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Angular Momentum

Classical rotation

Molecules tumble, and electrons circle nuclei. Lecture 4.1 found the rotational levels of HCl about 20 cm−1^{-1} apart, in the microwave, and Chapter 5 names the atomic orbitals s, p, d after their angular momentum. Angular momentum is the quantity that organizes all of this.

The simplest rotation, and the model system of this lecture, is a particle moving on a circle. This section describes it classically and defines the quantities of rotation along the way; the next section treats the same particle quantum mechanically. Appendix B covers the classical side in more depth.

Kinematics on a circle

Press play or move the slider. Drag the picture to turn it, and look “from above” to see ω⃗\vec{\omega} point straight out of the screen.

The particle goes counterclockwise around a circle of radius rr. The angle ϕ\phi grows, and the particle covers the arc s=rϕs = r\phi (teal). The angular velocity ω⃗\vec{\omega} points along the axis, and at every instant v⃗=ω⃗×r⃗\vec{v} = \vec{\omega}\times\vec{r} is perpendicular to r⃗\vec{r} (the right-angle mark) and to ω⃗\vec{\omega}, so it runs along the circle.

As vectors, the angular velocity ω⃗\vec{\omega} points along the rotation axis, with length ω\omega and direction set by the right-hand rule (fingers curl with the motion, the thumb gives ω⃗\vec{\omega}). The velocity is then a vector product, v⃗=ω⃗×r⃗\vec{v} = \vec{\omega}\times\vec{r}: perpendicular to both ω⃗\vec{\omega} and r⃗\vec{r}, so tangent to the circle, with length ωr\omega r.

Angular momentum is a vector product

Momentum p⃗=μv⃗\vec{p} = \mu\vec{v} measures straight-line motion. Its rotational partner is the angular momentum, built with the same vector product as ω⃗×r⃗\vec{\omega}\times\vec{r}, now of position and momentum:

L⃗=r⃗×p⃗=∣ı^ȷ^k^xyzpxpypz∣=(ypz−zpy)ı^+(zpx−xpz)ȷ^+(xpy−ypx)k^\vec{L} = \vec{r}\times\vec{p} = \begin{vmatrix} \hat{\imath} & \hat{\jmath} & \hat{k} \\ x & y & z \\ p_x & p_y & p_z \end{vmatrix} = \left(yp_z - zp_y\right)\hat{\imath} + \left(zp_x - xp_z\right)\hat{\jmath} + \left(xp_y - yp_x\right)\hat{k}
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Fig. A particle moving counterclockwise on a circle, seen from above at an angle. L⃗=r⃗×p⃗\vec{L} = \vec{r}\times\vec{p} is perpendicular to both r⃗\vec{r} and p⃗\vec{p}: it points along the rotation axis, by the right-hand rule.

L=rpsin⁡αlength of r⃗×p⃗=r μvcircle: α=90∘, p=μv=μr2ωv=rω=IωI=μr2\begin{aligned} L &= rp\sin\alpha && \text{length of } \vec{r}\times\vec{p} \\ &= r\,\mu v && \text{circle: } \alpha = 90^\circ,\ p = \mu v \\ &= \mu r^2\omega && v = r\omega \\ &= I\omega && I = \mu r^2 \end{aligned}

Kinetic energy in terms of LL

The energy of the particle is all kinetic. Rewrite it step by step in the quantities of rotation:

E=12μv2kinetic energy=12μr2ω2v=rω=12Iω2I=μr2=L22Iω=L/I\begin{aligned} E &= \tfrac{1}{2}\mu v^2 && \text{kinetic energy} \\ &= \tfrac{1}{2}\mu r^2\omega^2 && v = r\omega \\ &= \tfrac{1}{2}I\omega^2 && I = \mu r^2 \\ &= \frac{L^2}{2I} && \omega = L/I \end{aligned}

This has the same form as p2/2μp^2/2\mu for straight-line motion, with LL in place of the momentum and II in place of the mass, and it carries straight into quantum mechanics.

