
Optional unit · institution-dependent · Interactive lesson
Wave packets and the uncertainty principle
This is where the uncertainty principle stops being a slogan. You build a localised packet out of plane waves, see why squeezing it in x must broaden it in k, follow it at the group velocity while it spreads, and learn to read ΔE Δt as the width of a spectral line.
UPIII-09.05 · Lesson 5 of 9 in this unit. Position is not a completion score.Optional unit · institution-dependent. This modern-physics material is an introductory survey, not a complete course in relativity, quantum, atomic, nuclear or particle physics. Your university determines the required depth and assessment. Optional work is not a required completion gate.
Build the model
To be somewhere, a wave has to be made of many wavelengths.
The key idea
A wave packet is a superposition of plane waves spanning a band of wavenumbers, localised because the components cancel away from its centre; its rms widths obey Δx Δk ≥ ½, and with p = ħk, Δx Δp ≥ ħ/2.
Example. An electron packet with Δx = 0.10 nm needs Δk ≥ 1/(2 × 0.10 nm) = 5.0 nm⁻¹, so Δp ≥ 5.3 × 10⁻²⁵ kg m s⁻¹ and Δv ≥ 5.8 × 10⁵ m s⁻¹, about a quarter of the electron's speed in the hydrogen ground state.
The complete physical model and assumptions
A plane wave e(i(kx − ωt)) has one wavenumber, so by de Broglie one momentum ħk, and |ψ|² is the same everywhere: it describes a particle that is nowhere in particular. To put an electron somewhere, superpose plane waves over a band of wavenumbers, ψ(x) = (1/√(2π)) ∫ φ(k) e(ikx) dk. At the centre the components are in phase and add; a distance x away their phases have fanned out by about x Δk, and once that fan approaches a full turn they cancel. That is a theorem about Fourier pairs, not about electrons: the rms widths obey Δx Δk ≥ ½, with equality only for a Gaussian that carries no chirp. Multiply by ħ and it becomes Δx Δp ≥ ħ/2, a property of the state that no instrument can refine. The packet then moves at the group velocity dω/dk, which for ω = ħk²/2m is ħk₀/m, the classical velocity p/m, while its crests move at half that. Because different wavenumbers travel at different speeds, a free packet that starts as an unchirped Gaussian spreads: Δp is fixed, Δx grows, and the product climbs above its floor. Time is a parameter with no operator, so the energy-time relation says something different: a state that lasts only τ has its energy blurred by Γ = ħ/τ, which a spectrometer sees as a linewidth. The model is non-relativistic and single-particle. The Fourier bound survives relativity; ω = ħk²/2m, and the spreading rate built on it, do not.
1One wavelength means no location
A plane wave ψ = e(i(kx − ωt)) has a single wavenumber, so through p = ħk a single momentum, but |ψ|² = 1 at every x: it describes a particle that could be anywhere. Add a second wave and a location starts to appear. Waves with k₁ = 9.5 nm⁻¹ and k₂ = 10.5 nm⁻¹ sum to a carrier at 10 nm⁻¹ inside an envelope 2 cos(Δk x/2) whose beats repeat every 2π/Δk = 6.3 nm. Fill the band between them with many waves and the repeats disappear: the sum stays large only near x = 0. Treat each component as a phasor. At x = 0 they all point the same way; at distance x the phase of component k is kx, so across the band the phasors fan out by x Δk. When the fan has opened into a full circle, at x Δk = 2π for a flat band, they sum to zero, which is the packet's first null: 6.3 nm for a band 1.0 nm⁻¹ wide. A narrower band needs a larger x to close the fan, so a narrow spread of k can only build a wide packet.
2The rms widths obey Δx Δk ≥ ½
To turn “narrow needs broad” into a law, measure both widths the same way: Δx is the standard deviation of |ψ(x)|² and Δk that of |φ(k)|². A Gaussian packet ψ ∝ e(−x²/4σ²) e(ik₀x) transforms into φ ∝ e(−σ²(k − k₀)²); squaring each gives Δx = σ and Δk = 1/(2σ), so Δx Δk = ½ whatever σ is. No shape does better, which is the Fourier uncertainty theorem, and most do worse. Give the Gaussian a chirp, a phase e(iCx²/4σ²) that makes the local wavenumber drift across it: |ψ|² is untouched, but Δk grows by √(1 + C²), so C = 1 costs 41% more bandwidth and buys no localisation at all. The constant also depends on which width you quote. The full widths at half maximum of the same Gaussian pair multiply to 8 ln 2 × ½ = 2.77, and a flat band measured to its first null gives 2π, so order-of-magnitude statements say only that Δx Δk is of order 1. The floor of exactly ½ belongs to rms widths.
