understand that electromagnetic radiation has a particulate nature

Published by Patrick Mutisya · 14 days ago

Cambridge A‑Level Physics 9702 – Energy and Momentum of a Photon

Energy and Momentum of a Photon

Learning Objective

Understand that electromagnetic radiation possesses a particulate (photon) nature and be able to calculate the energy and momentum associated with a photon.

Key Concepts

  • A photon is a quantum of electromagnetic radiation.
  • Energy of a photon is directly proportional to its frequency.
  • Even though photons are mass‑less, they carry momentum.
  • The particulate description explains phenomena such as the photoelectric effect, Compton scattering and radiation pressure.

Energy of a Photon

The energy \$E\$ of a photon is given by Planck’s relation:

\$E = h\nu = \frac{hc}{\lambda}\$

where

  • \$h = 6.626\times10^{-34}\ \text{J·s}\$ is Planck’s constant,
  • \$\nu\$ is the frequency of the radiation,
  • \$c = 3.00\times10^{8}\ \text{m·s}^{-1}\$ is the speed of light in vacuum,
  • \$\lambda\$ is the wavelength.

Momentum of a Photon

From the relativistic energy‑momentum relation \$E^{2}=p^{2}c^{2}+m{0}^{2}c^{4}\$ and noting that the rest mass \$m{0}=0\$ for a photon, we obtain:

\$p = \frac{E}{c} = \frac{h}{\lambda}\$

Thus the momentum \$p\$ is inversely proportional to the wavelength.

Derivation from Relativistic Principles (Optional)

Starting with \$E = \gamma m{0}c^{2}\$ and \$p = \gamma m{0}v\$, for \$m_{0}=0\$ the Lorentz factor \$\gamma\$ becomes infinite, but the ratio \$E/p\$ remains finite and equals \$c\$. This leads directly to \$p = E/c\$ for a mass‑less particle.

Experimental Evidence for the Particulate Nature

  1. Photoelectric Effect – Electrons are emitted from a metal only if the incident light has a frequency above a threshold, regardless of intensity. The kinetic energy of the emitted electrons follows \$K_{\max}=h\nu-\phi\$, where \$\phi\$ is the work function.
  2. Compton Scattering – X‑rays scattered from electrons show a wavelength shift \$\Delta\lambda = \frac{h}{m_{e}c}(1-\cos\theta)\$, consistent with photon momentum transfer.
  3. Radiation Pressure – Light exerts a measurable pressure \$P = \frac{I}{c}\$ (or \$2I/c\$ for perfect reflection) on surfaces, explained by momentum transfer from photons.

Suggested diagram: Schematic of the photoelectric effect showing incident photons, metal surface, and emitted electrons.

Sample Calculations

Table 1 illustrates the energy and momentum of photons at selected wavelengths.

Wavelength \$\lambda\$ (nm)Frequency \$\nu\$ (THz)Energy \$E\$ (eV)Momentum \$p\$ (kg·m s⁻¹)
4007503.105.27 × 10⁻²⁸
6005002.073.51 × 10⁻²⁸
8003751.552.62 × 10⁻²⁸
10003001.242.07 × 10⁻²⁸

Conversion factors used: \$1\ \text{eV}=1.602\times10^{-19}\ \text{J}\$, \$p = E/c\$.

Key Formulas to Remember

  • \$E = h\nu = \dfrac{hc}{\lambda}\$
  • \$p = \dfrac{E}{c} = \dfrac{h}{\lambda}\$
  • Photoelectric kinetic energy: \$K_{\max}=h\nu-\phi\$
  • Compton wavelength shift: \$\Delta\lambda = \dfrac{h}{m_{e}c}(1-\cos\theta)\$
  • Radiation pressure (absorption): \$P = \dfrac{I}{c}\$

Summary

Electromagnetic radiation can be described as a stream of photons, each carrying a quantised amount of energy \$E = h\nu\$ and a corresponding momentum \$p = h/\lambda\$. This particulate description successfully explains phenomena that wave theory alone cannot, confirming the dual nature of light.