Linear and angular motion: the analogy

Every quantity of straight-line motion has a rotational partner:

straight linerotation
positionxxangle ϕ\phi
velocityv=dx/dtv = dx/dtangular velocity ω=dϕ/dt\omega = d\phi/dt
inertiamass μ\mumoment of inertia I=μr2I = \mu r^2
momentump=μvp = \mu vangular momentum L=IωL = I\omega
kinetic energyp2/2μp^2/2\muL2/2IL^2/2I
changed byforce, dp/dt=Fdp/dt = Ftorque, dL⃗/dt=r⃗×F⃗d\vec{L}/dt = \vec{r}\times\vec{F}
conserved whenno force actsno torque acts
quantum operatorp^=−iℏ d/dx\hat{p} = -i\hbar\,d/dxL^z=−iℏ d/dϕ\hat{L}_z = -i\hbar\,d/d\phi (next section)

A model system: the rigid dumbbell

A rigid dumbbell, such as a diatomic molecule turning with a fixed bond length, is the particle on a circle in disguise:

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Fig. Left: carbon monoxide as a rigid dumbbell, turning about its center of mass (+). Each atom moves on its own circle, with mCrC=mOrOm_Cr_C = m_Or_O. Right: the same motion as one particle of reduced mass μ\mu on a circle of radius r=rC+rOr = r_C + r_O, the bond length. Both have the same moment of inertia.

With rC=mOR/(mC+mO)r_C = m_OR/(m_C + m_O) and rO=mCR/(mC+mO)r_O = m_CR/(m_C + m_O),

I=mCrC2+mOrO2=mCmO2+mOmC2(mC+mO)2 r2=mCmOmC+mO r2=μr2I = m_Cr_C^2 + m_Or_O^2 = \frac{m_Cm_O^2 + m_Om_C^2}{(m_C + m_O)^2}\,r^2 = \frac{m_Cm_O}{m_C + m_O}\,r^2 = \mu r^2

the same reduced mass that turned a vibrating diatomic into one bead on a spring in Lecture 4.1. Everything in this lecture therefore applies to a rotating diatomic molecule, with I=μr2I = \mu r^2; in three dimensions (later) the dumbbell can also point in any direction.

No torque, no change: the spinning skater

Differentiate L⃗=r⃗×p⃗\vec{L} = \vec{r}\times\vec{p} with the product rule. The first term is v⃗×μv⃗=0\vec{v}\times\mu\vec{v} = 0, since the vector product of parallel vectors vanishes, and Newton’s law turns dp⃗/dtd\vec{p}/dt into the force:

dL⃗dt=dr⃗dt×p⃗+r⃗×dp⃗dt=r⃗×F⃗=τ⃗\frac{d\vec{L}}{dt} = \frac{d\vec{r}}{dt}\times\vec{p} + \vec{r}\times\frac{d\vec{p}}{dt} = \vec{r}\times\vec{F} = \vec{\tau}

The torque τ⃗\vec{\tau} changes angular momentum the way a force changes momentum. With no torque, L⃗\vec{L} stays fixed in size and direction. A force along r⃗\vec{r}, toward or away from the axis, exerts no torque, so pulling a mass inward cannot change L⃗\vec{L}. A spinning skater who pulls the arms in therefore spins faster:

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Fig. A spinning skater seen from above: a body with a weight in each hand. As the arms come in, the moment of inertia drops (orange). L=IωL = I\omega must stay the same (purple), so the angular velocity rises by the same factor (teal).

The same rule turns a diver’s tuck into a fast somersault, a collapsing star into a rapidly spinning pulsar, and keeps a molecule tumbling at a steady rate between collisions: nothing changes L⃗\vec{L} unless something twists.

Conservation from symmetry: Noether’s theorem

Emmy Noether, with drawings of symmetries and a conservation law

Fig. Emmy Noether (1882 to 1935) proved that every continuous symmetry of the laws of physics comes with a conserved quantity.

Why is angular momentum conserved at all? Noether’s theorem answers with symmetry:

if nothing changes when youthen this is conserved
shift the system in spacemomentum
turn the system about an axisangular momentum
shift the clockenergy

A free molecule, or an electron pulled toward a nucleus, looks the same after any turn about the center: its potential energy depends only on the distance. So its angular momentum is conserved. In quantum language, Lecture 3.7 showed that an observable is a constant of motion when its operator commutes with H^\hat{H}. For these systems L^\hat{L} commutes with H^\hat{H}, and angular momentum quantum numbers can label the stationary states.

