Problems 8

Part V ✎ Problems Phillips pp. 174–178 Β· ~25 min read

  • total angular momentum
  • spherical harmonic

The most important part of this set is a footnote in problem 6. It is where orbital angular momentum is shown to have no half-integer values, and the book does not flag it.

Nine problems, and they divide cleanly. 1–2 are counting and correspondence: how many states, and how large must ll get before quantization stops showing. 3–4 are the numbers β€” Zeeman splittings and the rigid rotor, and problem 4 lands on a result about hydrogen molecules that is worth carrying away. 5–8 build the machinery Β§8.3 used without proving: that L^z=βˆ’iβ„β€‰βˆ‚/βˆ‚Ο•\hat L_z = -i\hbar\,\partial/\partial\phi, that mlm_l is an integer, and which functions solve the angular equation. 9 goes back to Β§6.5’s three-dimensional oscillator and sorts its degenerate levels by angular momentum.

Counting and correspondence

1 Adding l = 3 and s = 1 derivation

A particle has orbital angular momentum l=3l = 3 and spin s=1s = 1.

(a) How many distinct states are there with different values for the zz components of the orbital and spin angular momenta? (b) What are the possible values of jj? (c) How many distinct states are there with different values for the magnitude and zz component of the total angular momentum?

(The book adds a note: the number of distinct (ml,ms)(m_l, m_s) states equals the number of distinct (j,mj)(j, m_j) states.)

βœ“ Worked solution

(a) mlm_l takes 2l+1=72l+1 = 7 values and msm_s takes 2s+1=32s+1 = 3, independently:

7Γ—3=21Β states7 \times 3 = \mathbf{21}\ \text{states}

(b) Eq. (8.6) runs from l+sl+s down to ∣lβˆ’s∣|l-s| in steps of 1:

j=4,Β 3,Β 2j = 4,\ 3,\ 2

(c) Each jj carries 2j+12j+1 values of mjm_j:

9+7+5=219 + 7 + 5 = \mathbf{21}

The counts agree, and the note is telling you this is not a coincidence. The labels (ml,ms)(m_l, m_s) and (j,mj)(j, m_j) describe the same 21 states β€” coupling is a change of basis, and a change of basis cannot alter a dimension. That is also why Eq. (8.6) stops at ∣lβˆ’s∣|l-s|: sort the uncoupled states by mj=ml+msm_j = m_l + m_s into a staircase and peel multiplets off the top, and the columns run out exactly there.

Eq. (8.6): combining two angular momenta, and checking the states add up
j = 3/2, 1/2 Β (from 3/2 down to 1/2)
uncoupled: (2l+1)(2s+1) = 6 states
coupled: Ξ£(2j+1) = 6 states
βœ“ equal β€” as they must be, because the two labellings describe one set of states
Each row is one value of mj = ml + ms. The stack of squares is how many uncoupled states share it; the colours are the multiplets peeled off from the top, largest j first.
3/2
1
1/2
2
-1/2
2
-3/2
1
j = 3/2 (4 states)j = 1/2 (2 states)

The staircase is why Eq. (8.6) stops where it does. Peel the widest multiplet off the top of the stack, then the next, and the columns run out exactly when j reaches |l βˆ’ s|. Try l = 3, s = 1 β€” problem 1's case: 21 states either way.

2 A classical electron, and how big l has to be numerical

A classical electron moves in a circle with a given radius and speed. (a) What value of ll gives a quantized angular momentum close to this classical one? (b) How many discrete values are possible for its zz component? (c) How closely spaced are these values, as a fraction of the magnitude?

πŸ’‘ Phillips' own hint

The classical angular momentum mevr=9.1Γ—10βˆ’33m_evr = 9.1\times10^{-33} J s is approximately equal to l(l+1) ℏ\sqrt{l(l+1)}\,\hbar if l=86l = 86.

βœ“ Worked solution

(a) Setting l(l+1) ℏ=9.1Γ—10βˆ’33\sqrt{l(l+1)}\,\hbar = 9.1\times10^{-33} J s gives l(l+1)=86.5\sqrt{l(l+1)} = 86.5, so

l=86l = 86

(b) 2l+1=1732l+1 = \mathbf{173} discrete values of LzL_z.

