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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
|
(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
|
(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
|
(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