recall and use E = hf

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

Recall and use the relation \$E = hf\$ to calculate the energy of a photon, and apply the associated momentum formula \$p = \dfrac{E}{c} = \dfrac{h}{\lambda}\$ in a variety of contexts.

Key Concepts

  • Photons are quanta of electromagnetic radiation and have no rest mass.
  • The energy of a photon is directly proportional to its frequency:

    \$E = hf\$

    where \$h = 6.626\times10^{-34}\ \text{J·s}\$ (Planck constant) and \$f\$ is the frequency.

  • Since \$c = \lambda f\$, the energy can also be expressed in terms of wavelength:

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

  • The momentum of a photon is related to its energy by:

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

  • Photon momentum, though small, can produce measurable effects (e.g., radiation pressure, photon recoil).

Useful Constants

ConstantSymbolValueUnits
Planck constant\$h\$6.626 × 10⁻³⁴J·s
Speed of light in vacuum\$c\$2.998 × 10⁸m·s⁻¹
Elementary charge\$e\$1.602 × 10⁻¹⁹C

Typical Photon Energies

Radiation TypeWavelength \$\lambda\$ (nm)Frequency \$f\$ (THz)Energy \$E\$ (eV)
Radio (AM)≈ 10⁶≈ 0.3≈ 1.2 × 10⁻⁶
Microwave (2.45 GHz)≈ 122 mm2.45≈ 1.0 × 10⁻⁵
Infrared (10 µm)10 00030≈ 0.124
Visible (green, 550 nm)550545≈ 2.25
Ultraviolet (200 nm)2001500≈ 6.20
X‑ray (0.1 nm)0.13 × 10⁶≈ 12.4 × 10³
Gamma (0.01 nm)0.013 × 10⁷≈ 124 × 10³

Derivation of Photon Momentum

Starting from the energy–frequency relation and the definition of wave speed:

\$E = hf,\qquad c = \lambda f\$

Eliminate \$f\$:

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

Since momentum \$p\$ for a massless particle satisfies \$E = pc\$, we obtain:

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

Example Problems

  1. Energy of a green photon

    A photon has a wavelength of \$550\ \text{nm}\$. Find its energy in joules and electron‑volts.

    Solution:

    \$E = \frac{hc}{\lambda} = \frac{(6.626\times10^{-34})(2.998\times10^{8})}{550\times10^{-9}} \approx 3.61\times10^{-19}\ \text{J}\$

    Convert to e \cdot using \$1\ \text{eV}=1.602\times10^{-19}\ \text{J}\$:

    \$E \approx \frac{3.61\times10^{-19}}{1.602\times10^{-19}} \approx 2.25\ \text{eV}\$

  2. Momentum of an X‑ray photon

    An X‑ray has a wavelength of \$0.1\ \text{nm}\$. Determine its momentum.

    Solution:

    \$p = \frac{h}{\lambda} = \frac{6.626\times10^{-34}}{0.1\times10^{-9}} = 6.63\times10^{-24}\ \text{kg·m·s}^{-1}\$

  3. Radiation pressure on a perfectly absorbing surface

    A laser beam of power \$5\ \text{W}\$ strikes a black surface perpendicularly. Find the force exerted by the photon momentum.

    Solution:

    For a completely absorbing surface, \$F = \dfrac{P}{c}\$ where \$P\$ is the power.

    \$F = \frac{5}{2.998\times10^{8}} \approx 1.67\times10^{-8}\ \text{N}\$

Common Misconceptions

  • Photons have zero rest mass but still carry momentum; momentum is not solely a function of mass.
  • The energy–frequency relation applies to all electromagnetic radiation, not just visible light.
  • When converting between wavelength and frequency, always keep track of units (nm ↔ m, THz ↔ Hz).

Suggested Classroom Activities

  1. Calculate the photon energy for the colours of the visible spectrum and plot \$E\$ versus \$\lambda\$.
  2. Demonstrate radiation pressure using a light‑mill or a solar‑sail model.
  3. Use a spectrometer to measure the wavelength of a laser and then compute its momentum.

Suggested diagram: A photon incident on a surface showing energy \$E = hf\$, momentum \$p = h/\lambda\$, and the resulting radiation pressure \$F = P/c\$.