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F. Revolutions in Modern Physics: Quantum Mechanics and Special Relativity · Quantum Mechanics

Quantum Mechanics: Unit Review

F1.1 F1.2 F2.1 F2.2 F2.4 F3 F3.1 F3.2About 40 minutes
Learning goals
  • I can solve problems involving photon energy and momentum, the photoelectric effect, the Compton effect, de Broglie wavelengths and hydrogen energy levels.
  • I can describe the experimental evidence for the particle model of light and the wave model of matter.
  • I can explain how quantum mechanics changed scientific thought and led to new technologies.

Words to know

h
Planck's constant, 6.63 × 10⁻³⁴ J·s (4.14 × 10⁻¹⁵ eV·s).
hc
1.24 × 10³ eV·nm, handy for photon energy E (eV) = 1240 ÷ λ (nm).
key equations
E = hf = hc/λ; p = h/λ; E(k,max) = hf − W = eV₀; Δλ = (h/mₑc)(1 − cos θ); λ = h/(mv); Eₙ = −13.6 eV/n²; Δx Δp ≥ h/(4π).

Let's review!

In this unit you followed one of the great revolutions in science. Planck's quanta explained the glow of hot objects. Einstein's photons explained the photoelectric effect, and Compton showed photons carry momentum. Then de Broglie turned the idea around: matter has waves, confirmed by electron diffraction. Bohr's quantized atom explained line spectra, and the uncertainty principle and probability interpretation completed the new picture. You saw how these ideas power solar cells, cameras, LEDs, lasers, electron microscopes and quantum computers, and how the Standard Model describes all known particles.

The sibling unit Special Relativity covers the other revolution of modern physics. This review has questions from every lesson. Try each one, then press Show answer.

How to use this review

Do two or three sections at a time. Keep a sheet with the key constants: h = 6.63 × 10⁻³⁴ J·s, c = 3.00 × 10⁸ m/s, e = 1.60 × 10⁻¹⁹ C, mₑ = 9.11 × 10⁻³¹ kg, hc = 1240 eV·nm. Before calculating, decide whether you are working in joules or electron-volts and stay consistent. For each question you miss, write down why (unit error? wrong formula for a particle vs a photon? sign error with energy levels?) and go back to the lesson named in the section title. Finish with the 10-question quiz.

How the quantum unit fits togetherBlackbody spectrumPlanck: E = nhf (1900)Photoelectric effectEinstein: photons, hf − WCompton effectphoton momentum p = h/λLine spectraBohr: Eₙ = −13.6/n² eVMatter wavesde Broglie: λ = h/pElectron diffractionDavisson-Germer, ThomsonsymmetryWave-particle duality, uncertainty, probability→ technologies: solar cells, cameras, lasers, EMs, qubits; Standard Model
The unit in one picture. Three puzzles about light led to photons; symmetry led de Broglie to matter waves, confirmed by electron diffraction and explaining Bohr's orbits. Together these give wave-particle duality and the technologies built on it.
Evidence for wave and particle behaviourwave behaviourparticle behaviourlightinterference, diffraction,polarizationphotoelectric effect, Comptoneffect, blackbody, pair productionmatter (electrons)electron diffraction(Davisson-Germer, G. P. Thomson)single spots on detectors,definite charge and massBoth light and matter: travel as waves, detected as particles (λ = h/p for both).
Light and matter both show wave and particle behaviour. Know at least one experiment for each box.
Just for fun

Quantum mechanics is the only subject where "it depends on how you look at it" is a completely correct physics answer.

Blackbody Radiation and Planck's Quantum Hypothesis

1

A star's spectrum peaks at 414 nm. Find its surface temperature.

2

What was the ultraviolet catastrophe, and how did Planck resolve it?

3

Find the energy of one quantum for an oscillator at 3.0 × 10¹³ Hz.

Photons: Light Comes in Packets

1

Find the energy of a 310 nm photon in eV and J.

2

A 3.0 mW laser at 532 nm: how many photons per second?

3

Making a beam of green light brighter changes what, in the photon model?

The Photoelectric Effect

1

List the observation about the photoelectric effect that shows a threshold, and explain why the wave model could not account for it.

2

A stopping voltage of 1.6 V is measured. Find E(k,max) in eV and J.

3

Doubling the intensity (above threshold) changes which: the photocurrent or the stopping voltage?

Einstein's Photoelectric Equation: Solving Problems

1

Light of 250 nm falls on aluminium (W = 4.1 eV). Find E(k,max) and V₀.

2

Find the threshold wavelength for a metal with W = 3.1 eV.

3

On an E(k,max) vs f graph, what do the slope and the horizontal intercept represent?

Investigation: Measuring Planck's Constant

1

A best-fit line of V₀ vs f has slope 4.0 × 10⁻¹⁵ V/Hz. Find h and the percent error.

2

Why is h found from the slope rather than from one data point?

3

A blue LED (470 nm) turns on at 2.6 V. Estimate h from this one LED.