A particle on a ring

Now the same particle on a circle, of mass μ\mu and radius rr with no potential energy, treated quantum mechanically. Real examples are the π\pi electrons that circulate around benzene (below), a methyl group spinning about its C−-C bond (Problem 1), or a diatomic turning in a plane.

The operator

The arc length along the ring is s=rϕs = r\phi. Momentum along the ring is p^s=−iℏ d/ds\hat{p}_s = -i\hbar\,d/ds, and the angular momentum about the axis is rr times it:

L^z=r p^s=−iℏ r dds=−iℏ ddϕ\hat{L}_z = r\,\hat{p}_s = -i\hbar\,r\,\frac{d}{ds} = -i\hbar\,\frac{d}{d\phi}

The energy is all kinetic, p^s2/2μ\hat{p}_s^2/2\mu, which with I=μr2I = \mu r^2 becomes

H^=L^z22I=−ℏ22I d2dϕ2\hat{H} = \frac{\hat{L}_z^2}{2I} = -\frac{\hbar^2}{2I}\,\frac{d^2}{d\phi^2}

The wave must join up

The eigenvalue equation L^zΦ=LzΦ\hat{L}_z\Phi = L_z\Phi reads −iℏ dΦ/dϕ=LzΦ-i\hbar\,d\Phi/d\phi = L_z\Phi, and its solution is

Φ(ϕ)=eiLzϕ/ℏ\Phi(\phi) = e^{iL_z\phi/\hbar}

On an infinite line any value of LzL_z would do, as any momentum does for a free particle. On a ring, ϕ\phi and ϕ+2π\phi + 2\pi are the same point, so after one full turn the wavefunction must return to its starting value:

Φ(ϕ+2π)=Φ(ϕ)⟹e2πiLz/ℏ=1⟹Lzℏ=m=0,±1,±2,…\Phi(\phi + 2\pi) = \Phi(\phi) \quad\Longrightarrow\quad e^{2\pi iL_z/\hbar} = 1 \quad\Longrightarrow\quad \frac{L_z}{\hbar} = m = 0, \pm 1, \pm 2, \dots

By Euler’s formula (Appendix A.2), e2πim=cos⁡2πm+isin⁡2πme^{2\pi im} = \cos 2\pi m + i\sin 2\pi m equals 1 exactly when mm is a whole number.

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Fig. The real part of eimϕe^{im\phi} drawn around the ring (dotted). For m=0,1,2,3m = 0, 1, 2, 3 a whole number of wavelengths fits, and the wave joins itself at the dot where it started. For m=2.5m = 2.5 the wave comes back to ϕ=0\phi = 0 at the open circle, away from its start: the function would have two values at one point, so m=2.5m = 2.5 is not allowed.

The quantization comes from no wall and no potential, only from the ring closing on itself. Normalizing on the ring, ∫02π∣Φ∣2 dϕ=1\int_0^{2\pi}\lvert\Phi\rvert^2\,d\phi = 1, gives the factor 1/2π1/\sqrt{2\pi}. Each Φm\Phi_m is an eigenfunction of H^\hat{H} as well:

H^ Φm=12I L^z(mℏ Φm)=m2ℏ22I Φm\hat{H}\,\Phi_m = \frac{1}{2I}\,\hat{L}_z\big(m\hbar\,\Phi_m\big) = \frac{m^2\hbar^2}{2I}\,\Phi_m

Pairs, and no zero-point energy

Cut the ring open and straighten it: a box of length 2πr2\pi r (Lecture 3.2). In the box, nn half wavelengths fit between the walls; on the ring, a whole number ∣m∣\lvert m\rvert of wavelengths must fit around. So the ring keeps only the box states with even n=2∣m∣n = 2\lvert m\rvert, and gains one that the box cannot have:

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Fig. Energy levels of a ring of radius rr (purple) and of the box of length 2πr2\pi r made by cutting it open (gray), in units of ℏ2/2I\hbar^2/2I. The box has n2/4n^2/4, the ring m2m^2. The ring keeps the even box levels, each twice: +m+m runs counterclockwise (↺) and −m-m clockwise (↻). Its lowest level, m=0m = 0, has no energy at all.

