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628 C Mathematical Formulas

Since only the m = m1 + m2 terms give nonvanishing contribution, this can be rewritten in the form

Yl1

1 (θ, ϕ)Yl2

2 (θ, ϕ) =

l

/

 

4π

(C.4.30)

m

m

 

 

 

 

(2l1 + 1)(2l2 + 1)(2l + 1)

 

×

m1

m2

(m1

+ m2)

 

l1

l2

 

l

0 0 0 Yl

(m1+m2 )

(θ, ϕ) ,

l1 l2 l

 

where the square-root term on the right-hand side is a Clebsch–Gordan coefficient, while the parenthesized terms are the Wigner 3j symbols. Both will be discussed in detail in Appendix F.

This formula and the orthogonality relation for spherical harmonics imply that the integral of the product of three spherical harmonics is

dΩ Y m1

(θ, ϕ)Y m2

(θ, ϕ)Y m3

(θ, ϕ)

 

 

 

 

 

 

(C.4.31)

 

l1

l2

l3

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

=

/

 

 

 

4π

+ 1)

 

m1

m2

m3

0 0 0

.

 

 

 

(2l1 + 1)(2l2 + 1)(2l3

 

 

l1

l2

l3

l1

l2

l3

The explicit expressions for the first few spherical harmonics are

Y00 =

Y10 =

Y1±1 =

Y20 =

Y2±1 =

Y2±2 =

Y30 =

Y3±1 =

Y3±2 =

Y3±3 =

 

 

 

1/2

,

 

4π

 

 

 

1

 

 

 

 

 

 

 

 

 

 

1/2

 

 

4π

 

cos θ ,

 

3

 

 

 

 

 

 

 

 

 

 

 

1/2

 

8π

sin θe±iϕ ,

 

 

3

 

 

 

 

 

 

 

 

1/2

 

16π

(3 cos2 θ − 1) ,

 

5

 

 

 

 

 

 

 

15

1/2

 

 

sin θ cos θe±iϕ ,

(C.4.32)

 

8π

15

 

1/2

 

 

 

sin2 θe±2iϕ ,

 

 

 

 

32π

 

7

 

 

1/2

 

 

 

 

(5 cos3 θ − 3 cos θ) ,

 

 

 

 

16π

 

 

64π

1/2

 

(5 cos2 θ − 1) sin θe±iϕ ,

 

 

21

 

 

 

 

 

 

 

1/2

 

32π

sin2 θ cos θe±2iϕ ,

 

105

 

 

 

 

 

 

64π

1/2

 

sin3 θe±3iϕ .

 

 

35

 

 

 

C.4 Orthogonal Polynomials

629

C.4.5 Expansion in Spherical Harmonics

It follows from the orthogonality and completeness relations that any function f (θ, ϕ) that depends only on the polar angles can be expanded in spherical harmonics:

l

f (θ, ϕ) =

 

 

clmY m(θ, ϕ) ,

(C.4.33)

 

l

 

where

l=0 m=−l

 

 

 

clm =

Ylm (θ, ϕ)f (θ, ϕ) dΩ .

(C.4.34)

Another expansion is used for functions that depend on the angle between two vectors specified by spherical coordinates. We shall denote the angle between the directions specified by the polar angles θ, ϕ and θ , ϕ by ζ. They are related by

cos ζ = cos θ cos θ + sin θ sin θ cos(ϕ − ϕ ) .

(C.4.35)

In the expansion in associated Legendre polynomials or spherical harmonics

Pl(cos ζ) = Pl(cos θ)Pl(cos θ )

+2

l

 

 

(l − m)! P m(cos θ)P m(cos θ ) cos m(ϕ

 

ϕ )

 

 

 

 

 

 

 

l

l

 

 

 

m=1

(l + m)!

 

 

 

4π

 

 

+l

 

 

 

 

 

 

 

 

 

 

 

 

=

 

 

 

 

Y m

(θ, ϕ)Y m(θ , ϕ ) .

