Problems 4

Part II ✎ Problems Phillips pp. 77–82 Β· ~22 min read

  • Hermitian operator
  • orthogonality
  • degeneracy
  • generalized Fourier series
  • natural line width

The first two problems supply what Β§4.5 assumed without proving. Everything after them is one expansion machine, pointed at a different starting state each time.

Eleven problems in four groups. 1–2 prove the two facts Β§4.5 leaned on without proving β€” that energy eigenvalues are real and that eigenfunctions of different eigenvalues are orthogonal. 3–5 apply En∝n2/ma2E_n \propto n^2/ma^2 at atomic and nuclear scales and in two dimensions. 6–9 exercise superposition, including the two most interesting problems in the set: a well that suddenly doubles in width, and the revival time. 10–11 turn Ξ΄t ΔEβ‰ˆβ„\delta t\,\Delta E \approx \hbar into measurements.

Group 1 β€” the two deferred proofs

1 Energy eigenvalues are real derivation

In practice the potential energy function for a particle is a real function. Show that this implies the energy eigenvalues are real.

The eigenfunction ψn(x)\psi_n(x) and its complex conjugate satisfy

[βˆ’β„22md2dx2+V(x)]ψn=Enψnand[βˆ’β„22md2dx2+V(x)]ψnβˆ—=Enβˆ—Οˆnβˆ—\left[-\frac{\hbar^2}{2m}\frac{\mathrm d^2}{\mathrm dx^2} + V(x)\right]\psi_n = E_n\psi_n \quad\text{and}\quad \left[-\frac{\hbar^2}{2m}\frac{\mathrm d^2}{\mathrm dx^2} + V(x)\right]\psi_n^* = E_n^*\psi_n^*

Multiply the first by ψnβˆ—\psi_n^* and the second by ψn\psi_n, subtract, and show

βˆ’β„22mddx[ψnβˆ—dψndxβˆ’Οˆndψnβˆ—dx]=(Enβˆ’Enβˆ—)ψnβˆ—Οˆn-\frac{\hbar^2}{2m}\frac{\mathrm d}{\mathrm dx}\left[\psi_n^*\frac{\mathrm d\psi_n}{\mathrm dx} - \psi_n\frac{\mathrm d\psi_n^*}{\mathrm dx}\right] = (E_n - E_n^*)\psi_n^*\psi_n

By integrating over xx and assuming ψn(x)\psi_n(x) is zero at x=±∞x = \pm\infty, show that En=Enβˆ—E_n = E_n^*.

πŸ’‘ Phillips' own hint

The VV terms cancel in the subtraction because VV is real β€” that is the whole role of the assumption, and it is worth noticing where it enters.

What is left is ψnβˆ—Οˆnβ€²β€²βˆ’Οˆnψnβˆ—β€²β€²\psi_n^*\psi_n'' - \psi_n\psi_n^{*\prime\prime}, and the trick is the same one problem 8 of chapter 3 used: that combination is a perfect derivative, equal to ddx[ψnβˆ—Οˆnβ€²βˆ’Οˆnψnβˆ—β€²]\frac{\mathrm d}{\mathrm dx}[\psi_n^*\psi_n' - \psi_n\psi_n^{*\prime}].

Integrating a perfect derivative gives a boundary term, which dies. So the right-hand side must integrate to zero β€” and ∫∣ψn∣2dx\int|\psi_n|^2\mathrm dx is certainly not zero.

βœ“ Worked solution

Multiplying and subtracting, the Vψnβˆ—ΟˆnV\psi_n^*\psi_n terms cancel exactly since VV is real, leaving

βˆ’β„22m[ψnβˆ—d2ψndx2βˆ’Οˆnd2ψnβˆ—dx2]=(Enβˆ’Enβˆ—)ψnβˆ—Οˆn-\frac{\hbar^2}{2m}\left[\psi_n^*\frac{\mathrm d^2\psi_n}{\mathrm dx^2} - \psi_n\frac{\mathrm d^2\psi_n^*}{\mathrm dx^2}\right] = (E_n - E_n^*)\psi_n^*\psi_n

The bracket is a perfect derivative, giving the stated form. Integrating over all xx:

βˆ’β„22m[ψnβˆ—dψndxβˆ’Οˆndψnβˆ—dx]βˆ’βˆž+∞=(Enβˆ’Enβˆ—)βˆ«βˆ’βˆž+∞∣ψn∣2 dx-\frac{\hbar^2}{2m}\left[\psi_n^*\frac{\mathrm d\psi_n}{\mathrm dx} - \psi_n\frac{\mathrm d\psi_n^*}{\mathrm dx}\right]_{-\infty}^{+\infty} = (E_n - E_n^*)\int_{-\infty}^{+\infty}|\psi_n|^2\,\mathrm dx

The left side vanishes because ψnβ†’0\psi_n \to 0 at infinity. The integral on the right is 1 for a normalized state β€” in any case strictly positive. Therefore

Enβˆ’Enβˆ—=0β‡’EnΒ isΒ realE_n - E_n^* = 0 \quad\Rightarrow\quad E_n \text{ is real}

Why it matters. An energy eigenvalue is something you can measure, and measurements return real numbers. This shows the formalism delivers that automatically, provided VV is real. Make VV complex and the argument fails β€” which is exactly how absorption is modelled, with the imaginary part giving states a finite lifetime.

2 Eigenfunctions of different eigenvalues are orthogonal derivation

For a real potential, ψn\psi_n and ψmβˆ—\psi_m^* satisfy

[βˆ’β„22md2dx2+V]ψn=Enψnand[βˆ’β„22md2dx2+V]ψmβˆ—=Emψmβˆ—\left[-\frac{\hbar^2}{2m}\frac{\mathrm d^2}{\mathrm dx^2} + V\right]\psi_n = E_n\psi_n \quad\text{and}\quad \left[-\frac{\hbar^2}{2m}\frac{\mathrm d^2}{\mathrm dx^2} + V\right]\psi_m^* = E_m\psi_m^*

Multiply the first by ψmβˆ—\psi_m^* and the second by ψn\psi_n, subtract, and show

βˆ’β„22mddx[ψmβˆ—dψndxβˆ’Οˆndψmβˆ—dx]=(Enβˆ’Em)ψmβˆ—Οˆn-\frac{\hbar^2}{2m}\frac{\mathrm d}{\mathrm dx}\left[\psi_m^*\frac{\mathrm d\psi_n}{\mathrm dx} - \psi_n\frac{\mathrm d\psi_m^*}{\mathrm dx}\right] = (E_n - E_m)\psi_m^*\psi_n

Integrating and assuming both vanish at infinity, show that βˆ«βˆ’βˆžβˆžΟˆmβˆ—Οˆn dx=0\int_{-\infty}^{\infty}\psi_m^*\psi_n\,\mathrm dx = 0 if Emβ‰ EnE_m \ne E_n.

πŸ’‘ Phillips' own hint

Structurally identical to problem 1 β€” the only change is that the second equation involves a different eigenfunction, so what appears on the right is (Enβˆ’Em)(E_n - E_m) rather than (Enβˆ’Enβˆ—)(E_n - E_n^*).

Note that the second equation has EmE_m and not Emβˆ—E_m^*: problem 1 has already established the eigenvalues are real, so you are entitled to that. The two problems are in this order for a reason.

βœ“ Worked solution

The VV terms cancel as before, the bracket is again a perfect derivative, and integrating kills the boundary term:

0=(Enβˆ’Em)βˆ«βˆ’βˆž+∞ψmβˆ—Οˆn dx0 = (E_n - E_m)\int_{-\infty}^{+\infty}\psi_m^*\psi_n\,\mathrm dx

If Em≠EnE_m \ne E_n the prefactor is non-zero, so the integral must vanish. That is Eq. (4.49).

What it does not cover. If Em=EnE_m = E_n β€” a degenerate level β€” the prefactor is zero and the equation says nothing at all. That is precisely the gap Β§4.5 acknowledges: eigenfunctions of a degenerate eigenvalue are not uniquely determined, and you must choose an orthogonal set (Gram–Schmidt). The proof does not fail there; it simply has no content.

Why it matters. Orthogonality is what makes the expansion coefficients extractable at all β€” every step of Eq. (4.51) depends on the cross terms vanishing.

Group 2 β€” applying the box formula

3 The energy gap, atomic and nuclear numerical

What is the energy difference between the lowest and first excited state of a particle of mass mm in a one-dimensional infinite square well of width aa? Evaluate this energy:

(a) for an electron in a well of atomic size, in eV;

(b) for a neutron in a well of nuclear size, in MeV.