3Multiply by ħ: a spread in the state, not in the ruler
De Broglie's p = ħk carries the theorem straight into mechanics: Δx Δp ≥ ħ/2, with ħ = 1.055 × 10⁻³⁴ J s. Nothing in the derivation mentions a measurement. Δx and Δp are the spreads of the results that ideal position and momentum measurements would return on many identically prepared particles, and a state narrow in both does not exist to be prepared. The size of ħ decides where this matters. An electron confined to Δx = 0.10 nm has Δp ≥ 5.3 × 10⁻²⁵ kg m s⁻¹, and because ⟨p²⟩ ≥ Δp², its mean kinetic energy is at least Δp²/2m = 0.95 eV: atomic confinement costs electron-volts, the energy scale of chemistry. A 1 μg dust grain held to 1 μm has Δv ≥ 5.3 × 10⁻²⁰ m s⁻¹, far below any thermal or instrumental jitter. That is the correspondence check: as m grows at fixed Δx, or as ħ → 0, the bound fades and a sharp classical trajectory is recovered.
4The envelope moves at dω/dk, the crests at ω/k
Let the packet evolve. Each component carries its own time factor e(−iω(k)t), and for a narrow band ω(k) ≈ ω₀ + vg(k − k₀) with vg = [dω/dk]₀. Pulling out e(i(k₀x − ω₀t)) leaves an integral that depends on x and t only through x − vg t, so the envelope translates at vg while the crests move at the phase velocity ω₀/k₀. For a free electron ω = E/ħ = ħk²/2m, so vg = ħk₀/m = p/m, the classical velocity, while vₚ = ħk₀/2m is half of it and the crests slide backwards through the envelope. At k₀ = 8.0 nm⁻¹ (λ = 0.79 nm, 2.4 eV) the packet moves at 9.3 × 10⁵ m s⁻¹ and its crests at 4.6 × 10⁵ m s⁻¹. The relativistic check agrees: with ω² = c²k² + (mc²/ħ)², vg = c²k/ω = pc²/E, again the particle velocity and always below c, even though vₚ = c²/vg exceeds c. Energy and information ride on the envelope.
5Dispersion makes a free packet spread
The next term in the expansion, ½(ħ/m)(k − k₀)², is where the band of k matters: components faster than vg run ahead, slower ones fall behind, and the leading edge collects the short wavelengths. For a packet that starts as an unchirped Gaussian the result is exact: Δx(t)² = Δx₀² + (Δv t)², with Δv = Δp/m = ħ/(2mΔx₀). Initial size and velocity spread add in quadrature, and tₛ = 2mΔx₀²/ħ marks where spreading takes over. An electron packet with Δx₀ = 0.50 nm has tₛ = 4.3 fs and doubles its width after √3 tₛ = 7.5 fs; a 1 μg grain held to 1 μm has tₛ = 1.9 × 10¹³ s, some 600 000 years. Throughout, |φ(k)|² never changes, because a free particle's momentum distribution is conserved. So Δp stays fixed while Δx grows, and Δx Δp = (ħ/2)√(1 + (t/tₛ)²) climbs off the floor: the packet has acquired exactly the chirp that spoils minimum uncertainty.
6Energy and time: a lifetime is a linewidth
Position and momentum are both observables, and the bound on their spreads follows from their operators. Time is not an observable here; it is the parameter the state evolves in, so ΔE Δt cannot be read the same way. Its precise content concerns change. A stationary state goes as e(−iEt/ħ) forever and has a sharp energy. An excited state that decays with mean lifetime τ has an amplitude e(−iE₀t/ħ) e(−t/2τ), and a wave train that dies away is a packet in time: its Fourier transform is a Lorentzian in energy with full width at half maximum Γ = ħ/τ. A level with τ = 20 ns is therefore blurred by Γ = 3.3 × 10⁻⁸ eV, a natural linewidth of 1/(2πτ) = 8.0 MHz, set by the decay rather than by any spectrometer. Particle physics reads the relation backwards: the Z boson's measured width of 2.50 GeV gives τ = ħ/Γ = 2.6 × 10⁻²⁵ s, a lifetime no clock could time.
Key equations
Read the units, assumptions and limits before substituting.
Fourier synthesis of a packet
ψ(x, 0) = (1/√(2π)) ∫ φ(k) e(ikx) dk
Any localised shape is a sum of plane waves. The band of k that φ(k) occupies decides how narrow the sum can be made.
k in m⁻¹, integrated over all k; φ(k) is the amplitude per unit k, in m¹⁄² when ψ is in m(−1/2)Reciprocal width theorem
Δx Δk ≥ ½
Halve a packet and the narrowest band of wavenumbers that can build it doubles. Pure Fourier analysis: it holds for sound, light and water waves alike.
