Wigner D-matrix

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Short description: Irreducible representation of the rotation group SO

The Wigner D-matrix is a unitary matrix in an irreducible representation of the groups SU(2) and SO(3). It was introduced in 1927 by Eugene Wigner, and plays a fundamental role in the quantum mechanical theory of angular momentum. The complex conjugate of the D-matrix is an eigenfunction of the Hamiltonian of spherical and symmetric rigid rotors. The letter D stands for Darstellung, which means "representation" in German.

Definition of the Wigner D-matrix

Let Jx, Jy, Jz be generators of the Lie algebra of SU(2) and SO(3). In quantum mechanics, these three operators are the components of a vector operator known as angular momentum. Examples are the angular momentum of an electron in an atom, electronic spin, and the angular momentum of a rigid rotor.

In all cases, the three operators satisfy the following commutation relations,

[Jx,Jy]=iJz,[Jz,Jx]=iJy,[Jy,Jz]=iJx,

where i is the purely imaginary number and the Planck constant ħ has been set equal to one. The Casimir operator

J2=Jx2+Jy2+Jz2

commutes with all generators of the Lie algebra. Hence, it may be diagonalized together with Jz.

This defines the spherical basis used here. That is, there is a complete set of kets (i.e. orthonormal basis of joint eigenvectors labelled by quantum numbers that define the eigenvalues) with

J2|jm⟩=j(j+1)|jm⟩,Jz|jm⟩=m|jm⟩,

where j = 0, 1/2, 1, 3/2, 2, ... for SU(2), and j = 0, 1, 2, ... for SO(3). In both cases, m = −j, −j + 1, ..., j.

A 3-dimensional rotation operator can be written as

ℛ(α,β,γ)=e−iαJze−iβJye−iγJz,

where α, β, γ are Euler angles (characterized by the keywords: z-y-z convention, right-handed frame, right-hand screw rule, active interpretation).

The Wigner D-matrix is a unitary square matrix of dimension 2j + 1 in this spherical basis with elements

Dm′mj(α,β,γ)≡⟨jm′|ℛ(α,β,γ)|jm⟩=e−im′αdm′mj(β)e−imγ,

where

dm′mj(β)=⟨jm′|e−iβJy|jm⟩=Dm′mj(0,β,0)

is an element of the orthogonal Wigner's (small) d-matrix (sometimes referred to as the reduced Wigner D-matrix).

That is, in this basis,

Dm′mj(α,0,0)=e−im′αδm′m

is diagonal, like the γ matrix factor, but unlike the above β factor.

Wigner (small) d-matrix

Wigner gave the following expression:[1]

dm′mj(β)=[(j+m′)!(j−m′)!(j+m)!(j−m)!]12∑s=sminsmax[(−1)m′−m+s(cos⁡β2)2j+m−m′−2s(sin⁡β2)m′−m+2s(j+m−s)!s!(m′−m+s)!(j−m′−s)!].

The sum over s is over such values that the factorials are nonnegative, i.e. smin=max(0,m−m′), smax=min(j+m,j−m′).

Note: The d-matrix elements defined here are real. In the often-used z-x-z convention of Euler angles, the factor (−1)m′−m+s in this formula is replaced by (−1)sim−m′, causing half of the functions to be purely imaginary. The realness of the d-matrix elements is one of the reasons that the z-y-z convention, used in this article, is usually preferred in quantum mechanical applications.

The d-matrix elements are related to Jacobi polynomials Pk(a,b)(cos⁡β) with nonnegative a and b.[2] Let

k=min⁡(j+m,j−m,j+m′,j−m′).

If

k={j+m:a=m′−m;λ=m′−mj−m:a=m−m′;λ=0j+m′:a=m−m′;λ=0j−m′:a=m′−m;λ=m′−m

Then, with b=2j−2k−a, the relation is

dm′mj(β)=(−1)λ(2j−kk+a)12(k+bb)−12(sin⁡β2)a(cos⁡β2)bPk(a,b)(cos⁡β),

where a,b≥0.

It is also useful to consider the relations a=|m′−m|,b=|m′+m|,λ=m−m′−|m−m′|2,k=j−M, where M=max⁡(|m|,|m′|) and N=min⁡(|m|,|m′|), which lead to:

dm′mj(β)=(−1)m−m′−|m−m′|2[(j+M)!(j−M)!(j+N)!(j−N)!]12(sin⁡β2)|m−m′|(cos⁡β2)|m+m′|Pj−M(|m−m′|,|m+m′|)(cos⁡β).

