5.2
Angular momentum eigenvalues and spherical harmonics
Climb out every angular momentum eigenvalue from the commutation relations alone, without solving a single differential equation; then return to the sphere to see what the eigenstates look like.
Recommended first
After this section you should be able to
- Derive the eigenvalues l(l+1)ħ² and mħ of L² and L_z in full using the ladder-operator method
- Explain why l can only be an integer or half-integer, and why orbital angular momentum keeps only the integers
- Write down the first few spherical harmonics and read their node structure and shapes
- Compute the coefficients produced when L± acts on |l, m⟩
The previous section placed a bet: the commutation relations (and their cyclic partners) alone can determine every eigenvalue. This section pays it off. The whole argument uses just three ingredients: the commutation relations, the Hermiticity of the operators, and the plain truth that “a squared length cannot be negative”.
Building the ladder
The lesson of the harmonic oscillator: to “hop rungs” among the eigenvalues, you need an operator whose commutator with is proportional to itself — then acting with on an eigenstate produces another eigenstate, with the eigenvalue shifted by one rung. Try this combination:
They are not Hermitian () and represent no observable — they are tools, not objects of study. Compute the two key commutators (both expand directly from the fundamental relations):
The first line says: raises the eigenvalue by and lowers it by — that is the ladder. The second line says: while you climb, the eigenvalue of does not budge — the ladder stands on a cone of fixed length.
Climbing out the full spectrum
The spectrum by pure algebra: from commutators to l(l+1)ħ²advanced~12 min
Set up notation. Let be a joint eigenstate:
(Factoring out makes and pure numbers. At this point we know nothing about either.)
Step 1: check that the ladder really climbs. Ask what is an eigenstate of:
So is either the zero vector or an eigenstate with . Likewise gives . And guarantees stays put.
Step 2: the ladder must have a top. The crucial physical input: a component cannot exceed the total length. Precisely,
The last step holds because the expectation of is , a squared length, hence non-negative. So : is trapped in a finite interval and the ladder cannot climb forever. There must be a top rung with
(Not “acts and survives” but outright annihilated — that is the only way a ladder can terminate.)
Step 3: solve for λ from the top-rung condition. We need an identity, obtained by direct expansion:
Apply it to the top-rung state: the left side is zero, and the right side gives
Step 4: treat the bottom the same way. With , the identity gives
Setting the two expressions equal: . Read as a quadratic in , the two roots are and . The latter is absurd (a bottom above the top), so
The ladder is symmetric about zero.
Step 5: integers or half-integers? Climbing from bottom to top in steps of takes some whole number of steps :
Conclusion. Writing (the conventional symbol):
where is a non-negative integer or half-integer, and runs from to one rung at a time — values in all. Not one differential equation solved, and the whole spectrum is in hand.
While we are at it, fix the ladder-operator coefficients (we will need them for building matrices and for Clebsch–Gordan coefficients). From the identity above, ; with the positive-real phase convention:
Substitute and the square root vanishes on the spot — the formula seals the top and bottom of the ladder all by itself.
Back to the sphere: orbital angular momentum drops half the values
The algebra allows half-integer . But orbital angular momentum — the kind genuinely built from — realises only the integer half. The reason lives in the wavefunction. In spherical coordinates (with the angle from the z axis and the azimuthal angle around it), takes a remarkably clean form:
Its eigenfunctions are . Now the decisive blow: and are the same point in space, and a wavefunction must have a single value at a single point:
Were , the wavefunction would change sign after one full turn — two values at the same point, which no function on space is allowed to do. So orbital angular momentum has only . The half-integer seats stand empty: the algebra plainly permits them, but a position wavefunction cannot accommodate them. Hold on to this loose end — next section it finds its owner.
Spherical harmonics: what the eigenstates look like
The joint eigenfunctions of depend only on the angles. Written , they are the spherical harmonics — “harmonics on the sphere”, playing the role that and play on a line. The construction copies the algebra: the top-rung condition is a first-order differential equation with solution , and walks you down from there. The first few:
The picture
How to read the shapes.
(the s states of chemistry): is constant — the probability is perfectly uniform over all directions, a round ball. No angular momentum means no “rotation axis” available to break spherical symmetry, which makes perfect sense.
(p states): is a dumbbell along the z axis — means no rotation about z, the angular momentum lies sideways, and the particle prefers the poles; is a doughnut around the equator — full-speed rotation about z, with the particle concentrated at the equator. The general rule: the closer is to , the more the distribution hugs the equatorial plane; hugs the z axis instead — just like a classical spinning top: whatever axis you spin about, the mass flings out into the plane perpendicular to it.
The mathematics
Node structure and basic properties.
has nodal lines (curves where the function vanishes) on the sphere: of them run along meridians, from the oscillation of the real/imaginary parts of , and run along circles of latitude, from the zeros of the part. counts the total nodal lines, counts the windings around the axis — the direct heir of the one-dimensional “number of nodes = n − 1” rule.
Orthonormality and completeness:
Any well-behaved function on the sphere can be expanded in the — they are to the sphere what plane waves are to the line.
Key formulas
Eigenvalue spectrum
A purely algebraic result; m = −l, …, +l gives 2l+1 values
Ladder operators
The coefficient vanishes at m = ±l: the ladder caps itself at both ends
Key identity
The engine of the spectrum derivation; also yields the ladder coefficients
Orbital angular momentum: integers only
Single-valuedness of the wavefunction excludes half-integers; those seats are reserved for spin
Spherical harmonics (l=1)
m=0 is a dumbbell along the axis, |m|=1 a doughnut at the equator
Self-check4 questions
- 1.
In the ladder-operator derivation, what is the physical basis for "the ladder must have a top"?
- 2.
Why can orbital angular momentum not have l = 1/2, even though the algebra allows it?
- 3.
Acting with L̂_+ on |l=1, m=0⟩ gives ħ·c·|1,1⟩. What is the coefficient c?
- 4.
A beam of particles is in an l = 3 state. At most how many distinct outcomes can a measurement of L_z give?
outcomes0% relative tolerance
What comes next
The algebra allows , yet wavefunctions on the sphere cannot house them. Mathematics reserved the seats; space cannot fill them — so were those seats reserved for nothing?
In 1922, two German physicists fired a beam of silver atoms through an inhomogeneous magnetic field and found two separated traces on a glass plate — precisely the value of at . The half-integer seat has an owner, and the angular momentum it carries has nothing to do with motion through space.
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