In 1924, Louis de Broglie proposed a radical idea: if light — long understood as a wave — could also behave as discrete particles (photons), then matter, long understood as particles, should also have a wave nature. This calculator applies his relation, λ = h/p, to find the wavelength of the matter wave associated with any moving object, from a subatomic electron to a thrown baseball.
How the de Broglie Wavelength Calculator works
The calculator implements λ = h/p, where h is Planck's constant and p is the particle's momentum. If you know mass and velocity, momentum is simply p = mv (the From Mass & Velocity tab). If momentum is already known from another calculation, the From Momentum tab skips straight to λ = h/p. If instead you know kinetic energy — as when an electron has been accelerated through a known voltage — the From KE tab first recovers momentum from p = √(2m·KE), then applies the same formula.
All three tabs use the CODATA-exact value of Planck's constant, h = 6.62607015 × 10⁻³⁴ J·s, fixed by the 2019 redefinition of the SI base units.
Inputs and what they mean
Mass is entered in kilograms — for subatomic particles this means very small numbers in scientific notation (an electron's mass is 9.10938 × 10⁻³¹ kg), while everyday objects use ordinary decimal values. Velocity is in meters per second. Momentum, when entered directly, is in kilogram-meters per second (kg·m/s). Kinetic energy on the From KE tab is entered in electronvolts (eV) rather than joules, since eV is the standard unit for particle-scale energies — 1 eV is the energy an electron gains crossing a 1-volt potential difference, so an electron accelerated through 100 V has exactly 100 eV of kinetic energy.
Limits and edge cases
The From KE tab uses the non-relativistic approximation p = √(2m·KE), which is accurate as long as kinetic energy stays well below the particle's rest-mass energy (511 keV for an electron). At relativistic speeds this simplified formula underestimates momentum and overestimates wavelength — a limitation shared with most introductory-level de Broglie calculations. The formula also assumes a free, non-interacting particle; wavelengths for bound or confined particles (like electrons in an atom) are a useful conceptual guide but require full quantum mechanics for exact results. Finally, for macroscopic objects the de Broglie wavelength is so many orders of magnitude smaller than anything physically measurable that the result is a mathematical curiosity rather than an observable effect.