 

(C.4.36)

2l + 1

 

 

 

 

 

 

l

 

l

 

 

 

m=−l

 

 

 

 

 

 

 

 

 

 

 

By applying the relation

eixy = (2l + 1)iljl(y)Pl(x)

l=0

to the expansion of a plane wave,

eik·r = (2l + 1)iljl(kr)Pl (cos θ)

l=0

+l

=4π iljl(kr)Ylm (θk , ϕk )Ylm(θr , ϕr ) ,

l=0 m=−l

(C.4.37)

(C.4.38)

where (θk , ϕk ), and (θr , ϕr ) are the polar angles of the vectors k and r. The so-called multipole expansion of the Coulomb potential is

1

 

|

rl

 

 

 

(C.4.39)

| −

 

 

<

 

 

 

r

r

 

=

rl+1

Pl(cos ζ)

 

 

 

 

l=0

>

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

rl

 

4π

+l

(θ, ϕ)Y m(θ , ϕ ) ,

 

 

 

=

<

 

 

Y m

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

l

l

 

 

 

l=0

r>l+1

 

2l + 1

m=−l

 

 

 

 

 

 

 

 

630 C Mathematical Formulas

where r< (r>) denotes the length of the shorter (longer) vector of r and r . As will be shown in Chapter 16 (Volume 2), the Green function of free

electrons can be written as

 

 

G(r, r ) =

me eik|r−r |

(C.4.40)

 

 

 

 

 

,

 

 

 

2π 2

|r − r |

since

 

 

 

 

 

 

 

 

 

 

 

eik|r|

 

 

 

 

 

cos k r

 

2 + k2

 

= 4πδ(r) ,

2 + k2

| |

= 4πδ(r) .

(C.4.41)

|r|

|r|

The Green function, as well as its real and imaginary parts can be expressed in terms of the spherical harmonics

eik|r−r |

 

 

 

 

 

(1)

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

(kr>)Pl(cos ζ)

 

(C.4.42)

|

 

 

 

|

 

 

 

 

 

 

 

 

r

 

r

 

 

= ik

(2l + 1)jl(kr<)hl

 

 

 

 

 

 

 

l=0

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

= 4π ik

+l

jl(kr<)h(1)(kr>)Y m (θ, ϕ)Y m(θ , ϕ ) ,

 

 

 

 

 

 

 

 

 

 

 

 

 

l

 

 

l

 

 

l

 

 

 

 

 

 

 

 

 

 

 

 

l=0 m=−l

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

sin(k|r − r |)

 

= k

 

 

 

 

 

 

 

 

 

 

 

 

(2l + 1)jl(kr<)jl(kr>)Pl(cos ζ)

(C.4.43)

 

 

 

|

r

r

|

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

l=0

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

+l

Ylm

(θ, ϕ)Ylm(θ

, ϕ ) ,

 

 

 

 

 

 

 

 

 

 

 

= 4πk

jl(kr<)jl(kr>)

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

l=0

 

 

m=−l

 

 

 

 

cos(k|r − r |)

 

=

 

k

(2l + 1)j (kr

)n (kr

 

)P (cos ζ)

 

 

 

 

|

 

 

r

|

 

 

 

l

<

l

 

> l

 

(C.4.44)

 

 

 

r

 

 

 

 

 

l=0

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

= 4πk

 

 

 

+l

 

 

 

 

 

 

 

 

 

 

 

 

 

 

j (kr )n (kr )

 

Y m (θ, ϕ)Y m(θ , ϕ )

 

 

 

 

 

 

 

 

 

 

 

 

 

l <

l

>

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

l

l

 

 

 

 

 

 

 

 

 

 

 

 

 

 

l=0

 

 

 

m=−l

 

 

where ζ is the angle between the directions of r and r , while (θ, ϕ) and (θ , ϕ ) are the polar angles of r and r .

It follows from the orthogonality relation for associated Legendre polynomials that if the two functions

l

Al(θ, ϕ) = a0Pl(cos θ) + (am cos + bm sin ) Plm(cos θ) ,

m=1

(C.4.45)

l

Bl (θ, ϕ) = α0Pl (cos θ) + (αm cos + βm sin ) Plm(cos θ)

m=1

(C.4.46)

C.4 Orthogonal Polynomials

631

are introduced with arbitrary coe cients, the following formulas are valid:

 

 

 

 

2π

π

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

dϕ

Al(θ, ϕ)Bl (θ, ϕ) sin θ dθ = 0

(C.4.47)

 

 

 

 

0

0

 

 

 

 

if

l = l

, and

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

2π

π

 

 

 

π

 

 

 

 

 

 

 

 

 

 

 

0

dϕ 0

Al(θ, ϕ)Pl (cos ζ) sin θ dθ =

4

Al(θ , ϕ ) .

(C.4.48)

 

 

2l + 1

 

The general solution of the free Schrödinger equation in spherical coordi-

nates can be written as

 

 

 

 

 

 

 

 

 

ψ(r , θ , ϕ ) =

fl(r )Ylm(θ , ϕ ) ,

(C.4.49)

 

 

 

 

 

 

l,m

 

 

 

 

 

 

 

 

 

 

 

where the fl(r ) are spherical Bessel functions of the first or second kind. The same function can be expanded around a di erent origin (displaced by r with respect to the first), using the spherical coordinates r , θ , ϕ of the vector r = r + r . The obtained functions fl(r ) are related to the fl(r ) via the Wigner 3j symbols:

fl(r )Ylm(θ , ϕ ) = l ,l ,m il

+l −l(1)m(2l + 1)(2l + 1)

 

l l

l

 

0 0

0

 

 

 

 

 

 

 

(C.4.50)

 

 

 

 

 

 

 

l l

l

m

m

 

 

m

 

× m −m m − m

jl (r)Yl

(θ, ϕ)fl (r )Yl

(θ , ϕ ) ,

where r, θ, ϕ are the spherical coordinates of r.

References

1.G. B. Arfken and H.-J. Weber, Mathematical Methods for Physicists, Sixth Edition, Elsevier/Academic Press, Amsterdam (2005).

2.Handbook of Mathematical Functions with Formulas, Graphs, and Mathematical Tables, Edited by M. Abramowitz and I. A. Stegun, 10th printing, Dover Publications, Inc., New York (1972). It is available online at www.math.sfu.ca/ cbm/aands.

3.I. S. Gradshteyn and I. M. Ryzhik, Table of Integrals, Series and Products, Sixth Edition, Edited by A. Je rey and D. Zwillinger, Academic Press, Inc., Boston (2000).

632 C Mathematical Formulas

4.A. P. Prudnikov, Yu. A. Brychkov and O. I. Marichev, Integrals and Series, Vol. 1. Elementary Functions, Gordon and Breach Science Publishers, New York (1986).

5.A. P. Prudnikov, Yu. A. Brychkov and O. I. Marichev, Integrals and Series, Vol. 2. Special Functions, Gordon and Breach Science Publishers, New York (1990).

D

Fundamentals of Group Theory

As mentioned in Chapter 6, crystalline materials occupy a special place among solids not in the least because the symmetries of their structure manifest themselves in macroscopic properties, which highly facilitates the theoretical description of their behavior. Symmetry operations form a group in the mathematical sense, therefore statements of general validity can often be based on group-theoretical considerations. In this appendix we shall review some basic notions and relationships of group theory, then present the irreducible representations of the Oh group, and finally list the group theoretical theorems related to the quantum mechanical eigenvalue problem.

D.1 Basic Notions of Group Theory

There exists a whole wealth of group theoretical textbooks written by physicists for physicists. A few of them are listed among the references. These contain plenty of solid-state physics applications. Therefore below we shall discuss only a few basic notions and theorems.

D.1.1 Definition of Groups

The set of elements R, S, T, . . . are said to form a group G if a binary operation called multiplication is defined among group elements, which satisfies the following requirements:

1.For any two elements R and S the product, denoted as R S, is an element T of the group:

R S = T

(R, S, T G) .

