equation

de Broglie formula

The de Broglie wavelength is the wavelength associated with a particle, given by λ = h/p.
10 related articles · 6 formulas · 1 who worked here

Description

Everything around us — not just light, but also matter particles, such as electrons — behaves like waves! Every moving particle has its own wavelength, calculated using the de Broglie formula. For large objects, this wavelength is vanishingly small, so we don't see a ball bending around corners. But for tiny particles, it is large enough to exhibit wave properties.

History

Louis de Broglie in 1924 suggested the universality of wave-particle duality, extrapolating the results of Planck and Einstein for light to all particles. In 1927, Clinton Davisson and Lester Germer experimentally discovered diffraction of slow electrons on nickel, and George Thomson in thin metal films. These experiments confirmed the hypothesis, and Erwin Schrödinger soon developed the mathematical apparatus to describe de Broglie waves.

How it works

The de Broglie formula is used to calculate diffraction gratings in electron and neutron optics, estimate quantum effects (tunneling, interference) during microparticle motion, and in scattering theories. In the macroscopic limit (m large), λ becomes negligibly small, consistent with classical mechanics. For ultra-relativistic particles, a relativistic expression for momentum is required.

Fun fact

If you throw a baseball, its de Broglie wavelength would be billions of times smaller than an atomic nucleus — no diffraction would be noticeable. But for a slowly moving electron, it can be the size of a molecule!

Concept graph →

Formulas

$$\lambda = \frac{h}{p}$$
Wavelength of a particle equals Planck's constant divided by momentum.
What is in the formula
\lambdavariablede Broglie wavelength of the particle — wavelength metre
pvariablemomentum of the particle — momentum kilogram metre per second
hconstantPlanck constant, the quantum of action — planck constant = 6.62607015e-34 joule second
λ=\frac{h}{p} · 2607.03465
\langle|{q}|^2\rangle\propto(n_e/ν) · 2607.08822
λ=\frac{h}{p}=\frac{h}{\sqrt{2me}} · 2607.10388
λ=\frac{h}{m_gc} · 2607.11764
$$d = \frac{0.61\lambda}{\sin\alpha}$$
Minimum resolvable distance depends on wavelength and aperture angle.
What is in the formula
dvariableMinimum resolvable distance between two point sources — distance metre
λvariableWavelength of the light — wavelength metre
αvariableHalf-angle of the aperture (angular radius) — angle radian
0.61constantConstant arising from the diffraction pattern of a circular aperture — airy disk factor = 0.61
d=\frac{0.61λ}{\sinα} · 2607.10388
$$\Box \varphi = -4\pi \rho$$
The wave equation for a scalar field with a source term.
What is in the formula
\varphivariablescalar field — scalar field
\rhovariablesource density — source density per cubic metre
\BoxoperatorLorentz-invariant second-order differential operator — d alembertian operator
\box\varphi^{(1)}=-4πdμ\int\frac{δ^{(4)}(x-y_p(τ))}{\sqrt{-g}}dτ · 2607.09310
$$\hat{H} \Psi = 0$$
The Hamiltonian constraint annihilates the wave function of the universe.
What is in the formula
ΨvariableWave function of the universe — wave function
ĤoperatorActs on the wave function to give total energy including gravitational and matter contributions — hamiltonian operator
\hat{h}\psi=0 · 2603.06481
\hat{h}|\psi\rangle=0 · 2605.06093v1
$$P = |\psi|^2$$
Probability equals the square of the wavefunction amplitude.
What is in the formula
Pvariableprobability density — probability density per metre cubed
ψvariablewavefunction — wave function per metre to the three halves
p=|ψ|^2 · 2604.07418
p=|ψ|^2 · 2605.16148
p(x)=|\langlex|ψ\rangle|^2 · 2606.28199
$$\Omega h^{3/2}$$
Combination of density parameter and Hubble constant.
What is in the formula
\OmegavariableDensity parameter (total energy density relative to critical) — density parameter
hvariableDimensionless Hubble constant (H0/100 km/s/Mpc) — hubble constant dimensionless
ω_mh^{3/2} · 2607.24694v1

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