Properties of the Wigner D-matrix

The complex conjugate of the D-matrix satisfies a number of differential properties that can be formulated concisely by introducing the following operators with (x,y,z)=(1,2,3),

𝒥^1=i(cos⁡αcot⁡β∂∂α+sin⁡α∂∂β−cos⁡αsin⁡β∂∂γ)𝒥^2=i(sin⁡αcot⁡β∂∂α−cos⁡α∂∂β−sin⁡αsin⁡β∂∂γ)𝒥^3=−i∂∂α

which have quantum mechanical meaning: they are space-fixed rigid rotor angular momentum operators.

Further,

𝒫^1=i(cos⁡γsin⁡β∂∂α−sin⁡γ∂∂β−cot⁡βcos⁡γ∂∂γ)𝒫^2=i(−sin⁡γsin⁡β∂∂α−cos⁡γ∂∂β+cot⁡βsin⁡γ∂∂γ)𝒫^3=−i∂∂γ,

which have quantum mechanical meaning: they are body-fixed rigid rotor angular momentum operators.

The operators satisfy the commutation relations

[𝒥1,𝒥2]=i𝒥3,and[𝒫1,𝒫2]=−i𝒫3,

and the corresponding relations with the indices permuted cyclically. The 𝒫i satisfy anomalous commutation relations (have a minus sign on the right hand side).

The two sets mutually commute,

[𝒫i,𝒥j]=0,i,j=1,2,3,

and the total operators squared are equal,

𝒥2≡𝒥12+𝒥22+𝒥32=𝒫2≡𝒫12+𝒫22+𝒫32.

Their explicit form is,

𝒥2=𝒫2=−1sin2β(∂2∂α2+∂2∂γ2−2cos⁡β∂2∂α∂γ)−∂2∂β2−cot⁡β∂∂β.

The operators 𝒥i act on the first (row) index of the D-matrix,

𝒥3Dm′mj(α,β,γ)*=m′Dm′mj(α,β,γ)*(𝒥1±i𝒥2)Dm′mj(α,β,γ)*=j(j+1)−m′(m′±1)Dm′±1,mj(α,β,γ)*

The operators 𝒫i act on the second (column) index of the D-matrix,

𝒫3Dm′mj(α,β,γ)*=mDm′mj(α,β,γ)*,

and, because of the anomalous commutation relation the raising/lowering operators are defined with reversed signs,

(𝒫1∓i𝒫2)Dm′mj(α,β,γ)*=j(j+1)−m(m±1)Dm′,m±1j(α,β,γ)*.

Finally,

𝒥2Dm′mj(α,β,γ)*=𝒫2Dm′mj(α,β,γ)*=j(j+1)Dm′mj(α,β,γ)*.

In other words, the rows and columns of the (complex conjugate) Wigner D-matrix span irreducible representations of the isomorphic Lie algebras generated by {𝒥i} and {−𝒫i}.

An important property of the Wigner D-matrix follows from the commutation of ℛ(α,β,γ) with the time reversal operator T,

⟨jm′|ℛ(α,β,γ)|jm⟩=⟨jm′|T†ℛ(α,β,γ)T|jm⟩=(−1)m′−m⟨j,−m′|ℛ(α,β,γ)|j,−m⟩*,

or

Dm′mj(α,β,γ)=(−1)m′−mD−m′,−mj(α,β,γ)*.

Here, we used that T is anti-unitary (hence the complex conjugation after moving T† from ket to bra), T|jm⟩=(−1)j−m|j,−m⟩ and (−1)2j−m′−m=(−1)m′−m.

A further symmetry implies

(−1)m′−mDmm′j(α,β,γ)=Dm′mj(γ,β,α).

Orthogonality relations

The Wigner D-matrix elements Dmkj(α,β,γ) form a set of orthogonal functions of the Euler angles α,β, and γ:[3]

∫02πdα∫0πdβsin⁡β∫02πdγDm′k′j′(α,β,γ)∗Dmkj(α,β,γ)=8π22j+1δm′mδk′kδj′j.

This is a special case of the Schur orthogonality relations.

Crucially, by the Peter–Weyl theorem, they further form a complete set.

The fact that Dmkj(α,β,γ) are matrix elements of a unitary transformation from one spherical basis |lm⟩ to another ℛ(α,β,γ)|lm⟩ is represented by the relations:[4]

∑kDm′kj(α,β,γ)*Dmkj(α,β,γ)=δm,m′,
∑kDkm′j(α,β,γ)*Dkmj(α,β,γ)=δm,m′.