(D.1.1)

The operation of group multiplication does not need to be commutative: in general the order of the elements is not immaterial. A group is called commutative or Abelian if group multiplication satisfies the commutative law, i.e., R S = S R for any two elements R and S.

634 D Fundamentals of Group Theory

2.Multiplication satisfies the associative law, i.e., for any elements R, S, and T

R(S T ) = (R S)T ,

(D.1.2)

where, naturally, multiplication within the parentheses has to be performed first.

3. There exists an identity element (also called unit element) E in the set. When any element R of the group is multiplied by E, it remains unchanged:

R E = E R = R .

(D.1.3)

4.For any element R of the group there exists a unique element S in the group such that

R S = S R = E .

(D.1.4)

This element S is called the inverse of R, and is denoted by S ≡ R1.

The number g of elements in the set is called the order of the group. The number of elements can be either finite or infinite; these correspond to finite and infinite groups. In solid-state physics applications we deal mostly with finite groups.

When the group is finite, the elements in the sequence R, R2, R3, . . .

repeat themselves from a certain point onward. Consequently one of these elements must be the identity element. The order of an element R in the group is the least positive integer n such that Rn = E.

A subset G of the group elements is called a subgroup of G if it satisfies in itself the previous requirements that define a group – i.e., it contains the identity element, for every element in G its inverse is also in G , and the product of any two elements in G is also in G .

A subgroup G of the group G is an invariant subgroup or normal subgroup if R S R1 G for every R G and every S G .

If R1, S1, T1, . . . are the elements of a group G1 of order g1, and R2, S2, T2, . . . are the elements of a group G2 of order g2, then the direct product (or Kronecker product ) of the two groups, denoted by G1 G2 is the group made up of the elements (R1, R2), (R1, S2), . . . , (S1, R2), (S1, S2), . . . , with the group multiplication defined as

(R1, S2)(T1, U2) = (R1T1, S2U2) . (D.1.5)

This group is of order g1 g2.

If G1 and G2 are such subgroups of G that 1.) the elements in G1 commute with the elements in G2; 2.) they have a single element in common, the identity element; and 3.) each element in G can be written as the product of an element in G1 and an element in G2, then the group G is isomorphic to the direct product group G1 G2.

The group G is the semidirect product of its subgroups G1 and G2 (G = G1 G2), if 1.) the elements in G1 do not commute with the elements in G2

D.1 Basic Notions of Group Theory

635

but G1 is an invariant subgroup; 2.) they have a single element in common, the identity element; and 3.) each element in G can be written as the product of an element in G1 and an element in G2.

D.1.2 Conjugate Elements and Conjugacy Classes

The group element S is conjugate to R if there exists at least one element U in the group such that S = U RU 1. This property is mutual, since along with U , its inverse U 1 is also an element of the group, consequently whenever the relation S = U RU 1 holds, so does R = U 1S(U 1)1. Thus S and R are said to be conjugate.

The conjugate property is transitive, that is if S and R are conjugate (S = U RU 1) and so are T and S (T = V SV 1) then T and R are conjugate,

too:

 

T = V SV 1 = V U RU 1V 1 = (V U )R(V U )1 .

(D.1.6)

Therefore the elements of the group can be unambiguously divided into classes of conjugate elements, conjugacy classes.

The multiplication rule R S = SR of Abelian groups implies that for any R and S the relation R = S1R S holds. Then each element is only conjugate to itself, and so forms a separate conjugacy class.

D.1.3 Representations and Characters

Consider a d-dimensional vector space spanned by the linearly independent vectors e1, e2, . . . , ed. Now define a nonsingular linear transformation O on this space such that each point

d

 

 

 

 

 

r =

aiei

(D.1.7)

i=1

 

 

of the space is taken into another point

 

 

 

d

 

 

 

r = Or =

biei .

