5.1
Orbital angular momentum operators
Carry the classical L = r × p into quantum mechanics and the three components refuse to commute with each other — and that single fact determines everything about it.
Recommended first
After this section you should be able to
- Write down the three component operators of L̂ and explain why they have no ordering ambiguity
- Derive [L̂ₓ, L̂ᵧ] = iħL̂_z in full and state what it means for measuring components simultaneously
- Verify that L² commutes with any one component, and explain why the standard choice is (L², L_z)
- Explain what is meant by saying that the commutation relations themselves define angular momentum
Every problem we have solved so far has been one-dimensional: a particle moving along a line. But real atoms are three-dimensional — the electron orbits the nucleus. And the moment anything “goes around”, classical mechanics hands us a leading character: angular momentum.
First, why does it matter classically? A planet around the Sun, an electron around a nucleus — these are central-force problems: the force always points at the centre. In that situation is conserved — its direction locks the orbital plane in place, and its magnitude sets how “fat” or “thin” the orbit is. Kepler’s second law (equal areas in equal times) is nothing but angular momentum conservation in disguise.
Meanwhile, experiment had long been hinting that angular momentum in atoms is not continuous. Put a glowing atom in a magnetic field and its spectral lines split into a finite number of components (the Zeeman effect), as if angular momentum could only point in a few discrete directions in space. The Bohr model simply postulated — the specific values later turned out to be wrong, but the intuition of “quantised angular momentum” was pointing exactly the right way.
This chapter answers the questions: what does angular momentum actually look like in quantum mechanics, which values can it take, and why does it drag in something with no classical counterpart whatsoever — spin.
From classical quantity to operator
The postulates of chapter 3 give us the recipe for building operators: take the classical expression and replace and by operators. For angular momentum:
The three formulas are really one formula: cycle and each line turns into the next.
The key calculation: do the components commute?
The lesson of section 3.6 was that whether two observables can be simultaneously sharp is decided entirely by their commutator. So the first thing to do with three new operators is to compute their commutators.
Computing [L̂ₓ, L̂ᵧ]basic~6 min
Goal: .
Step 1: expand into four terms. The commutator is linear in both slots, so
Step 2: throw away the trivial terms first. The operators appearing in the second term are — every pair among them commutes (coordinates and momenta along different directions leave each other alone), so the whole term vanishes. The third term contains and dies for the same reason. Only the first and fourth terms survive.
Step 3: the first term. Grinding through the product rule for would be tedious. Better to notice that the only pair with any “spark” here is and (); every other operator is a bystander. Pull the bystanders out front:
(Using .)
Step 4: the fourth term. Here the sparking pair is and :
Step 5: put it together.
Cycling immediately yields the other two. All three together:
The result is not zero. That one small line of algebra has enormous consequences.
The picture
Intuition: the angular momentum vector cannot be pinned down.
Classical angular momentum is an honest arrow: all three components have definite values at once, and the arrow points in a definite direction.
Quantum angular momentum cannot manage that. says that and generally cannot both be sharp: nail down , and and dissolve into a cloud of probabilities.
The right picture is not an arrow but a cone: is definite (the cone’s height is fixed), the length is definite (the cone’s slant is fixed), but on the surface of the cone the arrow is “everywhere and nowhere”.
The mathematics
Formula: a direct application of the generalised uncertainty relation.
Apply the generalised uncertainty relation of section 3.6, , to this pair:
Note that the right-hand side is an expectation value, not a constant: unlike , this bound changes from state to state. In a state with , and are allowed to vanish simultaneously — for instance a spherically symmetric state with zero angular momentum altogether.
Is anything simultaneously sharp?
The three components fight each other — so is there any quantity that lives at peace with them? There is: the squared magnitude of the angular momentum,
Verifying [L², L̂_z] = 0basic~4 min
Work term by term. First a small general-purpose tool (the product rule):
First term : using ,
Second term : using ,
Third term (any operator commutes with its own powers).
Add the three: the first two are equal and opposite and cancel exactly:
By symmetry (the three directions enter on an equal footing), commutes with and as well.
So the largest combination quantum mechanics lets us fix simultaneously is: the length plus one component. The conventional choice is — there is nothing physically special about ; it is pure notational tradition (in a real experiment, “the direction” is simply wherever your magnetic field points). This is the algebraic origin of the cone picture: the slant of the cone () and its height () can be fixed together; the azimuthal angle cannot.
Why the commutator can determine the spectrum
The natural next question: what are the eigenvalues of and ?
The chapter-2 approach would be to write down a differential equation and solve it. But here there is an astonishing shortcut: from the commutation relations alone, without solving a single differential equation, every eigenvalue can be pinned down.
We have already seen the seed of the idea: in the algebraic solution of the harmonic oscillator, the single commutation relation forces the levels into an evenly spaced ladder of — the commutator sets the rung spacing, positivity sets the bottom, and the spectrum is locked in. The angular momentum algebra is more intricate (the right-hand side is an operator, not a constant), but the same strategy works: build “ladder operators” that climb the eigenvalues one rung at a time, then use the finiteness of to cap the ladder at both ends.
Key formulas
Angular momentum operators
Coordinates and momenta in each term point along different directions: no ordering ambiguity, automatically Hermitian
Fundamental commutation relations
The true definition of angular momentum; anything satisfying it qualifies
Uncertainty relation
The bound depends on the state; when ⟨L_z⟩ = 0 both may vanish together
Compatible partners
Length plus one component can be fixed together; conventionally (L², L_z)
Self-check4 questions
- 1.
Why is there no operator-ordering ambiguity in the construction L̂_z = x̂p̂_y − ŷp̂_x?
- 2.
Which statements about σ_{L_x}σ_{L_y} ≥ (ħ/2)|⟨L̂_z⟩| are correct? (Select all that apply.)
Select all that apply
- 3.
If the three components refuse to commute with one another, why can L̂² and L̂_z still be used together as labels?
- 4.
A state has L̂² eigenvalue 6ħ² (next section: this corresponds to l = 2). What is the magnitude |L| in units of ħ? (Give three decimal places.)
ħ1% relative tolerance
What comes next
We have placed our bet on the commutation relations: the claim is that
alone determine every eigenvalue of and .
The next section makes good on that promise — climbing out the entire spectrum rung by rung with ladder operators. And the answer hides a surprise: the algebra allows half again as many eigenvalues as orbital motion actually uses. That extra half is the seat reserved for spin.
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