The same comparison with matrices. In Lecture 3.5 the box became a matrix with the curvature row (1,−2,1)(1, -2, 1) on every line. On a ring the last point’s neighbor is the first point, so gluing the ends changes just two corner entries:

box:  [0.25  1.    2.25  4.    6.249 8.998]
ring: [0.    1.    1.    4.    4.    8.998 8.998]

Running and standing waves

The density of a ring state is the same everywhere, ∣Φm∣2=1/2π\lvert\Phi_m\rvert^2 = 1/2\pi. A state with sharp LzL_z is spread evenly around the ring, while its phase winds mm times around it. With its time factor, Φm e−iEmt/ℏ∝ei(mϕ−Emt/ℏ)\Phi_m\,e^{-iE_mt/\hbar} \propto e^{i(m\phi - E_mt/\hbar)} is a wave running around the ring: counterclockwise for m>0m > 0, clockwise for m<0m < 0.

The states mm and −m-m have the same energy, and that is the physical point: any linear superposition of them is again a state of that energy. Take the simplest one,

Ψ=Φm+Φ−m2=cos⁡mϕπ,H^Ψ=EmΦm+EmΦ−m2=EmΨ\Psi = \frac{\Phi_m + \Phi_{-m}}{\sqrt{2}} = \frac{\cos m\phi}{\sqrt{\pi}}, \qquad \hat{H}\Psi = \frac{E_m\Phi_m + E_m\Phi_{-m}}{\sqrt{2}} = E_m\Psi

(by Euler’s formula, eimϕ+e−imϕ=2cos⁡mϕe^{im\phi} + e^{-im\phi} = 2\cos m\phi). Because the energies match, the superposition is still a stationary state, and its density cos⁡2mϕ/π\cos^2 m\phi/\pi never changes. That is unlike a superposition of different energies, whose density moves (Lecture 3.7). It is a standing wave with 2∣m∣2\lvert m\rvert nodes, like a state of the box. It is an eigenfunction of H^\hat{H} but not of L^z\hat{L}_z: a measurement of LzL_z gives +mℏ+m\hbar or −mℏ-m\hbar, each with probability 1/21/2 (Lecture 3.6), and ⟨Lz⟩=0\langle L_z\rangle = 0. The free particle showed the same pair, eikxe^{ikx} against cos⁡kx\cos kx, in Operators 2.

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Fig. Two running waves add up to a standing wave. The line is the real part of the wavefunction, drawn as bumps around the ring; the shaded band is the probability density ∣Ψ∣2\lvert\Psi\rvert^2. Left and middle: e+2iϕe^{+2i\phi} and e−2iϕe^{-2i\phi} run counterclockwise and clockwise, and their density is even all around and never changes. Right: their sum, 2cos⁡2ϕ2\cos 2\phi, stands still; its density drops to zero at four nodes.

Classical and quantum, side by side

classical particle on a circlequantum particle on a ring
angular momentumany value, L=IωL = I\omegaonly Lz=mℏL_z = m\hbar, m=0,±1,±2,…m = 0, \pm 1, \pm 2, \dots
energyany value, L2/2IL^2/2Ionly Em=m2ℏ2/2IE_m = m^2\hbar^2/2I
where it isa definite angle, ϕ=ωt\phi = \omega twith sharp LzL_z, anywhere: ∣Φm∣2=1/2π\lvert\Phi_m\rvert^2 = 1/2\pi
lowest energy0, at rest at a known angle0, with the angle completely unknown
two directionssame energy at the same speedthe pair ±m\pm m

Angular momentum in three dimensions

Spherical coordinates

Rotation in space is easiest to describe with a distance and two angles: the polar angle θ\theta, measured down from the zz axis, and the azimuthal angle ϕ\phi, measured around it as on the ring.