πŸ’‘ Phillips' own hint

From Eq. (4.38), E2βˆ’E1=(4βˆ’1)Ο€2ℏ2/2ma2=3Ο€2ℏ2/2ma2E_2 - E_1 = (4-1)\pi^2\hbar^2/2ma^2 = 3\pi^2\hbar^2/2ma^2.

Phillips’ own hint: for (a) take a=a0a = a_0, the Bohr radius, and note that the Rydberg energy is ER=ℏ2/2mea02=13.6E_R = \hbar^2/2m_ea_0^2 = 13.6 eV β€” so the answer is just 3Ο€2ER3\pi^2 E_R and needs no calculator.

For (b) take a=1a = 1 fm =10βˆ’15= 10^{-15} m, and remember the neutron is about 1839 times heavier than an electron.

βœ“ Worked solution
E2βˆ’E1=3Ο€2ℏ22ma2E_2 - E_1 = \frac{3\pi^2\hbar^2}{2ma^2}

(a) With a=a0a = a_0 the bracket is exactly the Rydberg energy:

E2βˆ’E1=3Ο€2Γ—13.6Β eVβ‰ˆ403Β eVE_2 - E_1 = 3\pi^2 \times 13.6\ \mathrm{eV} \approx 403\ \mathrm{eV}

The right order for atomic physics β€” soft X-ray. The crude box overestimates real atomic transitions (a few eV) because a real atom’s potential is a smooth Coulomb well rather than hard walls, but the scale is right.

(b) With a=1a = 1 fm and m=mnm = m_n:

E2βˆ’E1β‰ˆ614Β MeVE_2 - E_1 \approx 614\ \mathrm{MeV}

The point of the pair. Same formula, no new physics, and six orders of magnitude between them. The mass rises by 1839 (lowering the levels) but the box shrinks by a factor of 5Γ—1055\times10^5, and that enters squared. Confinement scale alone explains why atomic physics is measured in eV and nuclear physics in MeV.

4 A standing wave is two travelling waves derivation

The wave functions for a particle with energy EnE_n in an infinite square well are Ξ¨n(x,t)=Nsin⁑knx eβˆ’iEnt/ℏ\Psi_n(x,t) = N\sin k_nx\,e^{-iE_nt/\hbar}. Show that these can be thought of as standing waves formed by a linear superposition of travelling waves trapped in the region 0<x<a0 < x < a.

πŸ’‘ Phillips' own hint

Phillips’ hint is the whole problem: rewrite using

sin⁑knx=e+iknxβˆ’eβˆ’iknx2i\sin k_nx = \frac{e^{+ik_nx} - e^{-ik_nx}}{2i}

Then read off what each of the two resulting terms is.

βœ“ Worked solution
Ξ¨n(x,t)=N2i[e+i(knxβˆ’Ent/ℏ)βˆ’eβˆ’i(knx+Ent/ℏ)]\Psi_n(x,t) = \frac{N}{2i}\left[e^{+i(k_nx - E_nt/\hbar)} - e^{-i(k_nx + E_nt/\hbar)}\right]

The first term is a plane wave travelling to the right with momentum +ℏkn+\hbar k_n; the second travels to the left with βˆ’β„kn-\hbar k_n. Equal amplitudes, so the standing wave is an equal superposition of the two.

This is Β§3.4’s momentum result, arrived at from the other direction. There, transforming sin⁑knx\sin k_nx gave two momentum peaks near Β±nℏπ/a\pm n\hbar\pi/a; here the same fact is visible in one line of algebra. And it explains why ⟨p⟩=0\langle p\rangle = 0 while Ξ”pβ‰ 0\Delta p \ne 0: the two travelling waves cancel in the mean and add in the spread.

A caution about the picture. It is tempting to say the particle β€œbounces back and forth”. Nothing in the formalism supports that: ∣Ψ∣2|\Psi|^2 is completely static, so there is no bouncing to observe. The superposition is of two momentum possibilities, not two phases of a journey.

5 A two-dimensional box, and an accidental degeneracy numerical

A particle of mass mm in a two-dimensional box with V=0V = 0 for 0<x<a0 < x < a, 0<y<b0 < y < b and ∞\infty elsewhere. States of definite energy carry two quantum numbers.

