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# Eigenfunctions of Orbital Angular Momentum

In Cartesian coordinates, the three components of orbital angular momentum can be written

 (363) (364) (365)

using the Schrödinger representation. Transforming to standard spherical polar coordinates,

 (366) (367) (368)

we obtain

 (369) (370) (371)

Note that Equation (371) accords with Equation (346). The shift operators become

 (372)

Now,

 (373)

so

 (374)

The eigenvalue problem for takes the form

 (375)

where is the wavefunction, and is a number. Let us write

 (376)

Equation (375) reduces to

 (377)

where use has been made of Equation (374). As is well-known, square integrable solutions to this equation only exist when takes the values , where is an integer. These solutions are known as spherical harmonics, and can be written

 (378)

where is a positive integer lying in the range . Here, is an associated Legendre function satisfying the equation

 (379)

We define

 (380)

which allows to take the negative values . The spherical harmonics are orthogonal functions, and are properly normalized with respect to integration over the entire solid angle:

 (381)

The spherical harmonics also form a complete set for representing general functions of and .

By definition,

 (382)

where is an integer. It follows from Equations (371) and (378) that

 (383)

where is an integer lying in the range . Thus, the wavefunction , where is a general function, has all of the expected features of the wavefunction of a simultaneous eigenstate of and belonging to the quantum numbers and . The well-known formula

 (384)

can be combined with Equations (372) and (378) to give

 (385) (386)

These equations are equivalent to Equations (344)-(345). Note that a spherical harmonic wavefunction is symmetric about the -axis (i.e., independent of ) whenever , and is spherically symmetric whenever (since ).

In summary, by solving directly for the eigenfunctions of and in the Schrödinger representation, we have been able to reproduce all of the results of Section 4.2. Nevertheless, the results of Section 4.2 are more general than those obtained in this section, because they still apply when the quantum number takes on half-integer values.

Next: Motion in Central Field Up: Orbital Angular Momentum Previous: Rotation Operators
Richard Fitzpatrick 2013-04-08