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de Broglie Wavelength Calculator

Compute the de Broglie wavelength of a particle with momentum p = m·v. Quantum mechanics says every massive particle has a wavelength that controls its diffraction, scattering, and interference behavior.

Category: Physics

de Broglie Wavelength Calculator Inputs

Enter values to calculate

Particle mass in kg (electron ≈ 9.11×10⁻³¹ kg).

Speed of the particle (m/s). Subrelativistic speeds assumed.

Enable JavaScript for interactive calculation and step-by-step results.

de Broglie Wavelength Calculator Formula

Equation

\lambda = (h)/(p) = (h)/(m \, v)

Excel Formula

=(h)/(p)=(h)/(mv)

Variables

  • Mass m (kg) — Particle mass in kg (electron ≈ 9.11×10⁻³¹ kg).
  • Velocity v (m/s) — Speed of the particle (m/s). Subrelativistic speeds assumed.

How the de Broglie Wavelength Calculator Works

Louis de Broglie proposed in 1924 that every particle has a wavelength inversely proportional to its momentum. The idea is the core of quantum mechanics: not just electromagnetic waves but also protons, electrons, neutrons, and even large molecules can show interference. The shorter the wavelength, the harder the wave behavior is to detect.

The core relationship is \lambda = \frac{h}{p} = \frac{h}{m \, v}. Typical inputs include Mass m, Velocity v.

Enter your values in the de broglie wavelength calculator above, review the step-by-step solution, and compare against the worked examples below so you can see how each input changes the result. This free online physics tool is built for homework, design checks, and professional verification.

de Broglie Wavelength Calculator Theory & Explanation

de Broglie relation

Every particle of momentum p has an associated wavelength inversely proportional to p:

\lambda = (h)/(p)

Non-relativistic form

For a particle of mass m and speed v (much less than c), momentum p = m v, so

\lambda = (h)/(m \, v)

Thermal de Broglie wavelength

For a gas of mass m at temperature T, the typical de Broglie wavelength is the "thermal wavelength":

\Lambda = (h)/(√(2 π m k_B T))

Why everyday objects don't diffract

A 1 kg ball at 1 m/s has λ = 6.6×10⁻³⁴ m, far smaller than any subatomic distance. Real macroscopic objects have such short wavelengths that wave behavior is unmeasurable — this is why classical mechanics works at everyday scales.

Electron diffraction

A beam of electrons accelerated through ~100 V has de Broglie wavelength on the order of 0.1 nm — about the size of an atom. This is why electron microscopes resolve structures a thousand times finer than visible-light microscopes.

Why Macroscopic Objects Show No Wave Behaviour

Planck's constant is about 6.626×10^-34\ \mathrmJ\,s, and it sits in the numerator. Any everyday momentum therefore produces a wavelength far too small to observe.

A 150 g cricket ball at 40 m/s has momentum 6 kg·m/s and a de Broglie wavelength around 1.1×10^-34 m — roughly twenty orders of magnitude smaller than a proton. No aperture could ever diffract it, so the ball follows a classical trajectory. An electron, by contrast, has a mass of only 9.11×10^-31 kg, so even at modest speeds its wavelength lands in the range of atomic spacings, where crystal lattices act as ready-made diffraction gratings. The transition between quantum and classical behaviour is not a change in the physics; it is simply that h is small.

\lambda = (h)/(p) = (h)/(mv)

Wavelength from Accelerating Voltage

For a charged particle accelerated from rest through a potential difference V, the kinetic energy is qV, so the momentum is p = √(2mqV) and the wavelength follows directly. For electrons this yields a convenient shortcut: \lambda ≈ √(1.5/V) nanometres, with V in volts.

So 100 V gives about 0.123 nm, 10 kV about 0.0123 nm, and the 100–300 kV of a transmission electron microscope gives a few picometres — though above roughly 50 kV a relativistic correction becomes necessary, since the electrons are moving at an appreciable fraction of c. This relationship is the design equation for electron optics: raising the accelerating voltage shortens the wavelength and improves the diffraction-limited resolution, at the cost of more radiation damage to the specimen.

\lambda = (h)/(√(2mqV))

Experimental Confirmation and Matter-Wave Limits

Davisson and Germer confirmed the hypothesis in 1927 by scattering electrons off a nickel crystal and finding diffraction peaks exactly where the de Broglie wavelength predicted; G. P. Thomson independently demonstrated it with thin foils. The irony is often noted that J. J. Thomson won a Nobel Prize for showing the electron is a particle and his son won one for showing it is a wave.

Since then, matter-wave interference has been demonstrated with neutrons, whole atoms, and molecules as large as fullerenes and beyond — in each case with wavelengths measured in picometres. Neutron diffraction is now a routine tool for locating hydrogen atoms in crystals, where X-rays struggle. The practical ceiling is not any sudden failure of the relation but decoherence: the larger the object, the more it interacts with its surroundings, and the more quickly the phase relationship that makes interference visible is destroyed.

de Broglie Wavelength Calculator Worked Examples

Worked Example

Inputs

  • mass: 9.1093837015e-31
  • velocity: 10000000

Result: wavelength: 7.274e-11 wavelengthNm: 0.0727 momentum: 9.109e-24

Explanation

An electron (9.11×10⁻³¹ kg) accelerated to 10⁷ m/s has momentum p = 9.11×10⁻²⁴ kg·m/s and de Broglie wavelength λ = 6.626×10⁻³⁴ / 9.11×10⁻²⁴ ≈ 7.27×10⁻¹¹ m = 0.073 nm — small enough to resolve single atoms.

Second Scenario

Inputs

  • mass: 1
  • velocity: 10000000

Result: wavelength: 7.274e-11 wavelengthNm: 0.0727 momentum: 9.109e-24

Explanation

This scenario uses different inputs (mass = 1, velocity = 10000000) to show how changing one variable affects the de broglie wavelength result. Run the calculator above with these values to get the exact updated output with step-by-step work.

Common de Broglie Wavelength Calculator Use Cases

  • Physics problem sets and labs
  • Engineering design checks
  • Unit and formula verification
  • Scattering
  • And interference behavior.

de Broglie Wavelength Calculator FAQs

Does the de Broglie wavelength depend on mass?

It scales as 1/m: heavier particles at the same speed have shorter wavelengths. A proton has nearly 2000× the mass of an electron, so its de Broglie wavelength is about 1/2000 as large at the same speed.

Is the formula valid at relativistic speeds?

In special relativity, momentum is p = γ m v and the speed c replaces v for the limit. The full relativistic form is λ = h/(γ m v). For most practical applications at electron voltages of a few hundred, non-relativistic is accurate; at multi-kV the relativistic correction matters.

Why don't we see matter waves for everyday objects?

Their wavelengths are absurdly small (10⁻³⁰ m for a 1 kg object moving at 1 m/s). To see interference, you need slits spaced on the order of the wavelength. Matter-wave interference has been demonstrated for individual electrons, neutrons, and even large molecules like buckminsterfullerene (C60) — but never for an object visible to the eye.

How does electron diffraction work?

When a beam of mono-energetic electrons strikes a crystal, the electrons scatter off lattice planes. Constructive interference occurs when the path difference between waves from adjacent planes equals an integer multiple of the wavelength. This is the principle behind every electron-diffraction pattern.

Do I need the relativistic formula?

Use the relativistic momentum once the particle exceeds roughly 10% of the speed of light, where the classical result is already about 0.5% low. For electrons that threshold is around 2.6 keV, so any electron microscope above a few kilovolts needs the correction — at 100 kV the classical wavelength is too large by more than 20%.