Electron accelerating-voltage wavelength Created 2026-10-14 Updated 2026-10-20
Let an electron start with negligible kinetic energy and move through an increase in electric potential. Its electric charge is , where is the elementary charge, so the decrease in potential energy is . In a field-free region after acceleration,This is an electron formula, not a universal conversion from voltage to wavelength. It assumes negligible initial kinetic energy, negligible losses, and , where is the speed of light. It describes the de Broglie wavelength outside the crystal; the potential energy inside a material can change the local kinetic momentum.
For , take , , and . The rounded electron mass is consistent with the 2022 recommended constants.[ref]
CODATA Value: electron mass by National Institute of Standards and Technology. CODATA electron mass: numerical value and 2022 adjustment label
The electronvolt is an energy unit: must be converted to joules before combining it with in SI units. Dimensional analysis checks both steps:The resulting velocity is about , or , so the nonrelativistic assumption is consistent. For a larger accelerating voltage, the relativistic energy-momentum relation gives , with , while still holds. At the relativistic wavelength is shorter by about .Explicitly, the exact special relativity formula and its nonrelativistic quantum mechanics limit areHere is the gained kinetic energy; the total energy is . At , the nonrelativistic quantum mechanics expression gives , about larger than the exact . This difference matters when using electron diffraction ring positions to infer lattice plane spacings.
Electron microscope resolution Created 2026-10-18 Updated 2026-10-20
Electron microscope resolution concerns distinguishable specimen detail under a specified contrast criterion. It depends on diffraction, lens defects, electron energy spread, specimen motion and detection. A smaller de Broglie wavelength permits finer detail in principle, but neither wavelength nor magnification is the instrument's measured resolution.
For an electron accelerated from negligible initial kinetic energy through a positive electric potential difference , combine , the relativistic energy-momentum relation and the de Broglie wavelength:Here is the Planck constant, the electron mass, the elementary charge, and the speed of light. This includes the relativistic correction omitted by the low-voltage electron accelerating-voltage wavelength approximation. With and SI defining values of , calculated wavelengths are approximately , and at , and respectively. The rounded mass agrees with the recommended value.[ref]
For a circular aperture admitting a small semi-angle , the Rayleigh criterion suggests a diffraction-limited resolution scale . At and , this gives , already much larger than the wavelength. This is an ideal aperture estimate. Transmission electron microscopy with coherent illumination and a particular specimen requires its own image-contrast analysis; this scale alone is not a universal two-feature resolution test.
An original illustrative blur model adds competing effects:Define as a characteristic transverse blur from the electron-lens analogue of spherical aberration, and as one from energy-dependent focusing, the analogue of chromatic aberration. The coefficients have units of length, is a chosen characteristic kinetic energy spread, and is a fixed residual blur. Adding their squares is a declared heuristic, not a measured point spread function or a rigorous resolution theorem. The model omits contrast transfer, specimen scattering and signal statistics, so its minimum is only an estimate within its assumptions.
Choose , and at . At , the four contributions are about , , and , giving . At , the diffraction contribution falls to but the assumed spherical aberration contribution grows to . Thus opening the aperture indefinitely worsens this model's image. All these values are calculations with chosen parameters, not observations of any microscope.
Schrödinger equation Created 2026-09-24 Updated 2026-10-20
The Schrödinger equation governs the evolution of a quantum state between instances of measurement in quantum mechanics. For a particle of mass moving in a prescribed real potential energy , its position wavefunction satisfiesHere is the Planck constant, is the Laplace operator, and the Hamiltonian operator combines kinetic energy with potential energy. Specify an initial wavefunction, an operator domain and any boundary conditions: the differential expression alone does not completely specify a physical model. The Born rule then turns the evolving probability amplitude into position probabilities through and integration over a region.
This scalar Schrödinger operator describes nonrelativistic quantum mechanics, with relevant momenta much smaller than , where is the speed of light. It omits the constant rest energy , assumes fixed particle number, and suppresses active spin dynamics and coupling to a magnetic vector potential. A free electron with a fixed, uncoupled spin state can still use this scalar model; the Pauli equation supplies the additional spin components and magnetic coupling when needed. A prescribed real describes a closed evolution model or an approximation in which the source of that potential energy is treated as external. Dissipation, particle creation and a general measurement in quantum mechanics need further modelling.
For a time-independent self-adjoint Hamiltonian operator, the spectral theorem defines unitary time evolution byInitial states in the operator domain satisfy the differential equation in the Hilbert space sense; the unitary operator also evolves all other states in that Hilbert space. Time-dependent Hamiltonian operators need suitable regularity and domain hypotheses; their evolution is not generally the exponential of .
