Title: Angular-Momentum Theory
1Angular-Momentum Theory
- M. Auzinsh
- D. Budker
- S. Rochester
- Optically polarized atoms understanding
light-atom interactions - Ch. 3
2Rotations
- Classical rotations
- Commutation relations
- Quantum rotations
- Finding U (R )?
- D functions?
- Visualization
- Irreducible tensors
- Polarization moments
3Classical rotations
Rotations use a 3x3 matrix R
position or other vector
Rotation by angle ? about z axis
For ?p/2
For small angles
For arbitrary axis
Ji are generators of infinitesimal rotations
4Commutation relations
Rotate green around x, blue around y
From picture
Rotate blue around x, green around y
For any two axes
Using
Difference is a rotation around z
5Quantum rotations
- Want to find U (R) that corresponds to R
U(R) should be unitary, and should rotate various
objects as we expect
E.g., expectation value of vector operator
Remember, for spin ½, U is a 2x2 matrix A is a
3-vector of 2x2 matrices R is a 3x3 matrix
6Quantum rotations
Like classical formula, except
i makes J Hermitian
For small ?
? gives J units of angular momentum
minus sign is conventional
- The Ji are the generators of infinitesimal
rotations - They are the QM angular momentum operators.
- This is the most general definition for J
We can recover arbitrary rotation
7Quantum rotations
Start by demanding that U(R)? satisfies same
commutation relations as R
The commutation relations specify J, and thus
U(R)?
That's it!
E.g., for spin ½
8Quantum rotations
We've specified U(R), but does it do what we want?
Want to check
J is an observable, so check
Do easy case infinitesimal rotation around z
Neglect d2 term
Same Rz matrix as before
9D -functions
Matrix elements of the rotation operator
Rotations do not change j .
D-function
z-rotations are simple
so we use Euler angles (z-y-z)