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What is a photon, and how does the photoelectric effect show that light is quantised?

Photons: the photon as a quantum of electromagnetic energy E = hf, the photoelectric effect and Einstein's equation, the work function and threshold frequency, and the electronvolt.

A focused answer to the Eduqas A-Level Physics Component 3 photons content, covering the photon as a quantum of electromagnetic energy E = hf, the photoelectric effect and Einstein's photoelectric equation, the work function and threshold frequency, and the electronvolt as an energy unit.

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  1. What this dot point is asking
  2. The answer
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What this dot point is asking

Eduqas wants you to describe a photon as a quantum of electromagnetic energy with E=hfE = hf, explain the photoelectric effect, apply Einstein's photoelectric equation, define the work function and threshold frequency, and use the electronvolt as a unit of energy.

The answer

The photon

The photoelectric effect

Einstein's photoelectric equation

Work function, threshold frequency and the electronvolt

Examples in context

The photoelectric effect, for which Einstein won the Nobel Prize, established the quantum nature of light and underpins photomultiplier tubes, solar cells, light meters and the image sensors in digital cameras. Photon energy ideas explain why ultraviolet light causes sunburn and damages DNA while visible light does not, and they set the operating wavelengths of lasers, LEDs and fibre-optic communication.

Try this

Q1. State the equation for the energy of a photon. [1 mark]

  • Cue. E=hfE = hf (equivalently E=hcλE = \frac{hc}{\lambda}).

Q2. A photon has frequency 5.0×1014 Hz5.0 \times 10^{14}\ \text{Hz}. Find its energy (h=6.63×1034 J sh = 6.63 \times 10^{-34}\ \text{J s}). [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 no electrons are emitted below the threshold frequency, however intense the light. [2 marks]

  • Cue. Each photon has energy hf<ϕhf < \phi, so no single photon can free an electron; more such photons (greater intensity) still cannot.

Exam-style practice questions

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

Eduqas 20195 marksA metal surface has a work function of 2.3 eV2.3\ \text{eV}. Light of wavelength 400 nm400\ \text{nm} is shone on 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 1 eV=1.6×1019 J1\ \text{eV} = 1.6 \times 10^{-19}\ \text{J}.
Show worked answer →

Photon energy: E=hcλ=(6.63×1034)(3.0×108)400×109=1.989×10254.0×107=4.97×1019 JE = \dfrac{hc}{\lambda} = \dfrac{(6.63 \times 10^{-34})(3.0 \times 10^{8})}{400 \times 10^{-9}} = \dfrac{1.989 \times 10^{-25}}{4.0 \times 10^{-7}} = 4.97 \times 10^{-19}\ \text{J}.

Work function in joules: ϕ=2.3×1.6×1019=3.68×1019 J\phi = 2.3 \times 1.6 \times 10^{-19} = 3.68 \times 10^{-19}\ \text{J}.

Einstein's equation hf=ϕ+KEmaxhf = \phi + KE_\text{max}: KEmax=Eϕ=4.97×10193.68×1019=1.3×1019 JKE_\text{max} = E - \phi = 4.97 \times 10^{-19} - 3.68 \times 10^{-19} = 1.3 \times 10^{-19}\ \text{J}.

Markers reward the photon energy from hcλ\frac{hc}{\lambda}, converting the work function to joules, and KEmax1.3×1019 JKE_\text{max} \approx 1.3 \times 10^{-19}\ \text{J}.

Eduqas 20224 marksExplain why, in the photoelectric effect, no electrons are emitted below a threshold frequency no matter how intense the light, and why this supports the photon model rather than the wave model of light.
Show worked answer →

Each photon carries a single quantum of energy E=hfE = hf, and one photon is absorbed by one electron. An electron can only escape if its photon supplies at least the work function ϕ\phi, so emission needs hfϕhf \geq \phi, i.e. a frequency at or above the threshold f0=ϕhf_0 = \frac{\phi}{h}.

Below the threshold each photon has too little energy to free an electron, and increasing the intensity simply sends more such photons, none of which individually has enough energy: still no emission. The wave model wrongly predicts that enough intensity, given time, would always free electrons. The existence of a threshold frequency therefore supports the photon (quantum) model. Markers reward the one-photon-one-electron idea, the hfϕhf \geq \phi condition, and explaining why intensity cannot compensate below the threshold.

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