22.0Quantum Theory and the Atom
Overview: Quantum Theory and the Atom: Photons, Matter Waves and Atomic Models — American System Physics Revision Notes & Topical Questions
5 min read 7 parts Lesson 2 of 5 Unit quiz
Lesson summary
Describe the photoelectric effect.Below threshold frequency, no electrons are emitted regardless of intensity.1 eV = 1.60 × 10−19 J.Each element has a unique line spectrum.Hot objects emit a continuous spectrum that peaks at shorter λ when hotter.Electron microscopes use short de…
- Energy of a photon with f = 5.0 × 1014 Hz
- Planck's constant (h)
- Work function
- de Broglie wavelength
- Bohr model
- Emission spectrum
Section 1 of 7Overview: Quantum Theory and the Atom: Photons, Matter Waves and Atomic Models
1
2
Bohr's model works well only for hydrogen.
3
Lasers are monochromatic, coherent and directional.
4
Fluorescence emits visible light after UV absorption.
5
Quantum numbers describe electron states.
6
Einstein explained the photoelectric effect (Nobel Prize).
Section 2 of 7Process & sequence
1What the symbols mean:
Find photon energy: E = hf = hc/λ.
What the symbols mean: E = energy of one photon (J) · h = Planck constant (6.63 × 10−34 J s) · f = frequency (Hz)
2
Compare with work function.
3
If E > work function, KEmax = E − W.
4
Increasing intensity increases number of electrons, not their KE.
5
For atoms: photon energy = difference between levels.
Emission of a photonwrite these steps in this order; each step is a marking point.
- Atom absorbs energy
- Electron excited
- Drops to lower level
- Photon emitted
- E = hf = ΔE
Section 3 of 7Compare
| Phenomenon | Supports |
|---|---|
| Interference, diffraction | Wave nature |
| Photoelectric effect | Particle nature |
| Compton scattering | Photon momentum |
| Electron diffraction | Wave nature of matter |
| Model | Key idea |
|---|---|
| Thomson | Plum pudding |
| Rutherford | Small dense nucleus |
| Bohr | Quantised orbits |
| Quantum mechanical | Probability clouds (orbitals) |
Section 4 of 7Worked examples
Energy of a photon with f = 5.0 × 1014 Hz.
- E = 6.63 × 10−34 × 5.0 × 1014 = 3.3 × 10−19 J (≈ 2.1 eV).
Section 5 of 7Key terms
Section 6 of 7Command terms
Command terms
Identify / Describe (FRQ)
A short, specific statement; describing requires relevant characteristics, not a single word.
Explain / Justify (FRQ)
Give the cause-and-effect reasoning or evidence; a restated fact does not score.
Calculate
Show setup, substitution and the answer with units.
Predict
State the expected outcome; add a reason only if asked to justify.
MCQ technique
Read every option; eliminate distractors that are true statements but do not answer the question; watch for NOT/EXCEPT.
Section 7 of 7Exam technique
Keywords the mark scheme looks for in this lesson
Keywords the mark scheme looks for in this lesson
Photon · Planck's constant (h) · Photoelectric effect · Work function · de Broglie wavelength · Bohr model · Emission spectrum · Absorption spectrum · Laser · Heisenberg uncertainty principle
Learn each definition in the Key words tab exactly; a missing keyword in a definition usually loses the mark.
How to get full marks (examiner guidance)
1
Answer exactly what is asked; extra correct material does not earn credit, and contradictory statements can cancel credit (AP FRQ).
2
Use precise vocabulary (e.g. “active site”, “concentration gradient”, “allele”), never “it/stuff/things”.
3
Show units and working in calculations.
4
In MCQs, predict the answer before reading the options, then eliminate.
Instant feedbackCheck yourself
Q1. Increasing light intensity (above threshold) increases
1
A. electron KE
2
B. number of electrons
3
C. work function
4
D. frequency
Show answer
B. More photons.
Q2. Photon energy is proportional to
- A. wavelength
- B. frequency
- C. amplitude
- D. speed
Show answer
B. E = hf.
Q3. de Broglie wavelength decreases when momentum
- A. decreases
- B. increases
- C. stays
- D. is zero
Show answer
B. λ = h/p.
Q4. Line spectra show energy levels are
- A. continuous
- B. quantised
- C. infinite
- D. random
Show answer
B. Discrete lines.
Last updated:
