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photon energy and momentum

Learning objectives

  • Outcome

    Calculate photon energy from frequency or wavelength using E=hν=hc/λE=h\nu=hc/\lambda and express the result in joules and electron-volts.

  • Outcome

    Determine photon momentum from p=h/λp=h/\lambda and p=E/cp=E/c, stating its direction along the propagation of light.

  • Outcome

    Explain why a photon has zero rest mass but nonzero momentum using the relation E2=(pc)2+(m0c2)2E^2=(pc)^2+(m_0c^2)^2.

  • Outcome

    Compare photon energy and momentum in different spectral ranges (radio, visible, X-ray, gamma) and estimate their orders of magnitude.

Understand the idea

Photon energy and momentum

Text

Interference, diffraction and polarization show that light has wave properties, yet energy exchange with matter occurs in discrete portions.

Einstein proposed that light propagates and is absorbed in quanta with energy E=hν=hc/λE = h\nu = hc/\lambda, where hh is Planck's constant, ν\nu is frequency and λ\lambda is wavelength.

Special relativity gives the energy–momentum relation E2=(pc)2+(m0c2)2E^2 = (pc)^2 + (m_0 c^2)^2.

For a photon m0=0m_0 = 0 (a photon cannot be at rest), so E=pcE = pc, hence the momentum is p=E/c=h/λp = E/c = h/\lambda.

The momentum direction coincides with the direction of light propagation, which appears in radiation pressure and in the Compton effect.

Thus the photon is a massless particle with nonzero momentum, and its energy and momentum are related through the speed of light cc.

Worked examples

Direct

Problem

Find the energy (in joules and electron-volts) and momentum of a photon with wavelength λ=500\lambda = 500 nm.

Solution

Conveniently use hc=1240hc = 1240 eV·nm, then

E=hcλ=1240 eV⋅nm500 nm=2.48 eV.E=\frac{hc}{\lambda}=\frac{1240\ \text{eV·nm}}{500\ \text{nm}}=2.48\ \text{eV}.

In joules: E=2.48⋅1.602⋅10−19 J≈3.97⋅10−19 JE = 2.48 \cdot 1.602\cdot10^{-19}\ \text{J} \approx 3.97\cdot10^{-19}\ \text{J}.

Momentum: p=hλ=6.626⋅10−345.00⋅10−7≈1.33⋅10−27 kg⋅m/s.p=\frac{h}{\lambda}=\frac{6.626\cdot10^{-34}}{5.00\cdot10^{-7}}\approx 1.33\cdot10^{-27}\ \text{kg·m/s}.

Check with p=E/cp=E/c: (3.97⋅10−19)/(3.00⋅108)≈1.32⋅10−27 kg⋅m/s(3.97\cdot10^{-19})/(3.00\cdot10^8)\approx 1.32\cdot10^{-27}\ \text{kg·m/s}.

The momentum direction is along the light beam.

Application

Problem

A laser pointer with power P=1.0P=1.0 mW emits light of wavelength λ=650\lambda=650 nm. (a) How many photons are emitted per second? (b) What force does the light exert on a black absorbing target if the beam strikes it completely?

Solution

Energy of one photon: E=hcλ=1240 eV⋅nm650 nm≈1.91 eV=3.06⋅10−19 J.E=\frac{hc}{\lambda}=\frac{1240\ \text{eV·nm}}{650\ \text{nm}}\approx 1.91\ \text{eV}=3.06\cdot10^{-19}\ \text{J}.

Number of photons per second: N=PE=1.0⋅10−33.06⋅10−19≈3.3⋅1015 s−1.N=\frac{P}{E}=\frac{1.0\cdot10^{-3}}{3.06\cdot10^{-19}}\approx 3.3\cdot10^{15}\ \text{s}^{-1}.

Momentum of one photon is p=h/λ=E/cp=h/\lambda=E/c. Under complete absorption the target receives per second the total momentum Np=P/cNp=P/c, so the force is F=Pc=1.0⋅10−33.00⋅108≈3.3⋅10−12 N.F=\frac{P}{c}=\frac{1.0\cdot10^{-3}}{3.00\cdot10^8}\approx 3.3\cdot10^{-12}\ \text{N}.

For mirror reflection the force would be twice as large.

Transfer

Problem

An electron and a positron are at rest and annihilate, producing two identical photons that fly apart in opposite directions. The electron rest energy is mec2=0.511m_ec^2=0.511 MeV. Find the energy, momentum and wavelength of each photon.

Solution

The initial total momentum is zero, so the photon momenta are equal in magnitude and opposite in direction. From energy conservation 2Eγ=2mec22E_\gamma=2m_ec^2, hence Eγ=mec2=0.511 MeV.E_\gamma=m_ec^2=0.511\ \text{MeV}.

For a photon E=pcE=pc, so pγ=Eγc=0.511 MeV/c≈0.511⋅106⋅1.602⋅10−193.00⋅108≈2.73⋅10−22 kg⋅m/s.p_\gamma=\frac{E_\gamma}{c}=0.511\ \text{MeV}/c \approx \frac{0.511\cdot10^6\cdot1.602\cdot10^{-19}}{3.00\cdot10^8}\approx 2.73\cdot10^{-22}\ \text{kg·m/s}.

Wavelength: λ=hcEγ=1240 eV⋅nm5.11⋅105 eV≈2.43⋅10−3 nm=2.43 pm.\lambda=\frac{hc}{E_\gamma}=\frac{1240\ \text{eV·nm}}{5.11\cdot10^5\ \text{eV}}\approx 2.43\cdot10^{-3}\ \text{nm}=2.43\ \text{pm}.

