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Atomic Structure Theory

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22 1 Angular Momentum<br />

1.5 Spinor and Vector Spherical Harmonics<br />

In constructing atomic wave functions, it is often necessary to combine the orbital<br />

wave functions given by spherical harmonics and the spin wave functions<br />

to obtain eigenfunctions of J = L + S. Similarly, when considering electromagnetic<br />

interactions, it is often necessary to combine the spin and orbital angular<br />

momentum components of the vector potential to obtain eigenfunctions<br />

of J 2 and Jz. Combining spin 1/2 eigenfunctions with spherical harmonics<br />

leads to spherical spinors, while combining spin 1 eigenfunctions with spherical<br />

harmonics leads to vector spherical harmonics. These combined spin-angle<br />

functions are discussed in the following two subsections.<br />

1.5.1 Spherical Spinors<br />

Spherical spinors, which are eigenstates of J 2 and Jz, are formed by combining<br />

spherical harmonics Ylm(θ, φ), which are eigenstates of L 2 and Lz, and<br />

spinors χµ, which are eigenstates of S 2 and Sz. We denote spherical spinors<br />

by Ωjlm(θ, φ); they are defined by the equation<br />

Ωjlm(θ, φ) = <br />

C(l, 1/2,j; m − µ, µ, m)Yl,m−µ(θ, φ)χµ . (1.115)<br />

µ<br />

Using the explicit forms of the Clebsch-Gordan coefficients given in Table 1.1,<br />

we obtain the following explicit formulas for spherical spinors having the two<br />

possible values, j = l ± 1/2:<br />

⎛ <br />

l+m+1/2<br />

Ωl+1/2,l,m(θ, φ) = ⎝ 2l+1 Yl,m−1/2(θ, φ)<br />

<br />

l−m+1/2<br />

2l+1 Y ⎞<br />

⎠ , (1.116)<br />

l,m+1/2(θ, φ)<br />

⎛<br />

Ωl−1/2,l,m(θ, φ) = ⎝ −<br />

<br />

l−m+1/2<br />

2l+1 Yl,m−1/2(θ, φ)<br />

<br />

l+m+1/2<br />

Y ⎞<br />

⎠ . (1.117)<br />

l,m+1/2(θ, φ)<br />

2l+1<br />

Spherical spinors are eigenfunctions of σ·L and, therefore, of the operator<br />

The eigenvalue equation for K is<br />

K = −1 − σ·L.<br />

KΩjlm(θ, φ) =κΩjlm(θ, φ) , (1.118)<br />

where the (integer) eigenvalues are κ = −l − 1forj = l +1/2, and κ = l<br />

for j = l − 1/2. These values can be summarized as κ = ∓(j +1/2) for<br />

j = l ± 1/2. The value of κ determines both j and l. Consequently, the more<br />

compact notation Ωκm ≡ Ωjlm can be used. The states associated with l and<br />

j are designated by the spectroscopic notation s 1/2, p 1/2, p 3/2, ... where the

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