(a) Find the eigenfunctions ψnx,ny(x,y)\psi_{n_x,n_y}(x,y) and eigenvalues Enx,nyE_{n_x,n_y}.

(b) Draw diagrams showing the first four energy levels for a=ba = b and for a=2ba = 2b, indicating the degeneracy of each.

πŸ’‘ Phillips' own hint

For (a), separate again: ψ=X(x)Y(y)\psi = X(x)Y(y), and each factor is a 1-D box eigenfunction. The energies add.

For (b), work in units of Ο€2ℏ2/2ma2\pi^2\hbar^2/2ma^2 so that E=nx2+ny2(a/b)2E = n_x^2 + n_y^2(a/b)^2. Then a=ba = b gives nx2+ny2n_x^2 + n_y^2 and a=2ba = 2b gives nx2+4ny2n_x^2 + 4n_y^2. List the small values and count how many (nx,ny)(n_x,n_y) give each.

βœ“ Worked solution

(a) The two-dimensional versions of Eqs. (4.43) and (4.44):

ψnx,ny(x,y)=Nsin⁑(nxΟ€xa)sin⁑(nyΟ€yb),Enx,ny=Ο€2ℏ22m[nx2a2+ny2b2]\psi_{n_x,n_y}(x,y) = N\sin\left(\frac{n_x\pi x}{a}\right)\sin\left(\frac{n_y\pi y}{b}\right),\qquad E_{n_x,n_y} = \frac{\pi^2\hbar^2}{2m}\left[\frac{n_x^2}{a^2} + \frac{n_y^2}{b^2}\right]

(b) In units of Ο€2ℏ2/2ma2\pi^2\hbar^2/2ma^2:

first four levels
a=ba = b2 (Γ—1, 11) Β· 5 (Γ—2, 21) Β· 8 (Γ—1, 22) Β· 10 (Γ—2, 31)
a=2ba = 2b5 (Γ—1) Β· 8 (Γ—1) Β· 13 (Γ—1) Β· 17 (Γ—1) β€” all non-degenerate

The square box has degeneracies for the reason Β§4.4 gives: swapping xx and yy is a symmetry, so (1,2)(1,2) and (2,1)(2,1) must share an energy. Stretch it to a=2ba = 2b and that symmetry is gone, and so are the degeneracies.

Group 3 β€” superposition

6 A specified expectation value derivation

Two states of definite energy E1E_1 and E2E_2 are represented by the normalized, orthogonal solutions Ξ¨1=ψ1eβˆ’iE1t/ℏ\Psi_1 = \psi_1e^{-iE_1t/\hbar} and Ξ¨2=ψ2eβˆ’iE2t/ℏ\Psi_2 = \psi_2e^{-iE_2t/\hbar}.

(a) Write down a superposition of Ξ¨1\Psi_1 and Ξ¨2\Psi_2 for which the expectation value of the energy is 14E1+34E2\tfrac14E_1 + \tfrac34E_2.

(b) Find the uncertainty in energy for that state.

(c) Show that its probability density oscillates with time, and relate the period of oscillation to the energy uncertainty.

πŸ’‘ Phillips' own hint

For (a), Eq. (4.54) says ⟨E⟩=βˆ‘βˆ£cn∣2En\langle E\rangle = \sum|c_n|^2E_n, so you need ∣c1∣2=14|c_1|^2 = \tfrac14 and ∣c2∣2=34|c_2|^2 = \tfrac34. Take the coefficients real and positive.

For (c), follow Eq. (4.57)β€˜s worked example and modify: the cross terms carry eΒ±i(E1βˆ’E2)t/ℏe^{\pm i(E_1-E_2)t/\hbar} whatever the coefficients are, so the period does not depend on the mixing at all β€” only the amplitude of the oscillation does.

βœ“ Worked solution

(a) ∣c1∣2=14|c_1|^2 = \tfrac14 and ∣c2∣2=34|c_2|^2 = \tfrac34 give

Ξ¨=12β€‰Οˆ1eβˆ’iE1t/ℏ+32β€‰Οˆ2eβˆ’iE2t/ℏ\Psi = \tfrac12\,\psi_1e^{-iE_1t/\hbar} + \tfrac{\sqrt3}{2}\,\psi_2e^{-iE_2t/\hbar}

which is normalized since 14+34=1\tfrac14 + \tfrac34 = 1.

