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Next: Eigenvalues for the Orbital Up: Angular Momentum Previous: Introduction

Orbital AM

In classical mechanics, the AM of a particle (with respect to the origin) is given by the formula:

equation1825

so that,

eqnarray227

where tex2html_wrap_inline5011 and tex2html_wrap_inline5013 are the position and linear momentum vectors, respectively.

The mathematics of AM comes about through the quantum rule of replacing the linear momentum tex2html_wrap_inline5015 of a classical point particle, located at point r, by tex2html_wrap_inline5017 , thus replacing the classical angular momentum of a point particle (about the origin of some chosen Cartesian coordinate system), by the AM operator:

equation1827

This implies:

  eqnarray248

Equation (6) can be written more compactly as

  eqnarray1884

where tex2html_wrap_inline5019 component, tex2html_wrap_inline5021 component, tex2html_wrap_inline5023 component and we have used the Einstein summation convention (i.e. the expression is summed over repeated indices). tex2html_wrap_inline5025 is the completely antisymmetric tensor of the third rank (also called the Levi-Civita tensor)

displaymath292

Some useful identities that the tex2html_wrap_inline5025 satisfy are

equation1895

The antisymmetric nature of the tex2html_wrap_inline5025 means that

displaymath5035

The product of two of these tensors, when summed over a pair of indices (i.e. the indices are contracted) has the following useful properties

equation1897

equation1899

equation1901

which can be proved by expanding out the terms. We will use these results later to prove some AM operator identities, but familiarity with them will be useful in your future study of Special/General Relativity, Classical/Quantum Electrodynamics and Quantum Field Theory.

The quantal AM properties of a simple one-particle system are then to be inferred from the properties of these operators and their actions in the associated Hilbert space. In the following sections, we will deduce the eigenvalues and eigenfunctions of these operators. The components of the quantum mechanical AM operator satisfy the following commutation relations:

  eqnarray1903

or

  equation1926

Further identities include

  equation1937

  equation1948

truein


truein Problem : 1 Verify (15)-(17) by direct calculation.

Partial Solution Here is the proof for (15):

  equation1959

We use the following operator identity to expand out the right hand side of (18)

  eqnarray1979

Making the substitutions

  eqnarray2107

into (19) we have

  eqnarray2133

We now make use of the following operator identities

  equation2201

  equation2209

  equation2217

so that (18) reduces to

  eqnarray2225

Since tex2html_wrap_inline5037 etc. we find that

  eqnarray2257

Substituting (21) into (20) we have

  eqnarray2259

Note that in the last term of the above equation we have relabelled the indices tex2html_wrap_inline5039 and tex2html_wrap_inline5041 since these are dummy indices (remember, due to the summation convention, summing over repeated indices tex2html_wrap_inline5043 is the same as summing over repeated indices tex2html_wrap_inline5045 ). Equation (22) reduces to

  eqnarray2291

Since tex2html_wrap_inline5047 and tex2html_wrap_inline5049 we finally have the result we want to prove i.e.

  equation2320

Actually I have done the hardest part. The proof for the other identities is much easier! truein


truein

From these fundamental commutation relations, the entire theory of AM can be deduced. Evidently tex2html_wrap_inline5051 are incompatible observables so it will be futile to look for states that are simultaneous eigenfunctions of tex2html_wrap_inline5053 and tex2html_wrap_inline5055 . From the Generalised Uncertainty Principle we deduce that:

equation2346

On the other hand, the square of the total angular momentum, tex2html_wrap_inline5057 ,

equation2355

does commute with tex2html_wrap_inline5059 and tex2html_wrap_inline5061 . truein


truein Problem : 2 Show that:

equation2369

equation2375

equation2381

or more compactly,

equation2387

truein


truein Problem :3 Show that

truein


truein Problem :4

truein


truein
next up previous
Next: Eigenvalues for the Orbital Up: Angular Momentum Previous: Introduction

Gunaretnam Rajagopal
Tue Oct 15 17:55:22 BST 1996