(c) Adjacent values differ by ℏ\hbar, against a magnitude 86β‹…87 ℏ=86.5ℏ\sqrt{86\cdot87}\,\hbar = 86.5\hbar:

ℏl(l+1) ℏ=186.5=1.16%\frac{\hbar}{\sqrt{l(l+1)}\,\hbar} = \frac{1}{86.5} = 1.16\%

And that is the answer the problem is really after. A 1.16% step is already hard to resolve; for a spinning object of everyday size ll is around 103010^{30} and the steps are 10βˆ’3010^{-30} of the total. The quantization never switches off β€” there are always exactly 2l+12l+1 values β€” it just becomes unmeasurably fine. Β§8.1’s widget makes the same point with the cone angle, which at l=86l = 86 is already down to 6.15Β°6.15Β°.

Putting numbers on the magnetism

3 Hydrogen in a magnetic field, electron and proton numerical

The ground state of hydrogen has zero orbital angular momentum, with magnetic moments given by Eqs. (8.8) and (8.12). The atom is placed in a field of 0.5 T.

(a) Explain why, ignoring the proton’s moment, the ground state splits into two levels, and find the spacing in eV. (b) Explain why each of those levels is itself split in two when the proton’s moment is included, and find that spacing.

πŸ’‘ Phillips' own hint

(a) The splitting arises from the interaction of the electron magnetic moment with the field. By Eq. (8.16) it is 2ΞΌBB=5.8Γ—10βˆ’52\mu_B B = 5.8\times10^{-5} eV.

(b) Additional splitting equal to 2Γ—2.79 μNB=8.8Γ—10βˆ’82\times2.79\,\mu_N B = 8.8\times10^{-8} eV arises from the proton magnetic moment.

βœ“ Worked solution

(a) With l=0l = 0 the only angular momentum is the electron’s spin, s=12s = \tfrac12, so ms=Β±12m_s = \pm\tfrac12 β€” two states. By Eq. (8.8) their magnetic energies are βˆ“2ΞΌBBms\mp 2\mu_B B m_s, i.e. Β±ΞΌBB\pm\mu_B B, so the gap is

2ΞΌBB=2(9.274Γ—10βˆ’24)(0.5)=9.27Γ—10βˆ’24Β J=5.79Γ—10βˆ’5Β eV2\mu_B B = 2(9.274\times10^{-24})(0.5) = 9.27\times10^{-24}\ \mathrm J = 5.79\times10^{-5}\ \mathrm{eV}

(b) The proton is also spin-Β½, so it has its own two orientations, and Eq. (8.12) gives its moment as 2.79 μNmj2.79\,\mu_N m_j. Each electron level therefore splits again, by

2Γ—2.79 μNB=2(2.79)(5.05Γ—10βˆ’27)(0.5)=8.80Γ—10βˆ’8Β eV2\times2.79\,\mu_N B = 2(2.79)(5.05\times10^{-27})(0.5) = 8.80\times10^{-8}\ \mathrm{eV}

Four levels in total, in two widely separated pairs β€” the electron splitting is 658 times the proton splitting, because ΞΌB/ΞΌN=mp/me=1836\mu_B/\mu_N = m_p/m_e = 1836 and the proton’s 2.79 recovers only part of that.

4 The rigid rotor, and why hydrogen molecules spin at room temperature numerical

Two masses mm are attached to the ends of a massless rod of length aa, free to rotate in three dimensions about the centre of mass.

(a) Write down the classical rotational kinetic energy, and show the quantum levels are

El=l(l+1)ℏ2ma2,l=0,1,2,…E_l = \frac{l(l+1)\hbar^2}{ma^2},\qquad l = 0,1,2,\dots

(b) What is the degeneracy of the ll-th level? (c) The Hβ‚‚ molecule is two protons 0.075 nm apart. Find the energy needed to excite the first excited rotational state.

πŸ’‘ Phillips' own hint

(a) The classical rotational energy is L2/2IL^2/2I where II is the moment of inertia about the centre of mass. Here I=ma2I = ma^2, and the eigenvalues of L^2\hat L^2 are l(l+1)ℏ2l(l+1)\hbar^2.