(b) ⟨E2⟩=14E12+34E22\langle E^2\rangle = \tfrac14E_1^2 + \tfrac34E_2^2, so

(Ξ”E)2=14E12+34E22βˆ’(14E1+34E2)2=316(E1βˆ’E2)2(\Delta E)^2 = \tfrac14E_1^2 + \tfrac34E_2^2 - \left(\tfrac14E_1 + \tfrac34E_2\right)^2 = \tfrac{3}{16}(E_1-E_2)^2Ξ”E=34∣E1βˆ’E2∣\Delta E = \frac{\sqrt3}{4}|E_1 - E_2|

Compare Eq. (4.57)β€˜s equal mix, which gave 12∣E1βˆ’E2∣\tfrac12|E_1-E_2|. An uneven split has a smaller spread β€” sensible, since pushing all the weight onto one level would give Ξ”E=0\Delta E = 0.

(c)

∣Ψ∣2=14∣ψ1∣2+34∣ψ2∣2+34[ψ1βˆ—Οˆ2e+i(E1βˆ’E2)t/ℏ+c.c.]|\Psi|^2 = \tfrac14|\psi_1|^2 + \tfrac34|\psi_2|^2 + \tfrac{\sqrt3}{4}\left[\psi_1^*\psi_2e^{+i(E_1-E_2)t/\hbar} + \text{c.c.}\right]

The cross term oscillates at ∣E1βˆ’E2∣/ℏ|E_1-E_2|/\hbar, so the period is T=2πℏ/∣E1βˆ’E2∣T = 2\pi\hbar/|E_1-E_2|. Substituting ∣E1βˆ’E2∣=4Ξ”E/3|E_1-E_2| = 4\Delta E/\sqrt3:

T=3 πℏ2Ξ”ET = \frac{\sqrt3\,\pi\hbar}{2\Delta E}

which is Ξ΄t ΔEβ‰ˆβ„\delta t\,\Delta E \approx \hbar again, with the numerical factor depending on the mixing. The period is set by the level separation, not by the mixing; only the depth of the oscillation depends on the coefficients.

Problem 6's state, running

00.20.40.60.81.000.51.01.52.02.5position x (units of a)probability density |Ψ|²⟨x⟩

⟨x⟩ over one revival period T = 4maΒ²/Ο€Δ§

00.20.40.60.81.01.20.30.40.50.60.7time t⟨x⟩
⟨E⟩ 16.038
Ξ”E 6.411
period Ο€Δ§/Ξ”E 0.490
t 0.000

2 energies β€” a non-stationary state. The cross terms carry eΒ±i(Eβ‚˜βˆ’Eβ‚™)t/Δ§ and do not cancel, so |Ξ¨|Β² sloshes and ⟨x⟩ oscillates. More energy uncertainty means faster change β€” that is Eq. (4.58), Ξ΄tΒ·Ξ”E β‰ˆ Δ§, and you can watch the period shorten as you push Ξ”E up.

c₁ = Β½ and cβ‚‚ = √3/2, so |c₁|Β² = ΒΌ and |cβ‚‚|Β² = ΒΎ and ⟨E⟩ = E₁/4 + 3Eβ‚‚/4 as required. Compare it with the equal mix (the '1 + 2' preset): the period is identical because the level separation is, but the sloshing is shallower β€” an uneven split means less interference, hence a smaller Ξ”E.

7 Orthonormality and the Fourier coefficients derivation

The eigenfunctions of a particle in a 1-D infinite square well of width aa are ψn(x)=Nsin⁑knx\psi_n(x) = N\sin k_nx with kn=nΟ€/ak_n = n\pi/a.

(a) Show that ∫0a∣ψn∣2dx=1\int_0^a|\psi_n|^2\mathrm dx = 1 is satisfied by N=2/aN = \sqrt{2/a}.

(b) Show that ∫0aψmβˆ—Οˆn dx=0\int_0^a\psi_m^*\psi_n\,\mathrm dx = 0 if mβ‰ nm \ne n.

(c) For the Fourier sine series f(x)=βˆ‘ncnψn(x)f(x) = \sum_n c_n\psi_n(x) on 0<x<a0 < x < a, show that

cn=2a∫0asin⁑knx f(x) dxc_n = \frac{2}{a}\int_0^a\sin k_nx\,f(x)\,\mathrm dx
πŸ’‘ Phillips' own hint

(a) uses sin⁑2ΞΈ=12(1βˆ’cos⁑2ΞΈ)\sin^2\theta = \tfrac12(1 - \cos2\theta), and the cosine integrates to zero over a whole number of half-periods.