Photon Momentum and the Compton Effect

1

Find the momentum of a 0.020 nm X-ray photon.

2

X-rays of 0.0800 nm scatter at 180°. Find the scattered wavelength.

3

Why is the Compton effect evidence for photons?

Wave-Particle Duality of Light

1

In the single-photon double-slit experiment, what is particle-like and what is wave-like?

2

What is the minimum photon energy for electron-positron pair production?

3

How does a PET scanner locate a tracer?

Matter Waves: The de Broglie Wavelength

1

Find the wavelength of an electron moving at 3.0 × 10⁶ m/s.

2

Find the wavelength of an electron accelerated through 400 V.

3

A proton and an electron have the same kinetic energy. Which has the shorter wavelength? Why?

Evidence for Matter Waves: Electron Diffraction

1

Electrons accelerated through 81 V hit a crystal with row spacing 0.250 nm. Find the first-order angle.

2

In an electron diffraction tube, the voltage is reduced. What happens to the rings?

3

Why does the Davisson-Germer experiment support de Broglie's hypothesis?

The Bohr Model and Atomic Spectra

1

Find the wavelength of the 5 → 2 transition in hydrogen.

2

A ground-state hydrogen atom absorbs a photon and jumps to n = 4. What was the photon's energy?

3

How does de Broglie's idea explain Bohr's allowed orbits?

The Uncertainty Principle and the Probability Interpretation

1

An electron's position is known within 0.20 nm. Find the minimum uncertainty in its speed.

2

What does |ψ|² represent?

3

Name one technology that relies on quantum tunnelling.

Quantum Technologies I: Solar Cells, Digital Cameras, LEDs and Lasers

1

A semiconductor has a band gap of 1.9 eV. Find the longest wavelength it can absorb.

2

Explain stimulated emission in one sentence.

3

Give one benefit and one cost of solar panels.

Quantum Technologies II: Electron Microscopes, Quantum Computing and Society

1

Why do electron microscopes have much better resolution than light microscopes?

2

How many amplitudes describe 40 qubits?

3

Why are organizations adopting post-quantum cryptography now?

The Standard Model of Elementary Particles

1

Find the charge of the baryon uus.

2

Does p → n + π⁰ conserve charge? Is it allowed?

3

What did the Sudbury Neutrino Observatory show?

Check your understanding

Quiz

1.

Which experiment provided evidence that light has momentum?

2.

A photon of 4.0 eV strikes a metal with work function 2.5 eV. The stopping voltage is

3.

The wavelength of a photon of energy 2.0 eV is about

4.

If the speed of an electron doubles, its de Broglie wavelength

5.

Which statement about the photoelectric effect is correct?

6.

A hydrogen electron drops from n = 2 to n = 1. The photon emitted has energy

7.

Which experiment is direct evidence for the wave nature of electrons?

8.

According to the uncertainty principle, confining an electron to a smaller region

9.

Electron microscopes resolve finer detail than light microscopes because electrons

10.

Which particle is made of quarks?

For parents and teachers

Use the review to find what to revisit:

  • Wien's law errors, or confusion about what Planck assumed → Lesson 1 (Blackbody Radiation and Planck's Quantum Hypothesis).
  • J ↔ eV slips, or brightness vs photon energy → Lesson 2 (Photons: Light Comes in Packets).
  • Mixing up what intensity and frequency change → Lesson 3 (The Photoelectric Effect).
  • Negative kinetic energies, threshold calculations, graph slopes → Lesson 4 (Einstein's Photoelectric Equation).
  • Reading slopes and intercepts, percent error, sources of error → Lesson 5 (Investigation: Measuring Planck's Constant).
  • pm vs nm in Compton problems, or forgetting cos θ in degrees → Lesson 6 (Photon Momentum and the Compton Effect).
  • Explaining single-photon interference, pair production thresholds → Lesson 7 (Wave-Particle Duality of Light).
  • Using E = hc/λ for electrons, or missing the square root in 1.226/√V → Lesson 8 (Matter Waves).
  • Grating-equation setup for electrons, ring-size predictions → Lesson 9 (Electron Diffraction).
  • Sign errors with negative energy levels, choosing absorbed photon energies → Lesson 10 (The Bohr Model and Atomic Spectra).
  • Forgetting the 4π, or thinking uncertainty is just instrument error → Lesson 11 (Uncertainty and Probability).
  • Band-gap cut-offs, efficiency, laser ideas → Lesson 12 (Quantum Technologies I).
  • Resolution and wavelength, qubit counts, encryption issues → Lesson 13 (Quantum Technologies II).
  • Quark charges, conservation of baryon and lepton number → Lesson 14 (The Standard Model).

Looking ahead: the sibling unit Special Relativity completes strand F with Einstein's other revolution. In first-year university physics and chemistry, these quantum ideas return with more mathematics (the Schrödinger equation) and lead into chemistry, materials science, electronics and medical physics.