(b) For every ll, LzL_z can have 2l+12l+1 values, so there are 2l+12l+1 independent eigenfunctions with energy ElE_l.

(c) E1βˆ’E0=1.5Γ—10βˆ’2E_1 - E_0 = 1.5\times10^{-2} eV. Note that the rotational states of the hydrogen molecule are excited at room temperature, because kTβ‰ˆ1/40kT \approx 1/40 eV.

βœ“ Worked solution

(a) Each mass sits at distance a/2a/2 from the centre, so

I=2m(a2)2=ma22I = 2m\left(\frac a2\right)^2 = \frac{ma^2}{2}

Classically E=L2/2IE = L^2/2I. This system has no potential energy at all β€” nothing but rotation β€” so the Hamiltonian is L^2/2I\hat L^2/2I and its eigenvalues follow immediately from Eq. (8.23):

El=l(l+1)ℏ22I=l(l+1)ℏ22β‹…ma2/2=l(l+1)ℏ2ma2E_l = \frac{l(l+1)\hbar^2}{2I} = \frac{l(l+1)\hbar^2}{2 \cdot ma^2/2} = \frac{l(l+1)\hbar^2}{ma^2}

(b) 2l+12l+1, one for each mlm_l β€” the field-free degeneracy that Β§8.2’s magnetic field lifts.

(c) With m=mpm = m_p and a=0.075a = 0.075 nm,

E1βˆ’E0=2ℏ2mpa2=1.48Γ—10βˆ’2Β eVE_1 - E_0 = \frac{2\hbar^2}{m_pa^2} = 1.48\times10^{-2}\ \mathrm{eV}

Now compare with kTkT at room temperature, which is 0.02590.0259 eV. The rotational excitation costs less than the thermal energy available, so Hβ‚‚ molecules in a room are rotating β€” the states are thermally populated.

The machinery Β§8.3 used on credit

5 Where LΜ‚_z = βˆ’iΔ§ βˆ‚/βˆ‚Ο† comes from, and why m_l is an integer derivation

(a) Using x=rsin⁑θcos⁑ϕx = r\sin\theta\cos\phi, y=rsin⁑θsin⁑ϕy = r\sin\theta\sin\phi, z=rcos⁑θz = r\cos\theta and the chain rule, show that

L^z=βˆ’iℏ(xβˆ‚βˆ‚yβˆ’yβˆ‚βˆ‚x)=βˆ’iβ„βˆ‚βˆ‚Ο•\hat L_z = -i\hbar\left(x\frac{\partial}{\partial y} - y\frac{\partial}{\partial x}\right) = -i\hbar\frac{\partial}{\partial\phi}

(b) Verify that Zml(Ο•)=eimlΟ•/2Ο€Z_{m_l}(\phi) = e^{im_l\phi}/\sqrt{2\pi} is an eigenfunction of L^z\hat L_z with eigenvalue mlℏm_l\hbar. (c) Explain why it is not unreasonable to assume ψ(r,ΞΈ,Ο•)=ψ(r,ΞΈ,Ο•+2Ο€)\psi(r,\theta,\phi) = \psi(r,\theta,\phi+2\pi), and show this implies mlm_l is an integer. (d) Show ∫02Ο€Zmlβ€²βˆ—Zml dΟ•\int_0^{2\pi} Z^*_{m_l'}Z_{m_l}\,\mathrm d\phi is 1 if mlβ€²=mlm_l' = m_l and 0 otherwise. (e) Show that if ψ=βˆ‘mlcml(r,ΞΈ)Zml(Ο•)\psi = \sum_{m_l}c_{m_l}(r,\theta)Z_{m_l}(\phi) then cml(r,ΞΈ)=∫02Ο€Zmlβˆ—Οˆβ€‰dΟ•c_{m_l}(r,\theta) = \int_0^{2\pi}Z^*_{m_l}\psi\,\mathrm d\phi.

πŸ’‘ Phillips' own hint

(a) Show that L^zZml=mlℏZml\hat L_zZ_{m_l} = m_l\hbar Z_{m_l}.

(b) A point with coordinates (r,ΞΈ,Ο•)(r,\theta,\phi) also has coordinates (r,ΞΈ,Ο•+2Ο€)(r,\theta,\phi+2\pi).

βœ“ Worked solution

(a) By the chain rule, βˆ‚Οˆβˆ‚Ο•=βˆ‚Οˆβˆ‚xβˆ‚xβˆ‚Ο•+βˆ‚Οˆβˆ‚yβˆ‚yβˆ‚Ο•+βˆ‚Οˆβˆ‚zβˆ‚zβˆ‚Ο•\dfrac{\partial\psi}{\partial\phi} = \dfrac{\partial\psi}{\partial x}\dfrac{\partial x}{\partial\phi} + \dfrac{\partial\psi}{\partial y}\dfrac{\partial y}{\partial\phi} + \dfrac{\partial\psi}{\partial z}\dfrac{\partial z}{\partial\phi}. From the coordinate relations, βˆ‚x/βˆ‚Ο•=βˆ’rsin⁑θsin⁑ϕ=βˆ’y\partial x/\partial\phi = -r\sin\theta\sin\phi = -y, βˆ‚y/βˆ‚Ο•=+rsin⁑θcos⁑ϕ=+x\partial y/\partial\phi = +r\sin\theta\cos\phi = +x, and βˆ‚z/βˆ‚Ο•=0\partial z/\partial\phi = 0. Substituting,

βˆ‚βˆ‚Ο•=xβˆ‚βˆ‚yβˆ’yβˆ‚βˆ‚x\frac{\partial}{\partial\phi} = x\frac{\partial}{\partial y} - y\frac{\partial}{\partial x}

which is exactly the bracket in L^z\hat L_z.

(b) βˆ’iβ„β€‰βˆ‚βˆ‚Ο•eimlΟ•2Ο€=βˆ’iℏ(iml)eimlΟ•2Ο€=mlℏZml-i\hbar\,\dfrac{\partial}{\partial\phi}\dfrac{e^{im_l\phi}}{\sqrt{2\pi}} = -i\hbar(im_l)\dfrac{e^{im_l\phi}}{\sqrt{2\pi}} = m_l\hbar Z_{m_l}.

(c) (r,ΞΈ,Ο•)(r,\theta,\phi) and (r,ΞΈ,Ο•+2Ο€)(r,\theta,\phi+2\pi) are the same point in space, so a wave function that assigns two different values to them would not be a function of position. Requiring eiml(Ο•+2Ο€)=eimlΟ•e^{im_l(\phi+2\pi)} = e^{im_l\phi} gives e2Ο€iml=1e^{2\pi im_l} = 1, and hence

ml=0,Β±1,Β±2,…m_l = 0, \pm1, \pm2, \dots

(d) ∫02Ο€eβˆ’imlβ€²Ο•2Ο€eimlΟ•2Ο€dΟ•=12Ο€βˆ«02Ο€ei(mlβˆ’mlβ€²)ϕ dΟ•\displaystyle\int_0^{2\pi}\frac{e^{-im_l'\phi}}{\sqrt{2\pi}}\frac{e^{im_l\phi}}{\sqrt{2\pi}}\mathrm d\phi = \frac{1}{2\pi}\int_0^{2\pi}e^{i(m_l-m_l')\phi}\,\mathrm d\phi. For ml=mlβ€²m_l = m_l' the integrand is 1 and the result is 1; otherwise the exponential completes a whole number of cycles and integrates to zero.

(e) Multiply the expansion by Zmlβˆ—Z^*_{m_l} and integrate. By (d) every term vanishes except the one with matching index, which returns cmlc_{m_l}.

6 Decomposing sin 2Ο† cos Ο† numerical

A wave function has azimuthal dependence ψ∝sin⁑2Ο•cos⁑ϕ\psi \propto \sin 2\phi\cos\phi. What are the possible outcomes of a measurement of LzL_z, and their probabilities?