Spherical coordinates r, theta and phi, with a small patch of the sphere r dtheta tall and r sin theta dphi wide

Fig. Spherical coordinates. A small patch of the sphere is r dθr\,d\theta tall and rsin⁡θ dϕr\sin\theta\,d\phi wide.

x=rsin⁡θcos⁡ϕ,y=rsin⁡θsin⁡ϕ,z=rcos⁡θ,0≤θ≤π,0≤ϕ<2πx = r\sin\theta\cos\phi, \qquad y = r\sin\theta\sin\phi, \qquad z = r\cos\theta, \qquad 0 \leq \theta \leq \pi, \quad 0 \leq \phi < 2\pi

Three components, three operators

Classically each component of L⃗=r⃗×p⃗\vec{L} = \vec{r}\times\vec{p} uses the two coordinates perpendicular to its own axis: Lx=ypz−zpyL_x = yp_z - zp_y, Ly=zpx−xpzL_y = zp_x - xp_z and Lz=xpy−ypxL_z = xp_y - yp_x. Replacing each momentum by −iℏ-i\hbar times a derivative gives the operators:

L^z\hat{L}_z is the ring operator in disguise. Turning a point about zz changes only ϕ\phi. By the chain rule, with ∂x/∂ϕ=−rsin⁡θsin⁡ϕ=−y\partial x/\partial\phi = -r\sin\theta\sin\phi = -y and ∂y/∂ϕ=rsin⁡θcos⁡ϕ=x\partial y/\partial\phi = r\sin\theta\cos\phi = x,

∂∂ϕ=∂x∂ϕ∂∂x+∂y∂ϕ∂∂y=x∂∂y−y∂∂x⟹L^z=−iℏ ∂∂ϕ\frac{\partial}{\partial\phi} = \frac{\partial x}{\partial\phi}\frac{\partial}{\partial x} + \frac{\partial y}{\partial\phi}\frac{\partial}{\partial y} = x\frac{\partial}{\partial y} - y\frac{\partial}{\partial x} \quad\Longrightarrow\quad \hat{L}_z = -i\hbar\,\frac{\partial}{\partial\phi}

So L^z\hat{L}_z measures how a function changes when it is turned a little about the zz axis, and L^x\hat{L}_x, L^y\hat{L}_y do the same for turns about xx and yy. The ring had a single axis. Space has three, and turns about different axes get in each other’s way.

Turns about different axes do not commute

Give a book a quarter turn about xx, then a quarter turn about yy. Start again and make the same two turns in the other order. The book ends up facing a different way:

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Fig. A book given the same two quarter turns in opposite orders. Left: about xx (dashed red line), then about yy. Right: about yy, then about xx. The axes stay fixed in space (corner triad). The two books end facing different directions, with the arrow on the cover pointing different ways.

Each component of L^\hat{L} measures the effect of a small turn about its axis, so if the turns do not commute, neither can the components. The flip and swap matrices of Operators 2 showed the same thing for mirrors. Turns add one more feature: two small turns, about xx and then about yy, differ from the opposite order by a small extra turn about zz. That is why the commutator of L^x\hat{L}_x and L^y\hat{L}_y comes out proportional to L^z\hat{L}_z.

The commutators

The commutator follows from [x^,p^x]=iℏ[\hat{x}, \hat{p}_x] = i\hbar. Expand [L^x,L^y]=[yp^z−zp^y, zp^x−xp^z][\hat{L}_x, \hat{L}_y] = [y\hat{p}_z - z\hat{p}_y,\ z\hat{p}_x - x\hat{p}_z] into four commutators. A coordinate and the momentum along a different axis commute, as do two coordinates or two momenta; only zz and p^z\hat{p}_z fail to commute. So the two terms without both zz and p^z\hat{p}_z, [yp^z,xp^z][y\hat{p}_z, x\hat{p}_z] and [zp^y,zp^x][z\hat{p}_y, z\hat{p}_x], vanish, and in the other two the remaining factors slide out:

[L^x,L^y]=[yp^z, zp^x]+[zp^y, xp^z]=yp^x [p^z,z]+xp^y [z,p^z]=−iℏ yp^x+iℏ xp^y=iℏ L^z\begin{aligned} [\hat{L}_x, \hat{L}_y] &= [y\hat{p}_z,\ z\hat{p}_x] + [z\hat{p}_y,\ x\hat{p}_z] \\ &= y\hat{p}_x\,[\hat{p}_z, z] + x\hat{p}_y\,[z, \hat{p}_z] \\ &= -i\hbar\,y\hat{p}_x + i\hbar\,x\hat{p}_y = i\hbar\,\hat{L}_z \end{aligned}

Cycling the labels x→y→z→xx \to y \to z \to x gives the other two.

