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. 1β2 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. 3β5 apply at atomic and nuclear scales and in two dimensions. 6β9 exercise superposition, including the two most interesting problems in the set: a well that suddenly doubles in width, and the revival time. 10β11 turn into measurements.
Group 1 β the two deferred proofs
In practice the potential energy function for a particle is a real function. Show that this implies the energy eigenvalues are real.
The eigenfunction and its complex conjugate satisfy
Multiply the first by and the second by , subtract, and show
By integrating over and assuming is zero at , show that .
π‘ Phillips' own hint
The terms cancel in the subtraction because is real β that is the whole role of the assumption, and it is worth noticing where it enters.
What is left is , and the trick is the same one problem 8 of chapter 3 used: that combination is a perfect derivative, equal to .
Integrating a perfect derivative gives a boundary term, which dies. So the right-hand side must integrate to zero β and is certainly not zero.
β Worked solution
Multiplying and subtracting, the terms cancel exactly since is real, leaving
The bracket is a perfect derivative, giving the stated form. Integrating over all :
The left side vanishes because at infinity. The integral on the right is 1 for a normalized state β in any case strictly positive. Therefore
Why it matters. An energy eigenvalue is something you can measure, and measurements return real numbers. This shows the formalism delivers that automatically, provided is real. Make complex and the argument fails β which is exactly how absorption is modelled, with the imaginary part giving states a finite lifetime.
For a real potential, and satisfy
Multiply the first by and the second by , subtract, and show
Integrating and assuming both vanish at infinity, show that if .
π‘ 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 rather than .
Note that the second equation has and not : 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.
β Worked solution
The terms cancel as before, the bracket is again a perfect derivative, and integrating kills the boundary term:
If the prefactor is non-zero, so the integral must vanish. That is Eq. (4.49).
What it does not cover. If 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 (GramβSchmidt). 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
What is the energy difference between the lowest and first excited state of a particle of mass in a one-dimensional infinite square well of width ? 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.
π‘ Phillips' own hint
From Eq. (4.38), .
Phillipsβ own hint: for (a) take , the Bohr radius, and note that the Rydberg energy is eV β so the answer is just and needs no calculator.
For (b) take fm m, and remember the neutron is about 1839 times heavier than an electron.
β Worked solution
(a) With the bracket is exactly the Rydberg energy:
The right order for atomic physics β soft X-ray. The crude box overestimates real atomic transitions (a few eV) because a real atomβs potential is a smooth Coulomb well rather than hard walls, but the scale is right.
(b) With fm and :
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 , and that enters squared. Confinement scale alone explains why atomic physics is measured in eV and nuclear physics in MeV.
The wave functions for a particle with energy in an infinite square well are . Show that these can be thought of as standing waves formed by a linear superposition of travelling waves trapped in the region .
π‘ Phillips' own hint
Phillipsβ hint is the whole problem: rewrite using
Then read off what each of the two resulting terms is.
β Worked solution
The first term is a plane wave travelling to the right with momentum ; the second travels to the left with . Equal amplitudes, so the standing wave is an equal superposition of the two.
This is Β§3.4βs momentum result, arrived at from the other direction. There, transforming gave two momentum peaks near ; here the same fact is visible in one line of algebra. And it explains why while : 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 βbounces back and forthβ. Nothing in the formalism supports that: is completely static, so there is no bouncing to observe. The superposition is of two momentum possibilities, not two phases of a journey.
A particle of mass in a two-dimensional box with for , and elsewhere. States of definite energy carry two quantum numbers.
(a) Find the eigenfunctions and eigenvalues .
(b) Draw diagrams showing the first four energy levels for and for , indicating the degeneracy degeneracy Several independent eigenfunctions sharing one eigenvalue. It comes from symmetry β a cubical box has it, a box with unequal sides does not β which is why breaking a symmetry splits levels. defined in ch. 4 β open in glossary of each.
π‘ Phillips' own hint
For (a), separate again: , and each factor is a 1-D box eigenfunction. The energies add.
For (b), work in units of so that . Then gives and gives . List the small values and count how many give each.
β Worked solution
(a) The two-dimensional versions of Eqs. (4.43) and (4.44):
(b) In units of :
| first four levels | |
|---|---|
| 2 (Γ1, 11) Β· 5 (Γ2, 21) Β· 8 (Γ1, 22) Β· 10 (Γ2, 31) | |
| 5 (Γ1) Β· 8 (Γ1) Β· 13 (Γ1) Β· 17 (Γ1) β all non-degenerate |
The square box has degeneracies for the reason Β§4.4 gives: swapping and is a symmetry, so and must share an energy. Stretch it to and that symmetry is gone, and so are the degeneracies.