πŸ’‘ Phillips' own hint

Use sin⁑2Ο•=e2iΟ•βˆ’eβˆ’2iΟ•2i\sin2\phi = \dfrac{e^{2i\phi} - e^{-2i\phi}}{2i} and cos⁑ϕ=eiΟ•+eβˆ’iΟ•2\cos\phi = \dfrac{e^{i\phi} + e^{-i\phi}}{2}, and show that

ψ(r,ΞΈ,Ο•)∝e3iΟ•+eiΟ•βˆ’eβˆ’iΟ•βˆ’eβˆ’3iΟ•\psi(r,\theta,\phi) \propto e^{3i\phi} + e^{i\phi} - e^{-i\phi} - e^{-3i\phi}

Comparison with Eq. (8.27) shows a measurement of LzL_z can yield four possible values 3ℏ3\hbar, ℏ\hbar, βˆ’β„-\hbar and βˆ’3ℏ-3\hbar with equal probabilities of 1/4.

βœ“ Worked solution

Multiplying the two exponential forms:

sin⁑2Ο•cos⁑ϕ=(e2iΟ•βˆ’eβˆ’2iΟ•)2iβ‹…(eiΟ•+eβˆ’iΟ•)2=14i(e3iΟ•+eiΟ•βˆ’eβˆ’iΟ•βˆ’eβˆ’3iΟ•)\sin2\phi\cos\phi = \frac{(e^{2i\phi} - e^{-2i\phi})}{2i}\cdot\frac{(e^{i\phi} + e^{-i\phi})}{2} = \frac{1}{4i}\left(e^{3i\phi} + e^{i\phi} - e^{-i\phi} - e^{-3i\phi}\right)

Four terms, all of the same magnitude. Comparing with Eq. (8.27), the outcomes are ml=+3,+1,βˆ’1,βˆ’3m_l = +3, +1, -1, -3, each with probability 14\tfrac14.

Note which values are absent: ml=0m_l = 0 and ml=Β±2m_l = \pm2 never occur. A product of trigonometric functions does not spread over every harmonic β€” it picks out a specific few, exactly as multiplying two signals in DSP produces sum and difference frequencies and nothing else.

7 Decomposing cosΒ²Ο† numerical

A wave function has azimuthal dependence ψ∝cos⁑2Ο•\psi \propto \cos^2\phi. What are the possible outcomes of a measurement of LzL_z, and their probabilities?

βœ“ Worked solution

Use the same trick:

cos⁑2Ο•=1+cos⁑2Ο•2=12+e2iΟ•+eβˆ’2iΟ•4\cos^2\phi = \frac{1 + \cos2\phi}{2} = \frac12 + \frac{e^{2i\phi} + e^{-2i\phi}}{4}

So ml=0,+2,βˆ’2m_l = 0, +2, -2 with amplitudes in the ratio 12:14:14\tfrac12 : \tfrac14 : \tfrac14. Squaring gives 14:116:116\tfrac14 : \tfrac1{16} : \tfrac1{16}, and normalizing by their sum 38\tfrac38:

P(0)=23,P(+2ℏ)=P(βˆ’2ℏ)=16P(0) = \frac{2}{3},\qquad P(+2\hbar) = P(-2\hbar) = \frac16

Compare with problem 6. There, four equal amplitudes gave four equal probabilities. Here the amplitudes are unequal, and squaring exaggerates the imbalance: a 2:1 amplitude ratio becomes 4:1 in probability. Confirmed numerically above.

Note also that cos⁑2Ο•\cos^2\phi is real and even, so its decomposition is symmetric in Β±ml\pm m_l β€” the state has ⟨Lz⟩=0\langle L_z\rangle = 0 even though it is not an eigenstate.

