Salam Academy
Paper 4 · Module

Quantum physics

3 subtopics≈ 110 min in total
  1. Photons and the photoelectric effect

    Light comes in quanta called photons, each of energy E=hf=hcλE=hf=\dfrac{hc}\lambda (h=6.63×10−34h=6.63\times10^{-34} J s) and momentum p=Ecp=\dfrac Ec. When photons hit a metal, each can release one electron if its energy exceeds the work function Φ\Phi: hf=Φ+12mvmax⁡2hf=\Phi+\tfrac12mv_{\max}^2. Below the threshold frequency f0=Φhf_0=\dfrac\Phi h, no electrons are emitted, however bright the light. Brighter light means more photons, so more electrons, but not faster ones.

    ≈ 40 min
  2. Wave–particle duality

    Light behaves as a wave (diffraction, interference) and as particles (the photoelectric effect). Matter does too: de Broglie proposed that any moving particle has a wavelength λ=hp=hmv\lambda=\dfrac hp=\dfrac h{mv}. Electron diffraction through thin graphite proves it: electrons form rings like waves passing through a grating. Faster electrons have shorter wavelengths, so the rings get smaller.

    ≈ 35 min
  3. Energy levels and line spectra

    Electrons in an isolated atom can only have certain discrete energies, called energy levels (negative values, with zero meaning the electron is free). When an electron drops from level E1E_1 to a lower level E2E_2, it emits a photon with hf=E1−E2hf=E_1-E_2. Because only certain differences exist, only certain wavelengths appear: a line spectrum. An absorption spectrum shows dark lines where the atoms absorb exactly those photon energies from a continuous spectrum.

    ≈ 35 min