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Summary of Angular Momentum
We start from the classical expression for angular momentum,
, to obtain the quantum mechanical version
, where
,
, and
are all three-dimensional vectors. This definition
leads immediately to expressions for the three components of
:
From these definitions, we may easily derive the following commutators
where the indices
can be
,
, or
, and where the coefficient
is unity if
form a cyclic permutation of
[i.e., (
), (
), or (
)] and -1 for a reverse
cyclic permutation [(
), (
), or (
)]. The final
commutator indicates that we cannot generally know
,
, and
simultaneously except if we have an eigenstate with eigenvalue 0 for each
of these.
Classically, any component of the angular momentum must be less than or
equal to the
magnitude of the overall angular momentum vector. Quantum mechanically,
the average value of any component of the angular momentum must be
less than or equal to the square root of the expectation value of
dotted with itself:
 |
(7) |
is simply
.
Since
commutes with any component
, we can have simultaneous eigenfunctions of
and a given component
. We usually pick the
axis, since the expression for
is the easiest of the three when we work in spherical polar
coordinates:
Of course it is also possible to express
in terms of the unit
vectors for spherical polar coordinates,
Here,
 |
(14) |
and
The simultaneous eigenfunctions of
and
are
called the spherical harmonics,
, where
is the total angular momentum quantum number, and
is the so-called
magnetic quantum number. The spherical harmonics are defined as
 |
(16) |
where
are the associated Legendre polynomials. We require
that
, and spherical harmonics with
are defined in
terms of the spherical harmonics with
according to
. The spherical harmonics are normalized over integration of
angular coordinates such that
![\begin{displaymath}
\int_0^{\pi} sin \theta \hspace{0.1cm} d\theta \int_0^{2 \pi...
... \phi)]^* Y_l^m(\theta, \phi) =
\delta_{l,l'} \delta_{m, m'},
\end{displaymath}](img62.png) |
(17) |
and they have the following special
properties:
It can be useful to define ladder operators for angular momentum. The
following ladder operators work not only for straight angular momentum
, but also for combined angular momenta such as
. If
 |
(20) |
then
![\begin{displaymath}
{\bf\hat J}_{\pm} \vert jm \rangle =
\hbar \left[ (j \mp m)(j \pm m + 1) \right]^{1/2} \vert j, m \pm 1 \rangle .
\end{displaymath}](img69.png) |
(21) |
We can see that these ladder operators raise or lower the magnetic quantum
number
but leave
alone.
One can also show that in spherical polar coordinates
![\begin{displaymath}
{\bf\hat L}^2 = - \hbar^2 \left[
\frac{1}{sin^2 \theta} \fr...
...pace{0.1cm} \frac{\partial}{\partial \theta}
\right) \right].
\end{displaymath}](img70.png) |
(22) |
By comparing this expression with that for
in spherical polar
coordinates,
 |
|
|
(23) |
we can see that the Hamiltonian can be written as
Clearly
commutes with the kinetic energy term,
has no
dependence. Likewise, if
, then
commutes with the whole Hamiltonian. Hence, for problems where
the potential depends only on
(central force problems), we can find
simultaneous eigenfunctions of
,
, and
.
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David Sherrill
2006-02-23