8 Which functions solve the angular equation derivation

In spherical polars,

L^2=βˆ’β„2(βˆ‚2βˆ‚ΞΈ2+cos⁑θsinβ‘ΞΈβˆ‚βˆ‚ΞΈ+1sin⁑2ΞΈβˆ‚2βˆ‚Ο•2)\hat L^2 = -\hbar^2\left(\frac{\partial^2}{\partial\theta^2} + \frac{\cos\theta}{\sin\theta}\frac{\partial}{\partial\theta} + \frac{1}{\sin^2\theta}\frac{\partial^2}{\partial\phi^2}\right)

Show that the simultaneous eigenfunctions of L^2\hat L^2 and L^z\hat L_z have the form Yl,ml(ΞΈ,Ο•)=Fl,ml(ΞΈ)eimlΟ•Y_{l,m_l}(\theta,\phi) = F_{l,m_l}(\theta)e^{im_l\phi}, where FF obeys

d2FdΞΈ2+cos⁑θsin⁑θdFdΞΈ+(l(l+1)βˆ’ml2sin⁑2ΞΈ)F=0\frac{\mathrm d^2F}{\mathrm d\theta^2} + \frac{\cos\theta}{\sin\theta}\frac{\mathrm dF}{\mathrm d\theta} + \left(l(l+1) - \frac{m_l^2}{\sin^2\theta}\right)F = 0

Finite solutions exist on 0≀θ≀π0 \le \theta \le \pi only for l=0,1,2,…l = 0,1,2,\dots and ml=βˆ’l,…,+lm_l = -l,\dots,+l. Find by substitution the ll and mlm_l for which Fa=AF_a = A, Fb=Bcos⁑θF_b = B\cos\theta and Fc=Csin⁑θF_c = C\sin\theta are solutions.

βœ“ Worked solution

Separation. L^z\hat L_z acts only on Ο•\phi, so its eigenfunctions fix the Ο•\phi dependence as eimlΟ•e^{im_l\phi} (problem 5). Substituting Y=F(ΞΈ)eimlΟ•Y = F(\theta)e^{im_l\phi} into L^2Y=l(l+1)ℏ2Y\hat L^2Y = l(l+1)\hbar^2Y, the βˆ‚2/βˆ‚Ο•2\partial^2/\partial\phi^2 term returns βˆ’ml2-m_l^2, the exponential cancels throughout, and the stated ODE remains.

The three substitutions.

Fa=AF_a = A: both derivatives vanish, leaving (l(l+1)βˆ’ml2/sin⁑2ΞΈ)A=0\left(l(l+1) - m_l^2/\sin^2\theta\right)A = 0 for all ΞΈ\theta. The ΞΈ\theta-dependent term must vanish on its own, so ml=0m_l = 0, and then l(l+1)=0l(l+1) = 0 gives l=0l = 0. (l,ml)=(0,0)(l, m_l) = (0,0).

Fb=Bcos⁑θF_b = B\cos\theta: Fβ€²β€²=βˆ’Bcos⁑θF'' = -B\cos\theta and (cos⁑θ/sin⁑θ)Fβ€²=βˆ’Bcos⁑θ(\cos\theta/\sin\theta)F' = -B\cos\theta, so the equation becomes Bcos⁑θ(βˆ’2+l(l+1)βˆ’ml2/sin⁑2ΞΈ)=0B\cos\theta\left(-2 + l(l+1) - m_l^2/\sin^2\theta\right) = 0. Again ml=0m_l = 0, and l(l+1)=2l(l+1) = 2 gives (l,ml)=(1,0)(l, m_l) = (1,0).

Fc=Csin⁑θF_c = C\sin\theta: substituting and multiplying through by sin⁑θ/C\sin\theta/C leaves 1βˆ’ml2+sin⁑2ΞΈ(l(l+1)βˆ’2)=01 - m_l^2 + \sin^2\theta\left(l(l+1) - 2\right) = 0. Both pieces must vanish separately, giving ml2=1m_l^2 = 1 and l(l+1)=2l(l+1) = 2: (l,ml)=(1,Β±1)(l, m_l) = (1,\pm1).

These are exactly Table 8.1’s l≀1l \le 1 entries, recovered from the differential equation rather than quoted.

Back to the oscillator

9 Sorting the 3-D oscillator by angular momentum derivation

Reconsider Β§6.5’s three-dimensional harmonic oscillator. Using Table 8.1, linear combinations of its degenerate eigenfunctions can be made into simultaneous eigenfunctions of energy, L2L^2 and LzL_z.

