The instructive answers here are the ones that come out wrong by a factor of ten thousand rather than by a factor of two.
Twelve problems, each with Phillipsβ own hint from Hints to selected problems (pp. 249β261) and a full worked solution. Both are collapsed β try the problem first; the boxes are there for when you are stuck or want to check.
Every numerical answer below was obtained by running the code shown with it, so the numbers on this page and the numbers your own script prints should agree.
A photon of energy and momentum strikes a stationary electron and is scattered through an angle . For a relativistic electron , and for a photon .
Show, by conserving momentum and energy separately and then combining them, that
π‘ Phillips' own hint
Rewrite the two conservation laws as and , then use the energyβmomentum relation for each particle. Finish with .
β Worked solution
This is the nine-step derivation stepped through on Β§1.1 β open the Compton scattering widget there and work along with it rather than reading a static wall of algebra.
The single move that makes it work: square both conservation laws, then subtract. Squaring turns the vector momentum equation into a scalar one containing (the cosine rule), and the subtraction is exactly what eliminates the two unknowns you do not care about β the recoiling electronβs energy and momentum β because they appear only in the combination , which you already know equals .
The result contains nothing about the incoming photon. That is the physical content: the shift depends only on the scattering angle and the mass of what you hit.
Electromagnetic radiation on a metal surface may eject electrons β the photoelectric effect photoelectric effect Light ejects electrons from a metal only above a threshold frequency, however intense it is β evidence that light delivers energy in hΞ½ lumps rather than continuously. defined in ch. 1 β open in glossary β but only above a threshold frequency. Show this follows if the mechanism is a photonβelectron interaction and there is a minimum energy needed to free an electron.
Magnesium needs at least . Show that light below produces no photoelectrons, however intense.
π‘ Phillips' own hint
If the minimum energy to eject an electron is , the photon must have frequency at least .
β Worked solution
One photon is absorbed by one electron, all or nothing. If the photonβs energy is less than the work function , no single absorption can free an electron β and turning up the intensity only sends more photons, each still too feeble. Hence a sharp threshold at :
That is nm β near ultraviolet. Magnesium is blind to all visible light, however bright.
Why this killed the wave picture. A classical wave deposits energy continuously, so a dim beam should just take longer to accumulate β a delay, never a threshold. And a brighter beam of any colour should work. Both predictions are wrong, and the disagreement is qualitative rather than numerical.
Black-body radiation can be treated as a gas of photons moving at with typical energies of order , so the emitted intensity (in ) is a function of , and only.
Use dimensional analysis to confirm , and find how depends on and .
π‘ Phillips' own hint
is an energy and is an energy Γ length, so is an energy per unit volume, and is an energy per second per unit area.
β Worked solution
Follow the hintβs construction:
- β an energy.
- β an energy Γ length.
- β energyβ΄ / (energyΒ³ Γ lengthΒ³) = energy per unit volume.
- Multiply by a speed and you get energy per second per unit area:
with a pure number dimensional analysis cannot supply. So falls straight out, and
Check it against the measured . Computing gives , and , so . The exact value from the full Planck calculation is .
Dimensional analysis got everything except a factor of β and, as Β§0.2 put it, that is exactly what it promises: the scale, never the pure number.
Β§1.3 built an atomic size from , and . Now try it the classical relativistic way instead: build a length from , and . Show it is possible β and far too small.
π‘ Phillips' own hint
is a rest energy and is a potential energy if is a length, so . Show this equals , where .
β Worked solution
Setting the two energies equal gives the only available length:
β the classical electron radius, about the size of a nucleus, roughly 19 000 times smaller than an atom.
The relationship to is worth seeing, because it says exactly where the factor came from:
Two factors of , each , giving .
An electron in a circular orbit about a proton can be described classically if its angular momentum . Show this holds when the orbit radius satisfies .
π‘ Phillips' own hint
The Coulomb force supplies the centripetal acceleration , and the orbital angular momentum is .
β Worked solution
Balance the forces:
Then
Requiring and squaring:
Assume an electron is located somewhere within a region of atomic size. Estimate the minimum uncertainty in its momentum, and by assuming this uncertainty is comparable with its average momentum, estimate its average kinetic energy.
π‘ Phillips' own hint
A particleβs momentum is at least as big as the uncertainty in its momentum. Use Eq. (1.15).
β Worked solution
Take . Then
and with ,
That is the Rydberg energy. The uncertainty principle alone β no Coulombβs law, no SchrΓΆdinger equation β produces the binding energy of hydrogen to three digits.
