Β§8.3aOrbital Angular Momentum: Operators and Angular Shape

Part V Phillips pp. 163–169 Β· ~15 min read

  • fuzzy vector

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 r=(x,y,z)\mathbf r = (x,y,z) with momentum p=(px,py,pz)\mathbf p = (p_x,p_y,p_z), the orbital angular momentum about the origin is

L=rΓ—p\mathbf L = \mathbf r \times \mathbf p

with components Lx=ypzβˆ’zpyL_x = yp_z - zp_y, Ly=zpxβˆ’xpzL_y = zp_x - xp_z, Lz=xpyβˆ’ypxL_z = xp_y - yp_x and magnitude ∣L∣=Lx2+Ly2+Lz2|\mathbf L| = \sqrt{L_x^2 + L_y^2 + L_z^2}.

The quantum operator

Replace p\mathbf p by p^=βˆ’iβ„βˆ‡\hat{\mathbf p} = -i\hbar\nabla and you have the operator:

L^=r^Γ—p^=βˆ’iℏ rΓ—βˆ‡(8.17)\hat{\mathbf L} = \hat{\mathbf r}\times\hat{\mathbf p} = -i\hbar\,\mathbf r\times\nabla\tag{8.17}

a vector operator with three components:

L^x=βˆ’iℏ(yβˆ‚βˆ‚zβˆ’zβˆ‚βˆ‚y),L^y=βˆ’iℏ(zβˆ‚βˆ‚xβˆ’xβˆ‚βˆ‚z)\hat L_x = -i\hbar\left(y\frac{\partial}{\partial z} - z\frac{\partial}{\partial y}\right),\qquad \hat L_y = -i\hbar\left(z\frac{\partial}{\partial x} - x\frac{\partial}{\partial z}\right) L^z=βˆ’iℏ(xβˆ‚βˆ‚yβˆ’yβˆ‚βˆ‚x)\hat L_z = -i\hbar\left(x\frac{\partial}{\partial y} - y\frac{\partial}{\partial x}\right)

Equation (8.17) β€” a vector whose components are three separate operators

symbol
is
NOT one operator but three, packaged as a vector. There is no single "angular momentum operator" whose eigenvalue is the vector β€” which is exactly why the direction has no value and Β§8.1 had to call it a fuzzy vector.
units
type
three operators in a trench coat

Click any symbol to see what it is, what units it carries, and what kind of object it is once you put it in an array.

When Ξ¨\Psi is known, expectation values follow the usual recipe: ⟨Lx⟩=βˆ«Ξ¨βˆ—L^xΨ d3r\langle L_x\rangle = \int\Psi^*\hat L_x\Psi\,\mathrm d^3\mathbf r and ⟨Lx2⟩=βˆ«Ξ¨βˆ—L^x2Ψ d3r\langle L_x^2\rangle = \int\Psi^*\hat L_x^2\Psi\,\mathrm d^3\mathbf r. And if Ξ¨\Psi happens to be an eigenfunction, L^xΞ¨=LxΞ¨\hat L_x\Psi = L_x\Psi, then Β§4.3’s argument gives ⟨Lx⟩=Lx\langle L_x\rangle = L_x and ⟨Lx2⟩=Lx2\langle L_x^2\rangle = L_x^2, so

Ξ”Lx=⟨Lx2βŸ©βˆ’βŸ¨Lx⟩2=0\Delta L_x = \sqrt{\langle L_x^2\rangle - \langle L_x\rangle^2} = 0

β€” the state has a precise xx component. This is the machinery; the rest of the section is four examples.

Four wave functions, worked by inspection

The book’s 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:

ψ(0,0)=R(r)(8.18)\psi_{(0,0)} = R(r)\tag{8.18} ψ(1,0)=R(r)zr,ψ(1,1)=R(r)(x+iy)r,ψ(1,βˆ’1)=R(r)(xβˆ’iy)r(8.19)\psi_{(1,0)} = R(r)\frac{z}{r},\qquad \psi_{(1,1)} = R(r)\frac{(x+iy)}{r},\qquad \psi_{(1,-1)} = R(r)\frac{(x-iy)}{r}\tag{8.19}

where R(r)R(r) is any well-behaved function of r=x2+y2+z2r = \sqrt{x^2+y^2+z^2}. The labels (0,0)(0,0) and (1,Β±1)(1,\pm1) are given in advance; the point of the section is to earn them.

ψ(0,0) = R(r): why every spherically symmetric state has zero angular momentum

step 1 of 4

No eigenvalue equation is solved here. The whole result follows from one geometric fact about the cross product.

  1. 1Start from Eq. (8.17) in the form that exposes the geometry, rather than from the three Cartesian components.

The other two, and a warning about z

Replacing zz by xx or yy in ψ(1,0)\psi_{(1,0)} gives

ψ(1,0)β€²=R(r)xrandψ(1,0)β€²β€²=R(r)yr(8.22)\psi'_{(1,0)} = R(r)\frac{x}{r}\qquad\text{and}\qquad \psi''_{(1,0)} = R(r)\frac{y}{r}\tag{8.22}

Both still have ∣L∣=2 ℏ|L| = \sqrt2\,\hbar; but Οˆβ€²\psi' has Lx=0L_x = 0 with LyL_y and LzL_z uncertain, and Οˆβ€²β€²\psi'' has Ly=0L_y = 0 with LzL_z and LxL_x uncertain.

Finally, the two complex ones. Applying the operators to xΒ±iyx \pm iy gives

L^zψ(1,Β±1)=Β±β„β€‰Οˆ(1,Β±1)andL^2ψ(1,Β±1)=2ℏ2ψ(1,Β±1)\hat L_z\psi_{(1,\pm1)} = \pm\hbar\,\psi_{(1,\pm1)} \qquad\text{and}\qquad \hat L^2\psi_{(1,\pm1)} = 2\hbar^2\psi_{(1,\pm1)}

so both have l=1l = 1 with ml=Β±1m_l = \pm1 β€” same magnitude, opposite zz component β€” and neither is an eigenfunction of L^x\hat L_x or L^y\hat L_y.

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 ∣Yl,ml∣2|Y_{l,m_l}|^2 β€” the book’s Figs. 8.4, 8.6 and 8.7. They are the same picture at l=1,2,3l = 1, 2, 3, so here they are as one object:

Angular shapes: |Yl,m(ΞΈ,Ο†)|Β² for l ≀ 3
z
state 3p, n_r = 1
⟨r⟩ = 12.50 aβ‚€, peak at 12.01 aβ‚€
nodes: 1 angular, 1 radial

m = 0 gives the most nodal circles — 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 φ, whatever l and m — because |eimφ|² = 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 ℏ=1.055Γ—10βˆ’34\hbar = 1.055\times10^{-34} J s as the natural unit. Every eigenvalue found above was 00, ±ℏ\pm\hbar or 2ℏ22\hbar^2 β€” never anything in between.
  • It is at best a fuzzy vector . 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. 1.Why does every spherically symmetric wave function have zero orbital angular momentum?

  2. 2. has and . What does that combination describe?

  3. 3.Why is independent of the azimuthal angle for every one of these states?

  4. In the widget, hold l = 3 and step |m| from 0 up to 3.

    4.What happens to the nodal circles, and why?

  5. 5.Eq. (8.22) gives and alongside . What is the point of writing them down?

  6. 6.What has this section established, and what has it not?