Understand that photoelectrons may be emitted from a metal surface when it is illuminated by electromagnetic radiation, and use the photon description of light to explain the observed phenomena.
A photon is a quantum of electromagnetic radiation. Its energy is directly proportional to its frequency (or inversely proportional to its wavelength):
\[
E = h\nu = \frac{hc}{\lambda}
\]
Because photons are mass‑less, their momentum follows from the relativistic relation \(E = pc\):
\[
p = \frac{E}{c} = \frac{h}{\lambda}
\]
Example: a photon of wavelength 500 nm carries
\[
p = \frac{6.626\times10^{-34}}{5.00\times10^{-7}}
= 1.33\times10^{-27}\ \text{kg·m·s}^{-1}.
\]
This tiny momentum underlies radiation‑pressure phenomena. For instance, sunlight exerts a pressure of about \(9.1\times10^{-6}\ \text{N·m}^{-2}\) on a perfectly absorbing surface, a principle exploited in solar‑sail spacecraft.
The photon model provides a particle description of light, while diffraction and interference require a wave description. The photoelectric effect is classic evidence for the particle nature because:
At the same time, the same light produces interference patterns in double‑slit experiments, demonstrating its wave character. Together these observations illustrate wave‑particle duality, as required by the syllabus.
Einstein treated each incident photon as delivering its whole energy to a single electron:
\[
h\nu = \phi + K_{\max}
\]
The work function is related to the threshold frequency by
\[
\phi = h\nu_0.
\]
| Quantity | Expression | Comment |
|---|---|---|
| Threshold frequency \(\nu_0\) | \(\displaystyle \nu_0 = \frac{\phi}{h}\) | Minimum frequency required for emission. |
| Threshold wavelength \(\lambda_0\) | \(\displaystyle \lambda_0 = \frac{hc}{\phi}\) | Photons with \(\lambda > \lambda_0\) cannot eject electrons. |
In the standard apparatus a reverse (retarding) voltage \(V_s\) is applied between the photocathode and anode. The most energetic electrons are just prevented from reaching the anode when
\[
eVs = K{\max} = h\nu - \phi,
\]
where \(e = 1.602\times10^{-19}\ \text{C}\) is the elementary charge. Measuring \(V_s\) therefore gives a direct value for the kinetic energy of the fastest electrons.
| Parameter | Requirement for Emission |
|---|---|
| Frequency \(\nu\) | \(\nu > \nu_0 = \dfrac{\phi}{h}\) |
| Photon energy \(E = h\nu\) | \(E > \phi\) (excess energy becomes kinetic energy) |
| Intensity | Controls the number of photons per second → controls the number of emitted electrons, not \(K_{\max}\). |
When a photon ejects an electron, conservation of momentum must be satisfied:
\[
\underbrace{\frac{h}{\lambda}}{\text{photon momentum}} = \underbrace{pe}{\text{electron}} + \underbrace{p{\text{recoil}}}_{\text{metal lattice}}.
\]
Because the metal’s mass is enormously larger than that of the electron, the recoil momentum of the lattice is negligible for A‑Level calculations, but the principle reinforces the particle picture of light.
Find \(K_{\max}\) for a sodium surface (\(\phi = 2.28\ \text{eV}\)) illuminated with light of wavelength \(400\ \text{nm}\).
\[
E = \frac{hc}{\lambda}
= \frac{6.626\times10^{-34}\times3.00\times10^{8}}{4.00\times10^{-7}}
= 4.97\times10^{-19}\ \text{J}.
\]
\[
K_{\max}=E-\phi = 4.97\times10^{-19} - 3.65\times10^{-19}
= 1.32\times10^{-19}\ \text{J}.
\]
Light of wavelength \(250\ \text{nm}\) shines on a metal with \(\phi = 3.0\ \text{eV}\). Determine the stopping potential required to just halt the most energetic electrons.
\[
E = \frac{hc}{\lambda}
= \frac{6.626\times10^{-34}\times3.00\times10^{8}}{2.50\times10^{-7}}
= 7.95\times10^{-19}\ \text{J}
= 4.96\ \text{eV}.
\]

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