A charmed quark of mass is confined to a region about across. Assuming its average momentum is comparable with the minimum uncertainty, show it can be treated non-relativistically, and estimate its average kinetic energy.
π‘ Phillips' own hint
Use the uncertainty principle to show that β and hence the minimum average momentum β is small compared with .
β Worked solution
The clean way is to work in energy units throughout, using the combination β worth memorising, because it turns every nuclear-scale estimate into arithmetic:
Compare with the rest energy :
Since , the quark is non-relativistic and applies:
In 1897 J. J. Thomson passed 200 eV electrons through a pair of plates 2 cm apart and concluded electrons are particles. In 1927 his son G. P. Thomson concluded they are waves. Explain why J. J. saw no evidence of wave behaviour.
π‘ Phillips' own hint
Evaluate the de Broglie wavelength of a 200 eV electron and consider the condition for strong diffraction by a slit.
β Worked solution
From Eq. (1.8), .
Diffraction through an aperture of width spreads the beam by roughly
Four nanoradians. Over a metre of apparatus that is a lateral spread of four nanometres β smaller than an atom, and utterly beyond 1897 instrumentation.
Both Thomsons were right, and neither result contradicts the other. The wave character was present in J. J.βs tube too; his aperture was simply 200 million times too wide to reveal it. G. P. did not use better electrons β he used a better aperture, namely the atomic spacing of a crystal, which is the same size as .
Electrons of energy 54 eV were scattered from a nickel surface whose parallel rows of atoms are apart. Explain the strong scattering observed at .
π‘ Phillips' own hint
Show that a 54 eV electron has . Constructive interference from the surface rows requires ; check that nm, and satisfy it.
β Worked solution
Waves scattered from adjacent rows travel path lengths differing by ; they arrive in step when that difference is a whole number of wavelengths. For :
Agreement to about 1%. Equivalently, solving for the predicted angle, against a measured 50Β°.
This is the experiment that settled it. A prediction from β a formula proposed four years earlier with no experimental support whatsoever β landing within a degree of a measured diffraction peak.
The electrons that carry current in copper have kinetic energies of about 7 eV. Calculate their wavelength and compare it with the spacing between copper atoms, to decide whether their wave nature matters as they move through the metal. (Density ; take the mass of a copper atom as 60 amu.)
π‘ Phillips' own hint
Show that the de Broglie wavelength of a 7 eV electron is 0.46 nm, and that this is comparable with the distance between atoms in copper.
β Worked solution
Wavelength. .
Atomic spacing. Number density , so the typical separation is
The wavelength is about twice the atomic spacing β the same order, not remotely negligible. A conduction electron is therefore strongly diffracted by the lattice, and treating it as a little ball bouncing between atoms is hopeless.
Neutrons from a reactor are brought to thermal equilibrium by repeated collisions in heavy water at . What is their average energy in eV and their typical wavelength? Explain why they are diffracted by crystalline solids.
π‘ Phillips' own hint
Show that the de Broglie wavelength of a neutron with thermal energy is comparable with the distance between atoms in a solid when .
β Worked solution
Atomic spacings in solids are 0.1β0.3 nm, so a room-temperature neutronβs wavelength lands squarely in the range where a crystal lattice acts as a diffraction grating.
Estimate the de Broglie wavelength of an oxygen molecule in air at NTP. Compare it with the average separation between molecules, and explain why the motion of oxygen molecules in air is unaffected by their wave nature.
π‘ Phillips' own hint
Estimate the thermal energy of an oxygen molecule at and show its de Broglie wavelength is much smaller than the typical distance between molecules in air.
β Worked solution
Wavelength. at 273 K, and with :
Separation. At NTP, , so
The separation is about 120 times the wavelength. Each moleculeβs wave is tiny compared with the space it moves through and with everything it might diffract from, so it travels in a straight line between collisions like a classical billiard ball β and the kinetic theory of gases works.
Check yourself
0 / 6 answered
1.Problems 8β12 all ask the same underlying question. What is it?
2.Problem 4 builds a length from , and and gets m. What does that establish?
3.Problem 3 gets with from experiment. The exact answer is . What is the lesson?
4.Problem 10 finds conduction electrons in copper have nm against a 0.22 nm atomic spacing. Why does that matter beyond this problem?
5.In problem 7, does most of the work. What is that number saying?
6.Problem 6 gives the electron in an atom a kinetic energy of about 13.6 eV β exactly the Rydberg energy. How much should you read into that?