Quantum & Nuclear: every key term you need (+ practice quiz)
26 flashcard terms for AP Physics 2 Unit 7, written to match the course framework. Read them here, drill them as flashcards, or take the 25-question quiz. Free, no account needed.
K_max vs frequency is a straight line: slope = h (same for every metal), x-intercept = threshold frequency f₀, y-intercept = −φ (work function). Intensity changes the current, never the slope or intercept.
Stopping Potential
eV_stop = K_max = hf − φ. Doubling light intensity leaves V_stop unchanged; raising frequency raises it linearly. Instantaneous emission even at low intensity contradicts the wave model.
Photon Momentum
p = h/λ = E/c. Photons carry momentum despite zero mass; light pressure and Compton scattering (wavelength lengthens after scattering off an electron) confirm it.
Compton Scattering
An X-ray photon striking an electron loses energy and emerges at longer wavelength; the shift grows with scattering angle. Cannot be explained by waves — energy and momentum are conserved photon-by-photon.
de Broglie Applications
λ = h/p = h/√(2mK). A 100 eV electron has λ ≈ 0.12 nm — comparable to atomic spacing, so electrons diffract from crystals (Davisson–Germer). Baseballs have λ ~ 10^-34 m, unobservable.
Energy Level Transitions
Photon emitted or absorbed with E = |E_i − E_f| = hc/λ. Only exact energy matches are absorbed; a photon with more energy than the ionization energy can eject the electron with leftover kinetic energy.
Hydrogen Energy Levels
E_n = −13.6 eV/n². Ionization from ground state needs 13.6 eV (91 nm). Balmer series (to n = 2) gives visible lines; Lyman (to n = 1) is ultraviolet; Paschen (to n = 3) is infrared.
An electron in level n can produce n(n − 1)/2 distinct downward transitions when many atoms are excited to n; from n = 4 that gives 6 lines.
Standing Waves in Bohr Orbits
Allowed orbits fit an integer number of de Broglie wavelengths: 2πr = nλ, equivalent to angular momentum quantization L = nh/2π. Explains why energy levels are discrete.
Mass–Energy Equivalence
E = mc²; 1 u ≈ 931.5 MeV/c². Binding energy = (mass of separate nucleons − nuclear mass) × c². Iron-56 region has the highest binding energy per nucleon, so fission of heavy and fusion of light nuclei both release energy.
Conservation Laws in Nuclear Reactions
Mass number A and charge Z are conserved (nucleon and charge conservation), as are total energy and momentum. Mass alone is not conserved — the mass defect appears as kinetic energy or photons.
Decay Modes
Alpha: A − 4, Z − 2. Beta-minus: n → p + e⁻ + antineutrino, Z + 1. Beta-plus: p → n + e⁺ + neutrino, Z − 1. Gamma: nucleus de-excites, A and Z unchanged.
Half-Life Reasoning
N = N₀(½)^(t/T). After 3 half-lives 1/8 remains; the activity (decays per second) also drops to 1/8. Half-life is unaffected by temperature, pressure, or chemical state.
Wave Function and Probability
|ψ|² gives the probability per unit length of finding a particle; regions where the wave function is large are where the particle is likely detected. Nodes are positions of zero probability.
Heisenberg Uncertainty Consequences
Δx·Δp ≥ h/4π. Confining an electron to an atom (Δx ~ 10^-10 m) forces a momentum spread that keeps it from sitting on the nucleus — the reason atoms have size.