(b) uses sin⁑Asin⁑B=12[cos⁑(Aβˆ’B)βˆ’cos⁑(A+B)]\sin A\sin B = \tfrac12[\cos(A-B) - \cos(A+B)], and both cosines integrate to zero when mβ‰ nm \ne n β€” check what goes wrong when m=nm = n, since that is exactly why the two cases differ.

(c) is Eq. (4.51) specialised: project with ψn\psi_n and substitute N=2/aN = \sqrt{2/a}. Note the 2/a2/a in the answer is N2N^2, not NN.

βœ“ Worked solution

(a) ∫0asin⁑2knx dx=a2\displaystyle\int_0^a\sin^2k_nx\,\mathrm dx = \frac{a}{2} (the mean of sin⁑2\sin^2 is 12\tfrac12 over a whole number of half-periods, which kn=nΟ€/ak_n = n\pi/a guarantees). So N2a/2=1N^2a/2 = 1 and N=2/aN = \sqrt{2/a}.

(b) With the product-to-sum identity,

∫0asin⁑kmxsin⁑knx dx=12∫0a[cos⁑(mβˆ’n)Ο€xaβˆ’cos⁑(m+n)Ο€xa]dx\int_0^a\sin k_mx\sin k_nx\,\mathrm dx = \frac12\int_0^a\left[\cos\frac{(m-n)\pi x}{a} - \cos\frac{(m+n)\pi x}{a}\right]\mathrm dx

Each cosine has an integer number of full periods in [0,a][0,a] and integrates to zero β€” provided mβ‰ nm \ne n. When m=nm = n the first cosine becomes cos⁑0=1\cos 0 = 1 and contributes a/2a/2, which is exactly part (a).

(c) Multiply the series by ψn\psi_n and integrate; orthogonality leaves one term:

∫0aψnf dx=cnβ‡’cn=2a∫0asin⁑knx f(x) dx\int_0^a\psi_nf\,\mathrm dx = c_n \quad\Rightarrow\quad c_n = \sqrt{\frac2a}\int_0^a\sin k_nx\,f(x)\,\mathrm dx

With the book’s convention of absorbing NN into ψn\psi_n so that f=βˆ‘cnsin⁑knxf = \sum c_n\sin k_nx, this becomes cn=2a∫0asin⁑knx f dxc_n = \frac2a\int_0^a\sin k_nx\,f\,\mathrm dx β€” the standard Fourier sine coefficient.

8 The well suddenly doubles in width numerical

A particle is in the ground state of an infinite square well of width a/2a/2, so at t=0t = 0

Ξ¨(x,0)={4a sin⁑2Ο€xaifΒ 0<x<a/20elsewhere\Psi(x,0) = \begin{cases}\sqrt{\dfrac4a}\,\sin\dfrac{2\pi x}{a} & \text{if } 0 < x < a/2\\[4pt] 0 & \text{elsewhere}\end{cases}

The well then suddenly widens to aa, without affecting the wave function. By writing Ξ¨\Psi as a superposition of the new eigenfunctions, find the probability that a subsequent energy measurement gives E1=Ο€2ℏ2/2ma2E_1 = \pi^2\hbar^2/2ma^2.

πŸ’‘ Phillips' own hint

The wave function does not change at the instant the wall moves β€” only the Hamiltonian does. So the same Ξ¨(x,0)\Psi(x,0) must now be expanded in the eigenfunctions of the wider well.

By Eq. (4.51), c1=∫0aψ1βˆ—Ξ¨(x,0) dxc_1 = \int_0^a\psi_1^*\Psi(x,0)\,\mathrm dx, and Ξ¨\Psi is zero beyond a/2a/2, so the integral only runs to a/2a/2. Use the product-to-sum identity, and note that sin⁑(Ο€x/a)\sin(\pi x/a) and sin⁑(2Ο€x/a)\sin(2\pi x/a) are not orthogonal over the half-interval β€” orthogonality holds on [0,a][0,a], not [0,a/2][0,a/2].

