Nothing here is solved. Four wave functions are written down and checked, and the checking is what establishes which shapes go with which quantum numbers.
Β§8.1 asserted the fuzzy-vector rules and Β§8.2 showed they are real. Neither said what any of it has to do with a wave function. This section closes that gap, and it does so in an unusually concrete way: rather than solving an equation, Phillips writes down four simple wave functions and applies the operators to them, reading off the angular momentum properties by inspection.
Classical first
For a particle at with momentum , the orbital angular momentum about the origin is
with components , , and magnitude .
The quantum operator
Replace by and you have the operator:
a vector operator with three components:
When is known, expectation values follow the usual recipe: and . And if happens to be an eigenfunction, , then Β§4.3βs argument gives and , so
β the state has a precise component. This is the machinery; the rest of the section is four examples.
Four wave functions, worked by inspection
The bookβs strategy is worth naming, because it is unusual. Instead of solving an eigenvalue equation, it guesses four wave functions with simple angular dependence and applies the operators to see what comes out:
where is any well-behaved function of . The labels and are given in advance; the point of the section is to earn them.
The other two, and a warning about z
Replacing by or in gives
Both still have ; but has with and uncertain, and has with and uncertain.
Finally, the two complex ones. Applying the operators to gives
so both have with β same magnitude, opposite component β and neither is an eigenfunction of or .
What the shapes look like
A particle with definite angular momentum has a wave function with a definite angular shape, and the probability density on a sphere is β the bookβs Figs. 8.4, 8.6 and 8.7. They are the same picture at , so here they are as one object:
m = 0 gives the most nodal circles β 1 of them, the maximum for this l. With no angular momentum about z, the density is free to pile up at the poles. Note there is no dependence on Ο, whatever l and m β because |eimΟ|Β² = 1. A definite Lz means the wave function is completely smeared around the z axis.
Three properties, now earned
The section closes by collecting what these examples have shown:
- Orbital angular momentum is quantized, with J s as the natural unit. Every eigenvalue found above was , or β never anything in between.
- It is at best a fuzzy vector fuzzy vector The chapter's name for a quantum angular momentum: an object with a definite magnitude and a definite value for exactly one Cartesian component, the other two being uncertain but quantized when measured. The classical picture of a vector pointing in a definite direction has no quantum counterpart. defined in ch. 8 β open in glossary . In every example, only the magnitude and one component could be specified β because the components are non-compatible observables in the sense of chapter 7.
- Definite angular momentum means a definite angular shape. Zero angular momentum gives a spherically symmetric wave function; non-zero gives angular dependence.
Check yourself
0 / 6 answered
1.Why does every spherically symmetric wave function have zero orbital angular momentum?
2. has and . What does that combination describe?
3.Why is independent of the azimuthal angle for every one of these states?
In the widget, hold l = 3 and step |m| from 0 up to 3.
4.What happens to the nodal circles, and why?
5.Eq. (8.22) gives and alongside . What is the point of writing them down?
6.What has this section established, and what has it not?