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De Broglie wavelength of electrons, protons and neutrons

Calculate the matter wavelength of a particle from its kinetic energy, with its momentum and speed, using the relativistic formula.

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De Broglie wavelength

0.1226 nm

Comparable to the spacing between atoms: diffraction by crystals

Speed

5,930,099 m/s

Same wavelength in picometers
122.6 pm
Momentum
5.403 × 10⁻²⁴ kg·m/s
Speed as a share of the speed of light
1.978%
Non-relativistic

Matter behaves like a wave

In 1924 Louis de Broglie suggested that the wave–particle duality of light also applies to matter. Every moving particle has a wavelength:

λ = h ÷ p

where h = 6.626 × 10⁻³⁴ J·s is Planck’s constant and p is the particle’s momentum. Three years later, Davisson and Germer confirmed it by bouncing electrons off a nickel crystal and seeing a diffraction pattern, exactly as X-rays would produce.

How the calculator works

You choose a particle (electron, proton, neutron or alpha particle) and its kinetic energy in electronvolts. The calculator converts the energy to joules and finds the momentum with the relativistic formula:

pc = √(E² + 2E × mc²)

then divides Planck’s constant by p. It also gives the particle’s speed, v = pc² ÷ (E + mc²), and that speed as a share of the speed of light. Using the relativistic formula means the answer stays correct for fast electrons, where the classical p = √(2mE) starts to drift.

Worked example

An electron with 100 eV of kinetic energy:

Result Value
Momentum 5.403 × 10⁻²⁴ kg·m/s
Wavelength 0.1226 nm (122.6 pm)
Speed about 5.93 million m/s
Share of c 1.98% (non-relativistic)

That wavelength is the same size as the spacing between atoms, which is why low-energy electron diffraction (LEED) is used to study crystal surfaces.

Some reference values

Particle and energy Wavelength
Electron, 1 eV 1.23 nm
Electron, 10 keV 0.0122 nm (12.2 pm)
Electron, 100 keV (electron microscope) 3.70 pm
Thermal neutron, 0.025 eV 0.181 nm
Proton, 1 MeV 28.6 fm

At 100 keV the electron already travels at 55% of the speed of light. The classical formula would give 3.88 pm, about 5% too long, which matters for electron microscope resolution.

Why it matters

The short wavelength of fast electrons is what lets electron microscopes see detail far smaller than light microscopes can, since resolution is limited to roughly half the wavelength. Thermal neutrons, with wavelengths near 0.18 nm, are used to map the positions of atoms in materials, and the same principle underlies quantum effects in electronics and chemistry.

For everyday objects the wavelength is absurdly small. A 145 g baseball at 40 m/s has λ ≈ 1.1 × 10⁻³⁴ m, so its wave nature can never be observed.

Frequently asked questions

What is the de Broglie wavelength?

Louis de Broglie proposed in 1924 that every moving particle behaves like a wave, with a wavelength λ = h ÷ p, where h is Planck's constant and p the particle's momentum. The faster or heavier the particle, the shorter the wavelength.

Why does an electron at 100 eV have a wavelength of about 0.12 nm?

Its momentum is about 5.4 × 10⁻²⁴ kg·m/s, and Planck's constant divided by that gives 0.1226 nm. That is close to the spacing between atoms in a crystal, which is why low-energy electrons diffract off crystal surfaces.

Does the calculator account for relativity?

Yes. It uses the relativistic momentum pc = √(E² + 2E·mc²), so results stay correct for fast electrons. Below about 10 keV for electrons the classical formula gives nearly the same answer; at 100 keV it is about 5% too long.

Why do baseballs not show wave behavior?

A 145 g ball at 40 m/s has a de Broglie wavelength around 10⁻³⁴ m, far smaller than any atom or slit. Wave effects only become visible when the wavelength is comparable to the size of the obstacle.

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Results are estimates provided for information purposes. They do not replace professional advice.