The group characters for SU(2) only depend on the rotation angle β, being class functions, so, then, independent of the axes of rotation,

χj(β)≡∑mDmmj(β)=∑mdmmj(β)=sin⁡((2j+1)β2)sin⁡(β2),

and consequently satisfy simpler orthogonality relations, through the Haar measure of the group,[5]

1π∫02πdβsin2(β2)χj(β)χj′(β)=δj′j.

The completeness relation is (cf. Eq. (3.95) in ref.,[5] or Eq. (4.10.7) in ref.[6])

∑jχj(β)χj(β′)=δ(β−β′),

whence, for β′=0,

∑jχj(β)(2j+1)=δ(β).

Kronecker product of Wigner D-matrices, Clebsch–Gordan series

The set of Kronecker product matrices

𝐃j(α,β,γ)⊗𝐃j′(α,β,γ)

forms a reducible matrix representation of the groups SO(3) and SU(2). Reduction into irreducible components is by the following equation:[4]

Dmkj(α,β,γ)Dm′k′j′(α,β,γ)=∑J=|j−j′|j+j′⟨jmj′m′|J(m+m′)⟩⟨jkj′k′|J(k+k′)⟩D(m+m′)(k+k′)J(α,β,γ)

The symbol ⟨j1m1j2m2|j3m3⟩ is a Clebsch–Gordan coefficient.

Relation to spherical harmonics and Legendre polynomials

For integer values of l, the D-matrix elements with second index equal to zero are proportional to spherical harmonics and associated Legendre polynomials, normalized to unity and with Condon and Shortley phase convention:

Dm0ℓ(α,β,γ)=4π2ℓ+1Yℓm*(β,α)=(ℓ−m)!(ℓ+m)!Pℓm(cos⁡β)e−imα.

This implies the following relationship for the d-matrix:

dm0ℓ(β)=(ℓ−m)!(ℓ+m)!Pℓm(cos⁡β).

A rotation of spherical harmonics ⟨θ,ϕ|ℓm′⟩ then is effectively a composition of two rotations,

∑m′=−ℓℓYℓm′(θ,ϕ)Dm′mℓ(α,β,γ).

When both indices are set to zero, the Wigner D-matrix elements are given by ordinary Legendre polynomials:

D0,0ℓ(α,β,γ)=d0,0ℓ(β)=Pℓ(cos⁡β).

In the present convention of Euler angles, α is a longitudinal angle and β is a colatitudinal angle (spherical polar angles in the physical definition of such angles). This is one of the reasons that the z-y-z convention is used frequently in molecular physics. From the time-reversal property of the Wigner D-matrix follows immediately

(Yℓm)*=(−1)mYℓ−m.

There exists a more general relationship to the spin-weighted spherical harmonics:

Dmsℓ(α,β,−γ)=(−1)s4π2ℓ+1sYℓm(β,α)eisγ.[7]

Connection with transition probability under rotations

The absolute square of an element of the D-matrix,

Fmm′(β)=|Dmm′j(α,β,γ)|2,

gives the probability that a system with spin j prepared in a state with spin projection m along some direction will be measured to have a spin projection m′ along a second direction at an angle β to the first direction. The set of quantities Fmm′ itself forms a real symmetric matrix, that depends only on the Euler angle β, as indicated.

Remarkably, the eigenvalue problem for the F matrix can be solved completely:[8][9]

∑m′=−jjFmm′(β)fℓj(m′)=Pℓ(cos⁡β)fℓj(m)(ℓ=0,1,…,2j).

Here, the eigenvector, fℓj(m), is a scaled and shifted discrete Chebyshev polynomial, and the corresponding eigenvalue, Pℓ(cos⁡β), is the Legendre polynomial.

Relation to Bessel functions

In the limit when ℓ≫m,m′, one obtains

Dmm′ℓ(α,β,γ)≈e−imα−im′γJm−m′(ℓβ)

where Jm−m′(ℓβ) is the Bessel function and ℓβ is finite.

List of d-matrix elements

Using sign convention of Wigner, et al. the d-matrix elements dm′mj(θ) for j = 1/2, 1, 3/2, and 2 are given below.