The local reason for conservation is especially tangible. Multiply the Schrödinger equation by the complex conjugate , subtract its conjugate multiplied by , and use the fact that the real potential energy terms cancel. For smooth wavefunctions this gives the probability continuity equationThe divergence theorem identifies the change in probability inside a region with minus the outward probability current. Decay at infinity, or appropriate probability-conserving boundary conditions, preserves wavefunction normalization. Conservation of total probability does not require a stationary probability density.
Its usefulness comes from being a linear partial differential equation: quantum superpositions of solutions are solutions, while different quantum phases can produce interference. For a fixed Hamiltonian operator, the time-independent Schrödinger equation finds the energy eigenstates; each then acquires just its own time-dependent quantum phase. One eigenvalue problem therefore organizes both allowed energies and the evolution of arbitrary quantum superpositions, with a continuous spectrum included when required. This is the attractive bridge between a spatial wave problem and a clock: energy differences determine the rate at which relative quantum phases change. It makes atomic spectral lines, quantum tunnelling and quantum scattering calculable from a specified model.
For an explicit example without confinement, take a free particle on the whole line, , initially in a Gaussian wave packet with position standard deviation and mean momentum :Unlike a single plane wave, this wavefunction satisfies wavefunction normalization. A Fourier transform writes it as a quantum superposition of plane waves. Their dispersion relation is , so each Fourier component gains the factor . Completing the square in the resulting Gaussian integral giveswith the square root chosen continuously from . Its position probability density and standard deviation areThe centre moves with the group velocity and the wave packet spreads because different wavenumbers have different group velocities. This is unitary wave dispersion, without a random force or loss of probability. Independently, the initial momentum standard deviation is and the initial position-momentum covariance vanishes. Free evolution gives in the Heisenberg picture, henceThis independently checks the spreading law. The Gaussian integral of is one at every time; the decreasing peak is exactly offset by increasing width.
As hypothetical preparation parameters, choose a free electron with and . Using and givesThe rounded electron mass uses the 2022 adjustment.[ref]
CODATA Value: electron mass by National Institute of Standards and Technology. Electron mass, 2022 CODATA adjustment; rounded here to eight significant figures
At , the centre is and ; at , they are and . The mean kinetic energy staysIt includes both mean motion and the momentum spread. The mean speed is about and the momentum spread corresponds to , making the nonrelativistic model accurate for the appreciably occupied part of this ideal Gaussian distribution. Its mathematically unbounded tails are an idealization.The complex width also explains where the probability goes. Write , where is the dimensionless quantum phase. Differentiating the exact solution givesRelative to the moving centre, the probability current points outward on both sides for . This is a flux statement, not an additional assumption about individual particle trajectories. At and , the relative flow speeds are , about . The probability within a moving interval of half-width falls from about initially to at , exactly because of this outward probability current.
Curved quantum phase drives spreading probability current
. The same free Gaussian wave packet at . With , removing the carrier and a spatially constant quantum phase leaves . The right panel plots : negative to the left, positive to the right. Flux through the marked moving interval endpoints explains its decreasing probability. Source. Details.Historically, the 1926 Quantisierung als Eigenwertproblem (Erste Mitteilung) by Erwin Schrödinger began with the stationary hydrogen atom problem. It distinguishes discrete negative energies from a positive continuous spectrum; it is not yet the general evolution equation displayed above.[ref]
Quantisierung als Eigenwertproblem (Erste Mitteilung) by Erwin Schrödinger. Printed pp. 361–363, especially p. 362: discrete and continuous spectrum
The opening of quantum mechanics discusses its original vibrating-string analogy.In the 12 December 1933 lecture The fundamental idea of wave mechanics by Erwin Schrödinger, Erwin Schrödinger explains the move from independent rays to waves through diffraction, then applies that analogy to atomic physics. His closing pages explicitly acknowledge the difficulty of reconciling wave language with observed particle tracks. This retrospective physical argument motivates the model; it does not derive the modern Born rule from classical mechanics.[ref]
The fundamental idea of wave mechanics by Erwin Schrödinger. Nobel Lectures, Physics 1922–1941, printed pp. 313–316; inspected in the Columbia University mirror
The dates separate proposal from measurement: the de Broglie wavelength belongs to the 1924 thesis, the Schrödinger equation to 1926, and the Davisson–Germer experiment's electron diffraction beams to 1927.[ref]
The discovery of electron waves by Clinton J. Davisson. Printed pp. 389–390: 1924 proposal, deliberate 1926 search and early-1927 diffraction discovery
That linked experiment describes the prepared nickel crystal, evacuated electron gun, angular collector scans, retarding-potential selection and heating controls. Its measured collector electric current tests wave-dependent scattering probabilities; it neither measures a wavefunction directly nor establishes this equation uniquely.


