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How does the photoelectric effect show that light is quantised, and how can particles behave as waves?

Quantum physics: the photon model and the photon energy equation, the photoelectric effect and Einstein's photoelectric equation, work function and threshold frequency, and wave-particle duality with the de Broglie wavelength.

A focused answer to the OCR H556 quantum physics content, covering the photon model and the energy of a photon, the photoelectric effect and Einstein's photoelectric equation, work function and threshold frequency, the electronvolt, and wave-particle duality with the de Broglie equation and electron diffraction.

Generated by Claude Opus 4.812 min answer

Reviewed by: AI editorial process; not yet individually human-reviewed

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  1. What this dot point is asking
  2. The answer
  3. Examples in context
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What this dot point is asking

OCR wants you to describe the photon model of electromagnetic radiation, use the photon energy equation, explain the photoelectric effect and apply Einstein's photoelectric equation with the work function and threshold frequency, use the electronvolt, and explain wave-particle duality using the de Broglie equation and electron diffraction.

The answer

The photon model

The electronvolt is a convenient energy unit at this scale: one electronvolt is the energy gained by an electron moving through a potential difference of one volt, 1 eV=1.6×1019 J1\ \text{eV} = 1.6 \times 10^{-19}\ \text{J}.

The photoelectric effect

The wave model predicts that any frequency, given enough time, should accumulate enough energy to release electrons. The observed threshold and instantaneous emission show energy arrives in discrete photons, one absorbed by one electron.

Einstein's photoelectric equation

A graph of KEmaxKE_{\max} against frequency is a straight line of gradient hh with an xx-intercept at the threshold frequency f0f_0 and a yy-intercept of ϕ-\phi.

Wave-particle duality

Examples in context

Solar cells and photodiodes rely on the photoelectric (photovoltaic) effect, releasing charge carriers when photons above the band-gap energy are absorbed. Photomultiplier tubes and image sensors detect single photons. The electron microscope exploits the tiny de Broglie wavelength of fast electrons to resolve detail far smaller than any optical microscope can, because resolution improves as wavelength falls. Light-emitting diodes emit photons of a fixed energy set by the material, demonstrating E=hfE = hf in reverse.

Try this

Q1. State what is meant by the work function of a metal. [1 mark]

  • Cue. The minimum energy needed to free an electron from the surface of the metal.

Q2. Calculate the energy of a photon of frequency 5.0×1014 Hz5.0 \times 10^{14}\ \text{Hz}. [2 marks]

  • Cue. E=hf=(6.63×1034)(5.0×1014)=3.3×1019 JE = hf = (6.63 \times 10^{-34})(5.0 \times 10^{14}) = 3.3 \times 10^{-19}\ \text{J}.

Q3. Explain why the photoelectric effect supports the photon model rather than the wave model of light. [3 marks]

  • Cue. Emission is instantaneous, there is a threshold frequency, and the maximum kinetic energy depends on frequency not intensity; the wave model cannot explain any of these, but a one-photon-one-electron model can.

Exam-style practice questions

Practice questions written in the style of OCR exam questions on this dot point, with worked answer explainers. The year tag is the paper they imitate, not the source.

OCR 20194 marksA clean metal surface has a work function of 2.8 eV2.8\ \text{eV}. Light of wavelength 4.0×107 m4.0 \times 10^{-7}\ \text{m} is shone onto it. Calculate the maximum kinetic energy of the emitted photoelectrons in joules. Take h=6.63×1034 J sh = 6.63 \times 10^{-34}\ \text{J s}, c=3.0×108 m s1c = 3.0 \times 10^{8}\ \text{m s}^{-1} and e=1.6×1019 Ce = 1.6 \times 10^{-19}\ \text{C}.
Show worked answer →

Photon energy: E=hcλ=(6.63×1034)(3.0×108)4.0×107=4.97×1019 JE = \frac{hc}{\lambda} = \frac{(6.63 \times 10^{-34})(3.0 \times 10^{8})}{4.0 \times 10^{-7}} = 4.97 \times 10^{-19}\ \text{J}.

Convert the work function to joules: ϕ=2.8×1.6×1019=4.48×1019 J\phi = 2.8 \times 1.6 \times 10^{-19} = 4.48 \times 10^{-19}\ \text{J}.

Einstein's equation: KEmax=hfϕ=4.97×10194.48×1019=4.9×1020 JKE_{\max} = hf - \phi = 4.97 \times 10^{-19} - 4.48 \times 10^{-19} = 4.9 \times 10^{-20}\ \text{J}.

Markers reward the photon energy, converting the work function from electronvolts to joules, and the value about 4.9×1020 J4.9 \times 10^{-20}\ \text{J}.

OCR 20213 marksAn electron is accelerated from rest, gaining a speed of 2.96×107 m s12.96 \times 10^{7}\ \text{m s}^{-1}. Calculate the de Broglie wavelength of the electron. Take h=6.63×1034 J sh = 6.63 \times 10^{-34}\ \text{J s} and the electron mass m=9.11×1031 kgm = 9.11 \times 10^{-31}\ \text{kg}.
Show worked answer →

Use the de Broglie equation with the momentum: λ=hmv\lambda = \frac{h}{mv}.

Momentum: p=mv=(9.11×1031)(2.96×107)=2.70×1023 kg m s1p = mv = (9.11 \times 10^{-31})(2.96 \times 10^{7}) = 2.70 \times 10^{-23}\ \text{kg m s}^{-1}.

So λ=6.63×10342.70×1023=2.5×1011 m\lambda = \frac{6.63 \times 10^{-34}}{2.70 \times 10^{-23}} = 2.5 \times 10^{-11}\ \text{m}.

Markers reward calculating the momentum, applying λ=hp\lambda = \frac{h}{p}, and the value about 2.5×1011 m2.5 \times 10^{-11}\ \text{m} (comparable to atomic spacing, hence diffraction).

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