(D.1.8)

i=1

Expressing the transforms of vectors ei in terms of the original vectors, the matrix D defined through

Oei =

 

(D.1.9)

Djiej

 

j

 

specifies the mapping between the components of r and r :

 

bi = Dij aj .

(D.1.10)

j

636 D Fundamentals of Group Theory

If the transformation between r and r is a one-to-one correspondence, then the inverse of the transformation O exists,

r = O1r ,

(D.1.11)

and this mapping can be given by the inverse of the matrix D:

 

 

 

 

ai =

D1

ij bj .

(D.1.12)

j

 

 

 

Consider a group G, and associate a linear operator O(R) and the corresponding matrix Dij (R) with each element R. If the same multiplication rule applies to the operators as to the group elements, i.e., for RS = T

O(R)O(S) = O(T ) ,

(D.1.13)

then the analogous relation

 

 

D(R)D(S) = D(T )

(D.1.14)

applies to the matrices, too. In component form

 

 

 

 

Djk (R)Dki (S) = Dji(T ) ,

(D.1.15)

k

 

 

as

 

 

 

 

O(R)O(S)ei = O(R)

Dki(S)ek

(D.1.16)

k

 

 

 

=

Dki(S)Djk (R)ej =

D(R)D(S) ji ej .

k j

j

 

The identity element E is associated with the identity operator and the unit matrix, while the inverse of the element R is associated with the inverse of the operator O(R) and the inverse of the matrix D(R). These matrices provide a representation of the group. The representation is faithful if the mapping is not only homomorphic but also isomorphic, i.e., there exists a one-to-one correspondence.

Two representations of a group are equivalent if there exists a unitary matrix U U = U 1 that transforms the matrices D(1)(R) and D(2)(R) belonging to the two representations into each other for each element of the group:

D(2)(R) = UD(1)(R)U 1 .

(D.1.17)

For every representation of a finite group there exists an equivalent representation in which the matrices are unitary. In what follows we shall only deal with unitary representations.

Being an invariant expression of the matrix elements, the diagonal sum (trace) of the matrices in the representation of the group plays an important

and D(ν)

D.1 Basic Notions of Group Theory

637

role in the characterization of the representations. The trace of matrix D(R) that represents the element R is called the character of the representation associated with the group element:

 

 

χ(R) = Tr D(R) = Dii(R) .

(D.1.18)

i

In any representation the characters of mutually conjugate elements (elements of the same conjugacy class) are identical, since if S = T R T 1 then

χ(S) = Tr D(T )D(R)D(T 1) = Tr D(R) = χ(R) .

(D.1.19)

Equivalent representations are associated with identical characters.

D.1.4 Reducible and Irreducible Representations

The matrices representing the group elements can be separately diagonalized by a unitary transformation D (R) = U D(R)U 1, however di erent matrices U are usually required for di erent elements. A representation is called reducible if there exists a matrix U that simultaneously block diagonalizes the matrices associated with each group element. If there exist no such unitary transformations that would lead to such a block-diagonal form, the representation is said to be irreducible.

Determining whether a representation is reducible or irreducible, finding the irreducible representations, and the reduction of a reducible representation rank among the most important applications of group theory in solidstate physics. These tasks are facilitated by the following theorems (presented without proof).

The number r of irreducible representations D(1), D(2), . . . , D(r) of a finite group is equal to the number of conjugacy classes in the group.

The dimensions dμ of irreducible representations and the number g of group elements (the order of the group) are related by

r

d2

= g .

(D.1.20)

μ

 

 

μ=1

The matrix elements of the matrices irreducible representations D(μ)

D(μ) and D(ν) belonging to the unitary satisfy the orthogonality relation

Dij(μ) (R)Dkl(ν)(R) = g δik δjlδμν ,

(D.1.21)

RG dμ

where dμ is the dimension of the μth irreducible representation.

This implies the following formula for the characters of unitary irreducible

representations:

 

χ(μ) (R)χ(ν)(R) = μν .

(D.1.22)

RG