, W; Winkler, S (2004). Hill's Equation. Courier Dover. p. 11. ISBN 0-486-49565-5.
  20. Kuchment, P.(1982), Floquet theory for partial differential equations, RUSS MATH SURV., 37, 1–60
  21. Katsuda, A.; Sunada, T (1987). "Homology and closed geodesics in a compact Riemann surface". Amer. J. Math. 110 (1): 145–156. doi:10.2307/2374542. JSTOR 2374542.
  22. Kotani M; Sunada T. (2000). "Albanese maps and an off diagonal long time asymptotic for the heat kernel". Comm. Math. Phys. 209 (3): 633–670. Bibcode:2000CMaPh.209..633K. doi:10.1007/s002200050033. S2CID 121065949.

Further reading

Condensed matter physics
States of matter
Phase phenomena
Electrons in solids
Phenomena
Theory
Conduction
Couplings
Magnetic phases
Quasiparticles
Soft matter
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