De Broglie Wavelength Calculator

Calculate the de Broglie wavelength of a particle based on its mass and velocity, revealing the wave-like nature of matter in quantum mechanics.

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What is the De Broglie Wavelength?

In 1924, Louis de Broglie proposed that all matter exhibits wave-like properties, with a wavelength inversely proportional to its momentum. This revolutionary hypothesis, which earned him the Nobel Prize in Physics in 1929, bridged the gap between classical mechanics and quantum theory. It suggested that particles such as electrons, protons, and even macroscopic objects have an associated wavelength, though for everyday objects this wavelength is so incredibly small as to be undetectable.

The de Broglie wavelength is fundamentally important in quantum mechanics. It determines when quantum effects become significant: if the de Broglie wavelength of a particle is comparable to the size of the system it interacts with, quantum behavior dominates. This is why electrons exhibit wave-like diffraction patterns when passing through crystal lattices, as demonstrated by the Davisson-Germer experiment in 1927.

The Formula

λ = h / (m × v) = h / p

Where λ is the de Broglie wavelength, h is Planck's constant (6.626 x 10^-34 J·s), m is the particle mass, v is the velocity, and p is the momentum. For relativistic particles, the relativistic momentum p = γmv must be used, where γ is the Lorentz factor.

Wavelength Examples

ParticleVelocityWavelength
Electron10^6 m/s0.727 nm
Proton10^6 m/s3.96 x 10^-4 nm
Baseball (0.145 kg)40 m/s1.14 x 10^-25 nm
Electron at 100 eV5.93 x 10^6 m/s0.123 nm

Physical Significance

  • Electron microscopy exploits small de Broglie wavelengths for high resolution imaging
  • Neutron diffraction uses thermal neutron wavelengths to study crystal structures
  • Atom interferometry relies on the wave nature of atoms for precision measurements
  • Quantum tunneling probability depends on the de Broglie wavelength

Frequently Asked Questions

Do macroscopic objects have a de Broglie wavelength?

Yes, but it is incredibly small. A 1 kg object moving at 1 m/s has a wavelength of about 6.6 x 10^-34 meters, which is far smaller than any atomic nucleus. This is why we never observe wave behavior in everyday objects. Quantum effects only become observable when the wavelength is comparable to the size of the relevant structures.

How is this used in electron microscopy?

Electron microscopes accelerate electrons to high energies, giving them very short de Broglie wavelengths (picometers). Since resolution is limited by wavelength, electron microscopes can resolve features thousands of times smaller than optical microscopes, which are limited by visible light wavelengths (400-700 nm).

What happens at very high velocities?

When velocities approach the speed of light, relativistic corrections are needed. The relativistic de Broglie wavelength uses relativistic momentum: λ = h / (γmv), where γ = 1/sqrt(1 - v^2/c^2). At v = 0.9c, the wavelength is about 2.3 times smaller than the non-relativistic prediction.