Group 3 β superposition
Two states of definite energy and are represented by the normalized, orthogonal solutions and .
(a) Write down a superposition of and for which the expectation value of the energy is .
(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.
π‘ Phillips' own hint
For (a), Eq. (4.54) says , so you need and . Take the coefficients real and positive.
For (c), follow Eq. (4.57)βs worked example and modify: the cross terms carry whatever the coefficients are, so the period does not depend on the mixing at all β only the amplitude of the oscillation does.
β Worked solution
(a) and give
which is normalized since .
(b) , so
Compare Eq. (4.57)βs equal mix, which gave . An uneven split has a smaller spread β sensible, since pushing all the weight onto one level would give .
(c)
The cross term oscillates at , so the period is . Substituting :
which is 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.
The eigenfunctions of a particle in a 1-D infinite square well of width are with .
(a) Show that is satisfied by .
(b) Show that if .
(c) For the Fourier sine series on , show that
π‘ Phillips' own hint
(a) uses , and the cosine integrates to zero over a whole number of half-periods.
(b) uses , and both cosines integrate to zero when β check what goes wrong when , since that is exactly why the two cases differ.
(c) is Eq. (4.51) specialised: project with and substitute . Note the in the answer is , not .
β Worked solution
(a) (the mean of is over a whole number of half-periods, which guarantees). So and .
(b) With the product-to-sum identity,
Each cosine has an integer number of full periods in and integrates to zero β provided . When the first cosine becomes and contributes , which is exactly part (a).
(c) Multiply the series by and integrate; orthogonality leaves one term:
With the bookβs convention of absorbing into so that , this becomes β the standard Fourier sine coefficient.
A particle is in the ground state of an infinite square well of width , so at
The well then suddenly widens to , without affecting the wave function. By writing as a superposition of the new eigenfunctions, find the probability that a subsequent energy measurement gives .
π‘ Phillips' own hint
The wave function does not change at the instant the wall moves β only the Hamiltonian does. So the same must now be expanded in the eigenfunctions of the wider well.
By Eq. (4.51), , and is zero beyond , so the integral only runs to . Use the product-to-sum identity, and note that and are not orthogonal over the half-interval β orthogonality holds on , not .
β Worked solution
Using :
Worth computing the rest. exactly, and exactly β as does every even except 2.
The general wave function of a particle in a 1-D infinite square well of width is with . Show that the wave function returns to its original form after a time
π‘ Phillips' own hint
Phillipsβ hint: show that , and then follows for every term at once.
You need to be an integer multiple of β for every simultaneously. Substitute and see what the -dependence does.
β Worked solution
Since is an integer, is an integer, and for every . Every term of the superposition therefore returns to its value at the same instant, so exactly β and the motion is periodic with period .
The essential ingredient is that . 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 Β§4.6 traces over exactly this period, which is why that curve closes.
Group 4 β energy uncertainty as a measurement
Radiation of wavelength is emitted when an atom drops from energy to a ground state . If the mean lifetime of the upper state is , show that the uncertainty in the emitted wavelength β the natural line width natural line width The unavoidable spectral width of light from a decaying state, ΞE β Δ§/Ο. A short-lived state has a correspondingly uncertain energy. defined in ch. 4 β open in glossary β is
π‘ Phillips' own hint
Two ingredients: , and from Eq. (4.59).
Differentiate the first to relate to , then substitute. Watch the difference between and β that factor of is where the answerβs comes from.
β Worked solution
From ,
Substituting and :
Note what it does not contain. depends on and but not on the atom, the transition, or the intensity β it is fixed entirely by how long the state lives.
The Z boson is an unstable gauge boson mediating the weak nuclear interaction. The fundamental uncertainty in its mass energy is GeV. Evaluate its mean decay lifetime.
π‘ Phillips' own hint
Direct application of Eq. (4.59) rearranged: .
Use eV s, which saves converting to joules.
β Worked solution
Read the relation backwards. No clock can time s, and no detector can see a particle whose decay length is 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 peakβs shape, and 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 Zβs mass is uncertain by 2.7% of itself. A βparticleβ 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 . 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.In problems 1 and 2, where exactly does the assumption that is real get used?
2.Problem 2 proves when . What happens when ?
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.For the box, the first four levels are non-degenerate β yet . What is that?
5.In problem 8 the well suddenly doubles in width. Why does the energy become uncertain when it was definite before?
6.In problem 8, exactly and exactly. Why are the even coefficients so clean?
7.Problem 9's revival at works because . What is essential about that?
8.The Z boson's lifetime comes out as s. How is that actually established experimentally?