The second line says the length commutes with every component:

A concrete check: L^z\hat{L}_z acting on xx, yy and zz

Only one component at a time

A particle on a sphere: the spherical harmonics

L^2\hat{L}^2 and the Hamiltonian

Written in spherical coordinates (a long application of the chain rule), the squared length is

L^2=−ℏ2[1sin⁡θ∂∂θ(sin⁡θ ∂∂θ)+1sin⁡2θ∂2∂ϕ2]\hat{L}^2 = -\hbar^2\left[\frac{1}{\sin\theta}\frac{\partial}{\partial\theta}\left(\sin\theta\,\frac{\partial}{\partial\theta}\right) + \frac{1}{\sin^2\theta}\frac{\partial^2}{\partial\phi^2}\right]
∇2=1r2∂∂r(r2∂∂r)−L^2ℏ2r2\nabla^2 = \frac{1}{r^2}\frac{\partial}{\partial r}\left(r^2\frac{\partial}{\partial r}\right) - \frac{\hat{L}^2}{\hbar^2r^2}

so the kinetic energy of any particle splits into a radial part and a rotational part, L^2/2μr2\hat{L}^2/2\mu r^2. Chapter 5 uses this split for the hydrogen atom.

H^=L^22I,I=μr2\hat{H} = \frac{\hat{L}^2}{2I}, \qquad I = \mu r^2

This is the rigid rotor, a diatomic molecule turning with a fixed bond length (Lecture 4.5). Its eigenfunctions are those of L^2\hat{L}^2.

The solution

Separate the angles, Y(θ,ϕ)=Θ(θ) Φ(ϕ)Y(\theta, \phi) = \Theta(\theta)\,\Phi(\phi). The angle ϕ\phi enters L^2\hat{L}^2 only through ∂2/∂ϕ2=−L^z2/ℏ2\partial^2/\partial\phi^2 = -\hat{L}_z^2/\hbar^2, so the ϕ\phi part is the ring all over again: Φm=eimϕ/2π\Phi_m = e^{im\phi}/\sqrt{2\pi} with whole mm. What remains is an equation for Θ(θ)\Theta(\theta). Its solutions stay finite at both poles only when the eigenvalue of L^2\hat{L}^2 is ℏ2l(l+1)\hbar^2l(l + 1), with ll a whole number no smaller than ∣m∣\lvert m\rvert. Otherwise they blow up at θ=0\theta = 0 or π\pi, much as the oscillator’s series blew up at large xx unless it stopped (Lecture 4.2). The finite solutions are polynomials in cos⁡θ\cos\theta and sin⁡θ\sin\theta (associated Legendre functions).

llmmYlm(θ,ϕ)Y_l^m(\theta, \phi)rl Ylmr^l\,Y_l^m in x,y,zx, y, z
0014π\sqrt{\dfrac{1}{4\pi}}14π\sqrt{\dfrac{1}{4\pi}}s
1034π cos⁡θ\sqrt{\dfrac{3}{4\pi}}\,\cos\theta34π z\sqrt{\dfrac{3}{4\pi}}\,zp
1±1\pm 1∓38π sin⁡θ e±iϕ\mp\sqrt{\dfrac{3}{8\pi}}\,\sin\theta\,e^{\pm i\phi}∓38π (x±iy)\mp\sqrt{\dfrac{3}{8\pi}}\,(x \pm iy)p
20516π (3cos⁡2θ−1)\sqrt{\dfrac{5}{16\pi}}\,(3\cos^2\theta - 1)516π (3z2−r2)\sqrt{\dfrac{5}{16\pi}}\,(3z^2 - r^2)d
2±1\pm 1∓158π sin⁡θcos⁡θ e±iϕ\mp\sqrt{\dfrac{15}{8\pi}}\,\sin\theta\cos\theta\,e^{\pm i\phi}∓158π z (x±iy)\mp\sqrt{\dfrac{15}{8\pi}}\,z\,(x \pm iy)d
2±2\pm 21532π sin⁡2θ e±2iϕ\sqrt{\dfrac{15}{32\pi}}\,\sin^2\theta\,e^{\pm 2i\phi}1532π (x±iy)2\sqrt{\dfrac{15}{32\pi}}\,(x \pm iy)^2d

