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Copyright by Kirsten Viering 2006 - Raizen Lab - The University of ...

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Appendix A<br />

Wigner-Eckart <strong>The</strong>orem<br />

When dealing with different angular momenta, their couplings, and transition proba-<br />

bilities, it can be very helpful to use the Wigner-Eckart <strong>The</strong>orem. It allows a separation<br />

<strong>of</strong> a matrix element 〈α ′ j ′ m ′ |T(k, q)|αjm〉 into a scalar matrix element (reduced matrix<br />

element) 〈α ′ j ′ ||T k ||αj〉, which carries the information about the dynamics <strong>of</strong> the system,<br />

and a Wigner-3j-symbol (Clebsch-Gordan coefficient), that carries the geometrical and<br />

symmetrical properties. <strong>The</strong> Wigner-3j-symbol therefore includes the selection rules<br />

for radiative transitions.<br />

We will follow the pro<strong>of</strong>s given <strong>by</strong> Zare [12] and Edmonds [32] and consider<br />

first a rotation <strong>of</strong> the state vector T(k, q)|α ′ j ′ m ′ 〉,<br />

R [T(k, q) |α ′ j ′ m ′ 〉] = R T(k, q) R −1 R |α ′ j ′ m ′ =<br />

〉<br />

<br />

q ′ ,m ′′<br />

D k q ′ q (R) Dj′<br />

m ′′ m ′(R) [T(k, q ′ )|α ′ j ′ m ′′ 〉]<br />

=<br />

<br />

D k ⊗ D j′<br />

[T(k, q ′ )|α ′ j ′ m ′′ 〉, (A.1)<br />

q ′ ,m ′′<br />

where Dl m ′ m (R) are the Wigner rotation matrix elements. <strong>The</strong>se can be expressed <strong>by</strong><br />

spherical harmonics Y1,q<br />

D 1<br />

q,0 (r) = (−1)q<br />

1/2<br />

4π<br />

Y1,q(θ(r), φ(r)). (A.2)<br />

3<br />

51

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