Unit 7: Quantum, Atomic, and Nuclear Physics

AP Physics 2: 62 practice questions with detailed explanations.

Unit Study Guide

Executive Summary

At the smallest scales physics becomes quantum: photons, quantized atomic levels, and nuclear transformations.

Photons and the photoelectric effect

Light arrives in quanta of energy E=hf=hcλE = hf = \frac{hc}{\lambda}. The photoelectric effect: electrons eject only above a threshold frequency; intensity controls how many, not their energy — Einstein's Nobel-winning evidence for photons.

Atomic models

Bohr's model quantized orbits; electron transitions emit or absorb photons (E=EiEfE = E_i - E_f). Wave-particle duality (λ=h/p\lambda = h/p, de Broglie) applies to matter itself. The uncertainty principle limits simultaneous position-momentum precision.

Nuclear physics

Nuclei hold protons via the strong force; mass defect becomes binding energy (E=mc2E = mc^2). Radioactive decay: α (He nuclei), β (electrons), γ (photons), with half-lives governing decay rates. Fusion powers stars; fission powers reactors and the bomb.

Exam traps

Photon energy depends on frequency only — intensity changes the count, not each photon's energy. Higher frequency light does NOT always eject electrons faster (photoelectric threshold). Half-life is statistical — after two half-lives, a quarter remains. Mass and energy interconvert in nuclear reactions.

Top 5 Concepts to Master

  1. 1Compute photon energy from frequency.
  2. 2Explain the photoelectric effect’s threshold.
  3. 3Relate transitions to photon emission/absorption.
  4. 4Apply half-life decay.
  5. 5Compare fission, fusion, and binding energy.

Key Terms & Definitions

Practice with Flashcards
Photon energy

E = hf = hc/λ.

Photoelectric effect

Light ejecting electrons above a threshold frequency.

Work function

Minimum energy to eject an electron.

Bohr model

Quantized orbits with discrete transitions.

De Broglie wavelength

λ = h/p for matter waves.

Half-life

Time for half a radioactive sample to decay.

Binding energy

Energy holding a nucleus; E = Δmc².

Fission

Splitting heavy nuclei.

Fusion

Fusing light nuclei (stars).

Common Misconceptions: Exam Traps

Brighter light means more energetic photons.

Correct: Intensity changes photon number; frequency changes each photon’s energy.

After two half-lives nothing remains.

Correct: A quarter remains — decay is exponential, never quite zero.

Electrons orbit the nucleus like planets.

Correct: Quantum models describe probability clouds, not paths.

Mass is conserved in nuclear reactions.

Correct: Mass converts to energy: ΔE = Δmc².

Question Bank Breakdown

By difficulty

easy 28medium 25hard 9

By topic

Nuclear Reactions and Radioactivity 22Photoelectric Effect 10Atomic Models and Energy Levels 7Mass-Energy Equivalence 7Quantum Mechanics and Wave Functions 6

All Questions in this Unit