Normalized and orthogonal on the sphere

numpy integrates every pair with l≤2l \leq 2 on a grid of angles:

[[1. 0. 0. 0. 0. 0. 0. 0. 0.]
 [0. 1. 0. 0. 0. 0. 0. 0. 0.]
 [0. 0. 1. 0. 0. 0. 0. 0. 0.]
 [0. 0. 0. 1. 0. 0. 0. 0. 0.]
 [0. 0. 0. 0. 1. 0. 0. 0. 0.]
 [0. 0. 0. 0. 0. 1. 0. 0. 0.]
 [0. 0. 0. 0. 0. 0. 1. 0. 0.]
 [0. 0. 0. 0. 0. 0. 0. 1. 0.]
 [0. 0. 0. 0. 0. 0. 0. 0. 1.]]

The 9×99\times9 overlap matrix is the identity: each YlmY_l^m has length 1 and is perpendicular to the other eight.

Pictures on the globe: ll nodal lines

A spherical harmonic is a wave on the surface of a sphere. Color each point by the sign of its real part:

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Fig. The real part of YlmY_l^m on a sphere, for l=0l = 0 to 3 and m=0m = 0 to ll, with the north pole tipped toward the viewer. Teal is positive, orange negative, and the dark lines are nodes. Under each globe: the nodal circles around the zz axis plus the circles through the poles, which always add up to ll.

Try it: pick ll and mm, drag the globe to turn it, and switch to the density to watch the circles through the poles disappear. The panel on the right is the vector model of the next section.

The vector model

The two sharp numbers fix the length of L⃗\vec{L} and its height along zz. Draw L⃗\vec{L} as an arrow with exactly those two properties:

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Fig. The vector model for l=1l = 1 and l=2l = 2. Every arrow has the same length l(l+1) ℏ\sqrt{l(l+1)}\,\hbar (dotted circle), and its height mℏm\hbar takes 2l+12l + 1 values. Where the arrow points around the zz axis is unknown, so each state is drawn as a cone of possible directions.

⟨Lx2⟩+⟨Ly2⟩=ℏ2[l(l+1)−m2]>0(l>0)\langle L_x^2\rangle + \langle L_y^2\rangle = \hbar^2\left[l(l+1) - m^2\right] > 0 \qquad (l > 0)

By the symmetry about zz each takes half, and ⟨Lx⟩=⟨Ly⟩=0\langle L_x\rangle = \langle L_y\rangle = 0. The part of L⃗\vec{L} perpendicular to zz has a definite size but no definite direction: that is the cone.

Toward the rigid rotor

particle on a ringparticle on a sphere
coordinatesϕ\phiθ\theta and ϕ\phi
sharp observablesL^z\hat{L}_zL^2\hat{L}^2 and L^z\hat{L}_z
quantum numbersm=0,±1,±2,…m = 0, \pm 1, \pm 2, \dotsl=0,1,2,…l = 0, 1, 2, \dots and m=−l,…,lm = -l, \dots, l
stateseimϕ/2πe^{im\phi}/\sqrt{2\pi}Ylm(θ,ϕ)Y_l^m(\theta, \phi)
HamiltonianL^z2/2I\hat{L}_z^2/2IL^2/2I\hat{L}^2/2I
energiesm2ℏ2/2Im^2\hbar^2/2Il(l+1)ℏ2/2Il(l+1)\hbar^2/2I
states per level2 (1 for m=0m = 0)2l+12l + 1
lowest energy00

Problems

Problem 1: A methyl group as a rotor

A methyl group spins about the C−-C bond of ethane. Treat it as three H atoms (mH=1.008m_{\text{H}} = 1.008 u) on a ring of radius 1.02 Å, with the carbon on the axis. Find the moment of inertia, the energy unit ℏ2/2I\hbar^2/2I in cm−1^{-1}, and the first gap. How many states lie below kBTk_BT at 300 K (kBT=208k_BT = 208 cm−1^{-1})? (Real methyl groups are hindered by a threefold barrier, which this model leaves out.)

