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Lesson 5 of 7Revolutions in Modern Physics
Unit 5 · Lesson 5 of 7

Matter Waves and Wave-Particle Duality

Photons carry momentum, electrons diffract like waves, and atoms emit light only at particular wavelengths. Together these show that light and matter both have a wave side and a particle side.

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Key things to remember

  1. 1Photon momentum: . In the Compton effect, scattered X-rays have a longer wavelength because they gave momentum to electrons.
  2. 2de Broglie wavelength of a particle: .
  3. 3Electron diffraction by crystals (Davisson and Germer, G. P. Thomson) is the evidence that matter has wave properties.
  4. 4An atomic transition emits or absorbs one photon with ; hydrogen's levels are .
  5. 5Emission spectra are bright lines; absorption spectra are dark lines at the same wavelengths for the same element.

The photoelectric effect showed that light, long accepted as a wave, also behaves like a stream of particles. That raised an obvious and daring question: if waves can act like particles, can particles act like waves? The answer turned out to be yes, and it changed how physicists describe electrons, atoms and everything built from them. This lesson follows the evidence in both directions.

Photons carry momentum

A photon has no mass, yet it has momentum. Shorter wavelength means more momentum.

If a photon is a particle, it should be able to collide with things and transfer momentum. In 1923 Arthur Compton fired X-rays at a solid target and measured the X-rays that scattered off its electrons. The scattered X-rays had a longer wavelength than the incoming ones, and the shift grew with the scattering angle. A wave scattering off a charge should come out with its wavelength unchanged. A photon behaving like a billiard ball, though, gives some of its energy and momentum to the electron it hits, so it leaves with less energy and therefore a longer wavelength. This Compton effect was strong evidence that photons carry momentum exactly as predicts.

Going further: the size of the Compton shift
Treating the collision with conservation of energy and momentum gives , where is the angle the photon is scattered through. The constant is tiny, which is why the effect only shows up clearly for X-rays and gamma rays, whose wavelengths are already very short.

Matter waves

In 1924 Louis de Broglie proposed that the relationship works both ways: any moving particle with momentum has an associated wavelength. For everyday objects this wavelength is absurdly small, because is so small and their masses are so large. For an electron, with its tiny mass, it comes out comparable to the spacing between atoms in a crystal — which suggests exactly how to test the idea.

The de Broglie wavelength. Use mass in kilograms and speed in metres per second to get metres.

Diffraction is only noticeable when a wave meets an opening or obstacle comparable in size to its wavelength. The regularly spaced atoms of a crystal act like a diffraction grating for waves with wavelengths around a tenth of a nanometre. In 1927 Clinton Davisson and Lester Germer directed a beam of electrons at a nickel crystal and found strong reflections only at particular angles — a diffraction pattern — and G. P. Thomson saw diffraction rings when electrons passed through thin metal foils. The measured wavelengths matched . Electron diffraction is the key evidence for the wave nature of matter, and electron microscopes exploit it: electron wavelengths are far shorter than those of visible light, so they can resolve far finer detail.

Energy levels and line spectra

Hydrogen Energy LevelsEnergyn = ∞0 eVn = 1−13.60 eVn = 2−3.40 eVn = 3−1.51 eVn = 4−0.85 eVn = 5−0.54 eVn = 6−0.38 eV656 nm486 nm434 nm410 nmto n = 1: ultraviolet (Lyman series)energy axis broken between n = 1 and n = 2Hydrogen visible line spectrum400500600700656486434410wavelength (nm)Balmer series: drops to n = 2each line = one photon energy, E = hc/λbigger drop → more energy → shorter λ
Fig 1Hydrogen energy levels. Each downward jump emits one photon whose energy equals the gap, producing one bright line in the spectrum.

A hot, low-pressure gas does not glow with a continuous rainbow. It emits only a few sharp wavelengths, a line spectrum unique to each element. Niels Bohr's 1913 model explained hydrogen's lines by allowing its electron only certain energy levels. An electron that drops from a higher level to a lower one emits a single photon carrying exactly the energy difference; an electron can jump up only by absorbing a photon with exactly the right energy. Matter waves later gave a reason for the allowed levels: an electron's wave must fit around the atom as a standing wave, a whole number of wavelengths, much like the harmonics on a guitar string.

Energies are negative because the electron is bound; zero energy means the electron has just escaped the atom.
AEmission spectrum
  • Bright lines on a dark background
  • Produced by a hot, low-pressure gas
  • Electrons drop to lower levels and emit photons
  • Each line's energy equals one level gap
BAbsorption spectrum
  • Dark lines in an otherwise continuous spectrum
  • Produced when white light passes through a cooler gas
  • Electrons absorb photons and jump to higher levels
  • Dark lines sit at the same wavelengths as that element's bright emission lines
Wave-particle duality
Light and matter both show wave behaviour (interference and diffraction) when they travel, and particle behaviour (arriving in discrete, localized amounts of energy and momentum) when they interact. No single experiment shows both aspects fully at once, and neither the wave model nor the particle model alone is complete. Quantum mechanics is the theory that combines them.

Worked examples

Reveal one step at a time and try to beat it to the next line.

Example 1
An electron () moves at . Find its de Broglie wavelength and explain why a crystal can diffract it.
Example 2
A baseball is thrown at . Find its de Broglie wavelength and explain why it never diffracts noticeably.
Example 3
An electron starts from rest and is accelerated through a potential difference of . Find its speed and its de Broglie wavelength.
Example 4
A hydrogen electron drops from the level to the level. Find the energy and wavelength of the emitted photon.

Where marks get lost

  • Calculating a photon's momentum with . A photon has no mass, so that formula does not apply; its momentum is .
  • Forgetting to convert grams to kilograms in , which makes the wavelength 1000 times too large.
  • Thinking the Compton effect makes X-rays shorter in wavelength. The photon loses energy to the electron, so its wavelength gets longer.
  • Subtracting energy levels in the wrong order and getting a negative photon energy. The photon energy is the size of the gap: higher level minus lower level.
  • Believing large objects have no wavelength. They do; it is simply far too small to detect.

Flashcards 8

Photon momentum
Compton effect
de Broglie wavelength
Electron diffraction
+ 4 more

Practice

1
What is the momentum of an X-ray photon with a wavelength of , in kg·m/s? (You may type an answer like 3.2e-25.)
kg·m/s
2
What is the de Broglie wavelength of an electron moving at , in nanometres?
nm
3
What is the de Broglie wavelength of a proton moving at , in metres? (You may type an answer like 2.5e-12.)
m
4
Which observation provides direct evidence that electrons have wave properties?
5
In the Compton effect, how does a scattered X-ray photon compare with the incoming photon?
6
Why does a thrown baseball never show diffraction as it passes through a doorway?
7
A hydrogen electron drops from to . What is the energy of the emitted photon, in electron-volts? Use .
eV
8
When an electron in an atom moves from a higher energy level to a lower one, does the atom emit or absorb a photon?
9
White light passes through cool hydrogen gas and then through a spectroscope. What is observed?
10
All four objects move at the same speed. Order them from the longest de Broglie wavelength to the shortest.
  1. 1A proton
  2. 2A baseball
  3. 3A grain of dust
  4. 4An electron
11
Match each experiment or observation to what it demonstrates.
Photoelectric effect
Compton effect
Electron diffraction
Line spectra of gases

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