βœ“ Worked solution
c1=∫0a/22asin⁑πxaβ‹…4asin⁑2Ο€xa dx=22a∫0a/2sin⁑πxasin⁑2Ο€xa dxc_1 = \int_0^{a/2}\sqrt{\frac2a}\sin\frac{\pi x}{a}\cdot\sqrt{\frac4a}\sin\frac{2\pi x}{a}\,\mathrm dx = \frac{2\sqrt2}{a}\int_0^{a/2}\sin\frac{\pi x}{a}\sin\frac{2\pi x}{a}\,\mathrm dx

Using sin⁑Asin⁑B=12[cos⁑(Aβˆ’B)βˆ’cos⁑(A+B)]\sin A\sin B = \tfrac12[\cos(A-B) - \cos(A+B)]:

=2a[aΟ€sin⁑πxaβˆ’a3Ο€sin⁑3Ο€xa]0a/2=2Ο€[1+13]=423Ο€= \frac{\sqrt2}{a}\left[\frac{a}{\pi}\sin\frac{\pi x}{a} - \frac{a}{3\pi}\sin\frac{3\pi x}{a}\right]_0^{a/2} = \frac{\sqrt2}{\pi}\left[1 + \frac13\right] = \frac{4\sqrt2}{3\pi}P(E1)=∣c1∣2=329Ο€2β‰ˆ0.360P(E_1) = |c_1|^2 = \frac{32}{9\pi^2} \approx 0.360

Worth computing the rest. ∣c2∣2=12|c_2|^2 = \tfrac12 exactly, and ∣c4∣2=0|c_4|^2 = 0 exactly β€” as does every even nn except 2.

9 The revival time derivation

The general wave function of a particle in a 1-D infinite square well of width aa is Ξ¨(x,t)=βˆ‘ncnψn(x)eβˆ’iEnt/ℏ\Psi(x,t) = \sum_n c_n\psi_n(x)e^{-iE_nt/\hbar} with En=n2Ο€2ℏ2/2ma2E_n = n^2\pi^2\hbar^2/2ma^2. Show that the wave function returns to its original form after a time

T=4ma2πℏT = \frac{4ma^2}{\pi\hbar}
πŸ’‘ Phillips' own hint

Phillips’ hint: show that eβˆ’iEnT/ℏ=1e^{-iE_nT/\hbar} = 1, and then Ξ¨(t+T)=Ξ¨(t)\Psi(t + T) = \Psi(t) follows for every term at once.

You need EnT/ℏE_nT/\hbar to be an integer multiple of 2Ο€2\pi β€” for every nn simultaneously. Substitute and see what the nn-dependence does.

βœ“ Worked solution
EnTℏ=n2Ο€2ℏ2ma2β‹…4ma2πℏ=2Ο€n2\frac{E_nT}{\hbar} = \frac{n^2\pi^2\hbar}{2ma^2}\cdot\frac{4ma^2}{\pi\hbar} = 2\pi n^2

Since nn is an integer, n2n^2 is an integer, and eβˆ’i2Ο€n2=1e^{-i2\pi n^2} = 1 for every nn. Every term of the superposition therefore returns to its t=0t = 0 value at the same instant, so Ξ¨(x,T)=Ξ¨(x,0)\Psi(x, T) = \Psi(x, 0) exactly β€” and the motion is periodic with period TT.

The essential ingredient is that En∝n2E_n \propto n^2. The ratio of any two energies is a ratio of integers, so all the phases are commensurate. A potential whose levels are not in rational ratios has no exact revival β€” the state comes arbitrarily close to its initial form but never returns to it.

The widget on §4.6 traces ⟨x⟩\langle x\rangle over exactly this period, which is why that curve closes.

Group 4 β€” energy uncertainty as a measurement

10 Natural line width in wavelength derivation

Radiation of wavelength Ξ»\lambda is emitted when an atom drops from energy E2E_2 to a ground state E1E_1. If the mean lifetime of the upper state is Ο„\tau, show that the uncertainty in the emitted wavelength β€” the natural line width β€” is

Δλ=Ξ»22Ο€cΟ„\Delta\lambda = \frac{\lambda^2}{2\pi c\tau}
πŸ’‘ Phillips' own hint

Two ingredients: hc/Ξ»=E2βˆ’E1hc/\lambda = E_2 - E_1, and Ξ”E2=ℏ/Ο„\Delta E_2 = \hbar/\tau from Eq. (4.59).

Differentiate the first to relate Δλ\Delta\lambda to Ξ”E\Delta E, then substitute. Watch the difference between hh and ℏ\hbar β€” that factor of 2Ο€2\pi is where the answer’s 2Ο€2\pi comes from.

βœ“ Worked solution

From E2βˆ’E1=hc/Ξ»E_2 - E_1 = hc/\lambda,

βˆ£Ξ”E∣=hcΞ»2Δλ⇒Δλ=Ξ»2hcΞ”E|\Delta E| = \frac{hc}{\lambda^2}\Delta\lambda \quad\Rightarrow\quad \Delta\lambda = \frac{\lambda^2}{hc}\Delta E

Substituting Ξ”E=ℏ/Ο„\Delta E = \hbar/\tau and ℏ=h/2Ο€\hbar = h/2\pi:

Δλ=Ξ»2hc⋅ℏτ=Ξ»22Ο€cΟ„\Delta\lambda = \frac{\lambda^2}{hc}\cdot\frac{\hbar}{\tau} = \frac{\lambda^2}{2\pi c\tau}

Note what it does not contain. Δλ\Delta\lambda depends on Ξ»\lambda and Ο„\tau but not on the atom, the transition, or the intensity β€” it is fixed entirely by how long the state lives.

11 The lifetime of the Z boson numerical

The Z boson is an unstable gauge boson mediating the weak nuclear interaction. The fundamental uncertainty in its mass energy is Ξ”E=2.5\Delta E = 2.5 GeV. Evaluate its mean decay lifetime.

πŸ’‘ Phillips' own hint

Direct application of Eq. (4.59) rearranged: Ο„=ℏ/Ξ”E\tau = \hbar/\Delta E.

Use ℏ=6.582Γ—10βˆ’16\hbar = 6.582\times10^{-16} eV s, which saves converting to joules.

βœ“ Worked solution
Ο„=ℏΔE=6.582Γ—10βˆ’16Β eV s2.5Γ—109Β eVβ‰ˆ2.6Γ—10βˆ’25Β s\tau = \frac{\hbar}{\Delta E} = \frac{6.582\times10^{-16}\ \mathrm{eV\,s}}{2.5\times10^{9}\ \mathrm{eV}} \approx 2.6\times10^{-25}\ \mathrm{s}

Read the relation backwards. No clock can time 10βˆ’2510^{-25} s, and no detector can see a particle whose decay length is cΟ„β‰ˆ8Γ—10βˆ’17c\tau \approx 8\times10^{-17} m β€” a thousandth of a proton radius. The Z is never observed to travel; it is created and decays at the same point.

So its lifetime is not measured. Its width is: experiments scan the collision energy and record the resonance peak’s shape, and Ξ”E=2.5\Delta E = 2.5 GeV is that measured width. Equation (4.59) then converts it into a lifetime that could not be observed any other way.

Note the scale: 2.5 GeV against a mass energy of 91.2 GeV means the Z’s mass is uncertain by 2.7% of itself. A β€œparticle” too short-lived to have a well-defined mass.

Chapter 4 is complete

Energy is described by an operator that also drives time evolution; confinement quantizes it; eigenfunctions form a basis; and the expansion coefficients are probability amplitudes.

Chapter 5 applies all of it to the harmonic oscillator β€” the potential that approximates every smooth minimum, and whose spectrum is evenly spaced rather than going as n2n^2. That difference has a consequence problem 9 makes easy to anticipate: with equally spaced levels, every superposition revives, and it does so at the classical oscillation period.

Check yourself

0 / 8 answered

  1. 1.In problems 1 and 2, where exactly does the assumption that is real get used?

  2. 2.Problem 2 proves when . What happens when ?

  3. 3.Problem 3 gives ~403 eV for an electron in an atom-sized box and ~614 MeV for a neutron in a nucleus-sized one. What drives the six orders of magnitude?

  4. 4.For the box, the first four levels are non-degenerate β€” yet . What is that?

  5. 5.In problem 8 the well suddenly doubles in width. Why does the energy become uncertain when it was definite before?

  6. 6.In problem 8, exactly and exactly. Why are the even coefficients so clean?

  7. 7.Problem 9's revival at works because . What is essential about that?

  8. 8.The Z boson's lifetime comes out as s. How is that actually established experimentally?