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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.

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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 L=r×p\vec L=\vec r\times\vec p 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 L=nL=n\hbar — 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 xx and pp by operators. For angular momentum:

L^=r^×p^L^x=y^p^zz^p^yL^y=z^p^xx^p^zL^z=x^p^yy^p^x\hat{\vec L}=\hat{\vec r}\times\hat{\vec p} \quad\Longrightarrow\quad \begin{aligned} \hat L_x&=\hat y\hat p_z-\hat z\hat p_y\\ \hat L_y&=\hat z\hat p_x-\hat x\hat p_z\\ \hat L_z&=\hat x\hat p_y-\hat y\hat p_x \end{aligned}

The three formulas are really one formula: cycle xyzxx\to y\to z\to x 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.

The result is not zero. That one small line of algebra has enormous consequences.

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,

L^2L^x2+L^y2+L^z2(5.1.7)\hat L^2\equiv\hat L_x^2+\hat L_y^2+\hat L_z^2\tag{5.1.7}

So the largest combination quantum mechanics lets us fix simultaneously is: the length plus one component. The conventional choice is (L^2,L^z)(\hat L^2,\hat L_z) — there is nothing physically special about zz; it is pure notational tradition (in a real experiment, “the zz direction” is simply wherever your magnetic field points). This is the algebraic origin of the cone picture: the slant of the cone (L|\vec L|) and its height (LzL_z) can be fixed together; the azimuthal angle cannot.

Why the commutator can determine the spectrum

The natural next question: what are the eigenvalues of L^2\hat L^2 and L^z\hat L_z?

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 [a^,a^]=1[\hat a,\hat a^\dagger]=1 forces the levels into an evenly spaced ladder of ω\hbar\omega — 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” L^x±iL^y\hat L_x\pm\ii\hat L_y that climb the LzL_z eigenvalues one rung at a time, then use the finiteness of L^2\hat L^2 to cap the ladder at both ends.

What comes next

We have placed our bet on the commutation relations: the claim is that

[L^x,L^y]=iL^z and its cyclic partners(5.1.13)[\hat L_x,\hat L_y]=\ii\hbar\hat L_z\ \text{and its cyclic partners}\tag{5.1.13}

alone determine every eigenvalue of L^2\hat L^2 and L^z\hat L_z.

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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