(a) Verify that the eigenfunction with energy 32ℏω\tfrac32\hbar\omega has l=0l = 0, ml=0m_l = 0. (b) Construct eigenfunctions with energy 52ℏω\tfrac52\hbar\omega and l=1l = 1, ml=βˆ’1,0,+1m_l = -1, 0, +1. (c) Construct eigenfunctions with energy 72ℏω\tfrac72\hbar\omega and l=2l = 2, ml=βˆ’2,βˆ’1,0,+1,+2m_l = -2,-1,0,+1,+2, and one with l=0l = 0, ml=0m_l = 0.

πŸ’‘ Phillips' own hint

(a) The eigenfunction with energy 32ℏω\tfrac32\hbar\omega has l=0l = 0 and ml=0m_l = 0 because it is spherically symmetric.

(b) Form linear combinations of eigenfunctions with energy 52ℏω\tfrac52\hbar\omega which are proportional to x+iyx+iy, zz and xβˆ’iyx-iy.

βœ“ Worked solution

The 3-D oscillator’s level nn has energy (n+32)ℏω(n + \tfrac32)\hbar\omega and degeneracy (n+1)(n+2)/2(n+1)(n+2)/2, with eigenfunctions being polynomials of degree nn in x,y,zx, y, z times the Gaussian eβˆ’r2/2a2e^{-r^2/2a^2}.

(a) n=0n = 0: one state, the bare Gaussian. It depends only on rr, so it is spherically symmetric β€” and Β§8.3a proved L^R(r)=0\hat{\mathbf L}R(r) = 0. Hence l=0l = 0, ml=0m_l = 0.

(b) n=1n = 1: three states, spanned by xx, yy, zz times the Gaussian. Table 8.1 says the combinations with definite LzL_z are

(x+iy) eβˆ’r2/2a2Β (ml=+1),z eβˆ’r2/2a2Β (ml=0),(xβˆ’iy) eβˆ’r2/2a2Β (ml=βˆ’1)(x+iy)\,e^{-r^2/2a^2} \ (m_l = +1),\qquad z\,e^{-r^2/2a^2} \ (m_l = 0),\qquad (x-iy)\,e^{-r^2/2a^2} \ (m_l = -1)

all with l=1l = 1, since each is rr times a Y1,mlY_{1,m_l}.

(c) n=2n = 2: six states, spanned by the quadratics x2,y2,z2,xy,yz,zxx^2, y^2, z^2, xy, yz, zx times the Gaussian. Five combinations match Y2,mlY_{2,m_l} β€” for instance (xΒ±iy)2(x\pm iy)^2 gives ml=Β±2m_l = \pm2, (xΒ±iy)z(x\pm iy)z gives ml=Β±1m_l = \pm1, and 3z2βˆ’r23z^2 - r^2 gives ml=0m_l = 0. That accounts for five.

The sixth is r2=x2+y2+z2r^2 = x^2+y^2+z^2 itself, which is spherically symmetric and therefore has l=0l = 0, ml=0m_l = 0.

So 6=5+16 = 5 + 1: this level carries two different values of ll at the same energy.

Angular shapes: |Yl,m(ΞΈ,Ο†)|Β² for l ≀ 3
z
state 3d, n_r = 0
⟨r⟩ = 10.50 aβ‚€, peak at 9.02 aβ‚€
nodes: 1 angular, 0 radial

Between the extremes: 1 nodal circle, and the density is pulled partway toward the equator. 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.

Check yourself

0 / 6 answered

  1. 1.Problem 5(c) requires . Why is that the deepest part of this problem set?

  2. Problem 6 gives four equal probabilities of ΒΌ; problem 7 gives β…”, β…™, β…™.

    2.Why does produce such lopsided probabilities when does not?

  3. 3.Problem 4(c) gives eV for Hβ‚‚, against eV at room temperature. What does the comparison explain?

  4. 4.Problem 8 finds that solves the angular equation for both and . Why can the equation not tell them apart?

  5. 5.Problem 9(c) finds six degenerate states at , splitting as (five states) plus (one). Why can they not all belong to a single ?

  6. 6.Problem 2's printed radius and speed give J s, while its hint says J s with . Why is this not a harmless typo?