This is hard gamma radiation.

Practice

Text

Self-study plan with a simulation (safe, no real radiation sources).

  1. Open the PhET simulation 'Photoelectric Effect'.
  2. Choose a metal (for example, sodium) and for wavelengths 400, 450, 500, 550 and 600 nm record the stopping voltage VsV_s.
  3. For each wavelength calculate the frequency ν=c/λ\nu=c/\lambda, the photon energy E=hνE=h\nu and the momentum p=h/λ=E/cp=h/\lambda=E/c; fill in a table.
  4. Plot eVseV_s versus ν\nu. The slope should be close to Planck's constant hh, and the intercept with the ν\nu axis should be close to the red threshold of the photoelectric effect.
  5. Double the intensity and verify that VsV_s and the photon energy do not change while the photocurrent increases. Explain this using the number of photons per second N=P/EN=P/E.
  6. Write a 3–4 sentence conclusion linking photon energy and momentum.

Visual reference

Purpose

Show that photon energy and momentum increase with frequency (and decrease with wavelength) and are related by E=pcE=pc, and provide benchmarks along the electromagnetic spectrum.

Representation

A two-panel diagram.

(a) A graph of EE versus ν\nu: a straight line with slope hh; points for radio waves, visible light, X-rays and gamma rays are marked on it.

(b) A sketch of a photon beam: for each photon the momentum vector p⃗\vec p points along the beam, and the vector length is proportional to 1/λ1/\lambda; next to it the relation E=pc=hνE=pc=h\nu is written.

Real-world examples

Green pixel of a phone screen

Scenario

A smartphone screen shows a green area of wavelength λ=550 nm\lambda = 550\ \text{nm} and gives off about P=0.10 WP = 0.10\ \text{W} of green light. Each photon carries E=hc/λ=6.63×10−34×3.00×1085.50×10−7=3.61×10−19 J=2.25 eV,E = hc/\lambda = \frac{6.63\times10^{-34} \times 3.00\times10^{8}}{5.50\times10^{-7}} = 3.61\times10^{-19}\ \text{J} = 2.25\ \text{eV}, so the screen emits N=P/E≈2.8×1017N = P/E \approx 2.8\times10^{17} photons every second.

Connection

This is the photon picture: E=hf=hc/λE = hf = hc/\lambda with h=6.63×10−34 J⋅sh = 6.63\times10^{-34}\ \text{J·s}, and each photon also carries momentum p=E/c=h/λ=1.20×10−27 kg⋅m/sp = E/c = h/\lambda = 1.20\times10^{-27}\ \text{kg·m/s}. Multiplying by the number of photons per second gives the total momentum carried away each second, 3.3×10−10 kg⋅m/s3.3\times10^{-10}\ \text{kg·m/s}, i.e. a light-pressure force of order 3×10−10 N3\times10^{-10}\ \text{N} — which is why a 0.20 kg0.20\ \text{kg} phone does not visibly recoil.

A kitchen microwave oven

Scenario

A microwave oven's magnetron runs at f=2.45 GHzf = 2.45\ \text{GHz}, so λ=c/f=12.2 cm\lambda = c/f = 12.2\ \text{cm}. One photon has E=hf=6.63×10−34×2.45×109=1.62×10−24 J=1.01×10−5 eV.E = hf = 6.63\times10^{-34} \times 2.45\times10^{9} = 1.62\times10^{-24}\ \text{J} = 1.01\times10^{-5}\ \text{eV}. An 800 W800\ \text{W} oven therefore delivers N=P/E≈4.9×1026N = P/E \approx 4.9\times10^{26} photons every second, and each of them carries p=E/c=5.4×10−33 kg⋅m/sp = E/c = 5.4\times10^{-33}\ \text{kg·m/s}.

Connection

The concept supplies both relations: E=hfE = hf turns a measured frequency into the energy of a single quantum, and p=E/cp = E/c shows that even a massless quantum has momentum. The value 1.01×10−5 eV1.01\times10^{-5}\ \text{eV} explains why such photons make water molecules rotate and heat food, yet cannot ionise atoms, whose ionisation energies are of order 11–10 eV10\ \text{eV}.

A laser rangefinder in golf

Scenario

A golf laser rangefinder fires a 905 nm905\ \text{nm} infrared pulse of energy 3.0×10−7 J3.0\times10^{-7}\ \text{J} lasting 10 ns10\ \text{ns} at a flag 150 m150\ \text{m} away and times the echo. One photon of that pulse has E=hc/λ=2.20×10−19 J=1.37 eVE = hc/\lambda = 2.20\times10^{-19}\ \text{J} = 1.37\ \text{eV}, so the pulse contains 3.0×10−7/2.20×10−19≈1.4×10123.0\times10^{-7}/2.20\times10^{-19} \approx 1.4\times10^{12} photons.

Connection

Each photon carries momentum p=h/λ=7.3×10−28 kg⋅m/sp = h/\lambda = 7.3\times10^{-28}\ \text{kg·m/s}; a pulse reflected straight back changes the momentum of every photon by 2p2p, so over the 10 ns10\ \text{ns} pulse the light pushes the flag with about 2.0×10−7 N2.0\times10^{-7}\ \text{N}. The same E=hc/λE = hc/\lambda fixes the photon energy the detector must register, which is why near-infrared light is chosen for the low-noise sensor.