For j = 1/2

d12,1212=cos⁡θ2d12,−1212=−sin⁡θ2

For j = 1

d1,11=12(1+cos⁡θ)d1,01=−12sin⁡θd1,−11=12(1−cos⁡θ)d0,01=cos⁡θ

For j = 3/2

d32,3232=12(1+cos⁡θ)cos⁡θ2d32,1232=−32(1+cos⁡θ)sin⁡θ2d32,−1232=32(1−cos⁡θ)cos⁡θ2d32,−3232=−12(1−cos⁡θ)sin⁡θ2d12,1232=12(3cos⁡θ−1)cos⁡θ2d12,−1232=−12(3cos⁡θ+1)sin⁡θ2

For j = 2[10]

d2,22=14(1+cos⁡θ)2d2,12=−12sin⁡θ(1+cos⁡θ)d2,02=38sin2θd2,−12=−12sin⁡θ(1−cos⁡θ)d2,−22=14(1−cos⁡θ)2d1,12=12(2cos2θ+cos⁡θ−1)d1,02=−38sin⁡2θd1,−12=12(−2cos2θ+cos⁡θ+1)d0,02=12(3cos2θ−1)

Wigner d-matrix elements with swapped lower indices are found with the relation:

dm′,mj=(−1)m−m′dm,m′j=d−m,−m′j.

Symmetries and special cases

dm′,mj(π)=(−1)j−mδm′,−mdm′,mj(π−β)=(−1)j+m′dm′,−mj(β)dm′,mj(π+β)=(−1)j−mdm′,−mj(β)dm′,mj(2π+β)=(−1)2jdm′,mj(β)dm′,mj(−β)=dm,m′j(β)=(−1)m′−mdm′,mj(β)

See also

References

  1. ↑ Wigner, E. P. (1951). Gruppentheorie und ihre Anwendungen auf die Quantenmechanik der Atomspektren. Braunschweig: Vieweg Verlag. OCLC 602430512.  Translated into English by Group Theory and its Application to the Quantum Mechanics of Atomic Spectra. Elsevier. 2013. ISBN 978-1-4832-7576-5. https://books.google.com/books?id=UITNCgAAQBAJ&pg=PR9. 
  2. ↑ Biedenharn, L. C.; Louck, J. D. (1981). Angular Momentum in Quantum Physics. Reading: Addison-Wesley. ISBN 0-201-13507-8. 
  3. ↑ Van de Wiele, Jacques (2001). "Rotations et moments angulaires en mécanique quantique". Annales de Physique 26 (6): 1–169. doi:10.1051/anphys:200106001. Bibcode: 2001AnPh...26f...1V. https://hal.science/in2p3-00019832. 
  4. ↑ 4.0 4.1 Rose, Morris Edgar (1995). Elementary theory of angular momentum. Dover. ISBN 0-486-68480-6. OCLC 31374243. https://books.google.com/books?id=3lSiev-MnLQC&pg=PR7. 
  5. ↑ 5.0 5.1 Schwinger, J. (January 26, 1952). On Angular Momentum (Technical report). Harvard University, Nuclear Development Associates. doi:10.2172/4389568. OSTI 4389568. NYO-3071, TRN: US200506%%295.
  6. ↑ Varshalovich, D A; Moskalev, A N; Khersonskii, V K (October 1988) (in en). Quantum Theory of Angular Momentum. World Scientific. doi:10.1142/0270. ISBN 978-9971-5-0107-5. Bibcode: 1988qtam.book.....V. https://www.worldscientific.com/worldscibooks/10.1142/0270. 
  7. ↑ Shiraishi, M. (2013). "Appendix A: Spin-Weighted Spherical Harmonic Function" (PDF). Probing the Early Universe with the CMB Scalar, Vector and Tensor Bispectrum (PhD). Nagoya University. pp. 153–4. ISBN 978-4-431-54180-6.
  8. ↑ Meckler, A. (1958). "Majorana formula". Physical Review 111 (6): 1447. doi:10.1103/PhysRev.111.1447. Bibcode: 1958PhRv..111.1447M. 
  9. ↑ Mermin, N.D.; Schwarz, G.M. (1982). "Joint distributions and local realism in the higher-spin Einstein-Podolsky-Rosen experiment". Foundations of Physics 12 (2): 101. doi:10.1007/BF00736844. Bibcode: 1982FoPh...12..101M. 
  10. ↑ Edén, M. (2003). "Computer simulations in solid-state NMR. I. Spin dynamics theory". Concepts in Magnetic Resonance Part A 17A (1): 117–154. doi:10.1002/cmr.a.10061.