Problem 2: An electron circling benzene

In the benzene example, an electron in the highest filled level has ∣m∣=1\lvert m\rvert = 1 on a ring of radius 139 pm. Using Lz=mevrL_z = m_e vr, find its speed, compare it with the speed of light, and find the time for one lap. Its density is the same all around the ring; in what sense is it “circling”? What changes for ∣m∣=2\lvert m\rvert = 2?

Problem 3: A lopsided state on a ring

A particle on a ring is in the state ψ(ϕ)=Ncos⁡2ϕ\psi(\phi) = N\cos^2\phi. Normalize it, write it as a sum of ring states Φm\Phi_m, and give the possible results of measuring LzL_z with their probabilities. Find ⟨Lz⟩\langle L_z\rangle and ⟨E⟩\langle E\rangle.

Problem 4: Powers of x+iyx + iy

Show that L^z(x+iy)=ℏ (x+iy)\hat{L}_z(x + iy) = \hbar\,(x + iy) and, using the product rule, that L^z(x+iy)k=kℏ (x+iy)k\hat{L}_z(x + iy)^k = k\hbar\,(x + iy)^k. Write (x+iy)k(x + iy)^k in spherical coordinates. Which spherical harmonic is it proportional to for k=1k = 1 and k=2k = 2 (on the unit sphere)? Why must (x+iy)k/rk(x + iy)^k/r^k be the top rung of its ladder?

Problem 5: Measuring LxL_x when LzL_z is sharp

A particle is in the l=1l = 1 state x+iyx + iy (up to normalization), which has Lz=+ℏL_z = +\hbar. Using the 3×33\times3 matrices (the “Going further” box after the L^z\hat{L}_z example), find the possible results of measuring LxL_x and their probabilities, and compute ⟨Lx⟩\langle L_x\rangle and ⟨Lx2⟩\langle L_x^2\rangle. Compare with the vector model.

Problem 6: The magic angle

Show that Y20∝3cos⁡2θ−1Y_2^0 \propto 3\cos^2\theta - 1 is an eigenfunction of L^2\hat{L}^2 with eigenvalue 6ℏ26\hbar^2. Find the angles θ\theta of its two nodal cones. Solid-state NMR spins samples at the first of these angles, the “magic angle”; look up why.

Problem 7: How fuzzy are LxL_x and LyL_y?

Use ⟨Lx2⟩=⟨Ly2⟩=12ℏ2[l(l+1)−m2]\langle L_x^2\rangle = \langle L_y^2\rangle = \frac{1}{2}\hbar^2\left[l(l+1) - m^2\right] and ⟨Lx⟩=⟨Ly⟩=0\langle L_x\rangle = \langle L_y\rangle = 0 to find σLxσLy\sigma_{L_x}\sigma_{L_y} in the state YlmY_l^m. Compare it with the bound ℏ2∣⟨Lz⟩∣\frac{\hbar}{2}\lvert\langle L_z\rangle\rvert from Lecture 3.6. For which mm is the bound reached exactly? Interpret the result with the cones.

Problem 8: Climbing with L^+\hat{L}_+

Use L^+=ℏ eiϕ(∂/∂θ+icot⁡θ ∂/∂ϕ)\hat{L}_+ = \hbar\,e^{i\phi}\left(\partial/\partial\theta + i\cot\theta\,\partial/\partial\phi\right) to compute L^+Y10\hat{L}_+Y_1^0 and L^+Y11\hat{L}_+Y_1^1, with the functions from the table. Check both against L^+Ylm=ℏl(l+1)−m(m+1) Ylm+1\hat{L}_+Y_l^m = \hbar\sqrt{l(l+1) - m(m+1)}\,Y_l^{m+1}.