One equation read in two directions. Light was a wave and turned out to carry momentum; matter was a particle and turned out to have a wavelength, and λ = h/p says both.
Classical physics had two kinds of thing in it. A particle was a discrete object with a definite position and momentum, moving by Newton’s laws. An electromagnetic wave was an extended field, present everywhere at once, changing by Maxwell’s laws. The division was clean and it worked: particles made up the world, waves lit it.
It stopped working in 1900. Explaining the spectrum of thermal radiation forced Max Planck to assume that atoms emit and absorb energy only in discrete lumps , with
These two sections are about what that constant does. It turns out to be the exchange rate between wave language and particle language — and once you have an exchange rate, the two currencies are not really different.
1.1 Photons
A photon photon A particle-like quantum of electromagnetic radiation, carrying momentum p = h/λ and energy E = hc/λ. Light delivers its energy in these lumps, not continuously. defined in ch. 1 — open in glossary is a particle-like quantum of electromagnetic radiation. It travels at , and it carries momentum and energy
The Compton effect
The decisive evidence came in 1923. A. H. Compton fired X-rays at electrons and found the scattered X-rays came back with a longer wavelength — the Compton effect compton effect The increase in an X-ray's wavelength when it scatters off an electron, Δλ = (h/mₑc)(1−cos θ). It is exactly what you get by treating the collision as elastic between two particles. defined in ch. 1 — open in glossary — which no classical wave should do. A classical wave shakes an electron at frequency ; the electron re-radiates at frequency . The colour should not change.
It changes exactly as it would if a particle had bounced off another particle.
The result is the Compton shift:
The prefactor is a constant of nature in its own right, the Compton wavelength compton wavelength h/mₑc = 2.43 × 10⁻¹² m. Sets the size of the Compton shift, and the floor on how precisely a particle of mass m can be located. defined in ch. 1 — open in glossary of the electron:
But light also interferes
So light is granular. The difficulty is that the same light, sent through two slits, does what only a wave can do.
Fig. 1.2 — two slits separated by , a screen at distance . Constructive interference at when the path difference is an integer number of wavelengths, so the fringes are evenly spaced by .
Nothing about that is unusual for a wave; Young used it to measure the wavelength of light in 1801. What is unusual is what you see when the light is made very faint. The pattern does not fade — it granulates. Individual photons arrive at individual points, apparently at random, and the interference pattern assembles itself out of thousands of them.
1.2 De Broglie waves
In 1923, Louis de Broglie asked the obvious question in the other direction. If a wave carries momentum , might a thing with momentum carry a wavelength ?
This is the de Broglie wavelength de broglie wavelength λ = h/p — the wavelength a particle of matter behaves with. For a non-relativistic electron, λ = √(1.5/E) nm with E in eV. defined in ch. 1 — open in glossary , and it is proposed for matter — electrons, atoms, cricket balls.
To connect to something measurable, start from the relativistic energy–momentum relation
and eliminate in favour of :
That single formula covers everything, and it has two limits worth having by heart.
Ultra-relativistic (, or a massless photon): drop and the square root collapses to :
which is Eq. (1.1) again — as it must be. A photon is the case of the same formula.
Non-relativistic ( with ): the two brackets become and , and
For an electron, substituting and measuring in electronvolts gives a formula worth memorising:
so 1.5 eV gives exactly 1 nm, and 15 keV gives 0.01 nm.
It is not just electrons
What §§1.1–1.2 have established
Phillips ends §1.2 with the observation that ties the two sections together, and it is worth stating flatly:
If Planck’s constant were zero, all de Broglie wavelengths would be zero and particles of matter would only exhibit classical, particle-like properties.
Everything strange in this book is downstream of one small number being non-zero. And because the same appears in for light and in for matter, light and matter are not two kinds of thing behaving oddly in two different ways. They are one kind of thing — Phillips calls it a quantum particle quantum particle Phillips' term for an object with both particle-like and wave-like character, used to avoid implying it has a classical trajectory. defined in ch. 1 — open in glossary — and the classical particle and the classical wave are the two limits in which you can get away with forgetting that.
What the next chapters must now supply is the machinery: a wave equation whose solutions have exactly these properties. That is chapter 2.
Check yourself
0 / 6 answered
1.The Compton shift for a 90° scattering is 0.0024 nm. What is it for a 90° scattering of a photon with ten times the wavelength?
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2.In the two-slit simulation, turning on the which-path detector destroys the fringes. Which statement describes what changed mathematically?
The neutron is about 1839 times heavier. Use .
3.An electron and a neutron are given the same kinetic energy. Which has the longer de Broglie wavelength, and by roughly what factor?
4.Why did nobody detect the wave nature of a cricket ball?
5.The book prints the momentum of a 663 nm photon as . What is wrong, and how would you catch it?
6.What does tell a signal-processing engineer?