Δx (m) and Δk (m⁻¹) are the rms widths of |ψ(x)|² and |φ(k)|²; equality only for an unchirped GaussianPosition–momentum uncertainty relation
Δx Δp ≥ ħ/2
Confining an electron to 0.10 nm forces Δp ≥ 5.3 × 10⁻²⁵ kg m s⁻¹, an energy scale near 1 eV; a 1 g bead held to 1 μm needs only Δv ≥ 5 × 10⁻²⁶ m s⁻¹.
p = ħk; ħ = h/2π = 1.055 × 10⁻³⁴ J s; Δx in m, Δp in kg m s⁻¹Group velocity of a free packet
vg = [dω/dk]₀ = ħk₀/m
The envelope moves at the classical velocity p/m. The crests move at ω₀/k₀ = vg/2 and slide backwards through it.
[ ]₀ means evaluated at the central wavenumber k₀; vg in m s⁻¹; uses the free, non-relativistic ω = ħk²/2mSpreading of a free Gaussian packet
Δx(t) = Δx₀ √[1 + (ħt/(2mΔx₀²))²]
Initial size and velocity spread add in quadrature. An electron packet of rms width 0.50 nm doubles it in 7.5 fs; narrower starts spread faster.
Δx₀ the initial rms width in m for an unchirped start, t in s, m in kg; equivalently Δx² = Δx₀² + (Δv t)², Δv = ħ/(2mΔx₀)Lifetime and natural linewidth
Γ = ħ/τ
A level living 20 ns is blurred by Γ = 3.3 × 10⁻⁸ eV, a line 8.0 MHz wide. The width comes from the decay, not from any energy measurement.
Γ the full width at half maximum of the line, in J or eV; τ the mean lifetime in s; ħ = 6.582 × 10⁻¹⁶ eV sInteractive lab
Predict first. Explore the model. Compare the result.
Explore the model
Try this. At t = 0, drag σ₀ from 1.5 to 0.4 nm: the packet narrows, |φ(k)|² broadens, and Δx Δk stays pinned at 0.50. Then advance t: the envelope runs at ħk₀/m while the crests drift back through it, Δx grows, Δk does not, and the product climbs off the floor.
Live results
- RMS WIDTH Δx
- 0.60 nm
- RMS SPREAD Δk
- 0.83 nm⁻¹
- Δx Δk (FLOOR 0.50)
- 0.50
- GROUP VELOCITY ħk₀/m
- 926 km s⁻¹
Results follow this lesson’s model and assumptions. Displayed values are rounded.
Predict → change one variable → check
Plan a change before running it. Every other input stays at the saved baseline.
Saved baseline. Initial rms width σ₀: 0.6 nm; Central wavenumber k₀: 8.0 nm⁻¹; Time since preparation t: 0.0 fs
This experiment is kept only while this page is open. It does not change saved course progress.
Catch the common trap
The commonest misreading is that the uncertainty principle limits instruments: measure more gently, or with a sharper probe, and Δx Δp could be pushed below ħ/2. It cannot, because the bound was derived before any instrument appeared. Δx and Δp are the widths of |ψ(x)|² and |φ(k)|² for one state, and the Fourier theorem forbids a state narrow in both. A single position reading can be as sharp as the detector allows; what cannot both be small are the scatter of position results and the scatter of momentum results over many identically prepared particles. Heisenberg's microscope, in which the photon that locates an electron also kicks it, is a separate statement about disturbance. Instrument error adds to the intrinsic spread and never replaces it: remove every source of it and ħ/2 is still there.
Practice & worked examples
3 authored examples. Make an attempt, then reveal the reasoning one step at a time.
EasyExample 1
An electron in a GaAs quantum dot behaves as a particle of effective mass m* = 0.067 mₑ. The dot confines it to an rms width Δx = 5.0 nm along one direction. Find the least possible Δp, the minimum mean kinetic energy this implies for that direction, and whether that energy stands out at 300 K or only at 4.2 K.
Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.
0 of 5 steps revealed.
- The uncertainty floor: Δp ≥ ħ/(2Δx) = 1.055 × 10⁻³⁴ J s ÷ (2 × 5.0 × 10⁻⁹ m) = 1.055 × 10⁻²⁶ kg m s⁻¹.
- The mean kinetic energy is ⟨p²⟩/2m*, and ⟨p²⟩ = Δp² + ⟨p⟩² ≥ Δp², so ⟨K⟩ ≥ Δp²/2m*. The effective mass is m* = 0.067 × 9.11 × 10⁻³¹ kg = 6.10 × 10⁻³² kg.
- ⟨K⟩ ≥ (1.055 × 10⁻²⁶ kg m s⁻¹)² ÷ (2 × 6.10 × 10⁻³² kg) = 9.1 × 10⁻²² J = 5.7 meV.
- Compare with kT. At 300 K, kT = 25.9 meV, 4.5 times larger, so thermal agitation swamps the confinement. At 4.2 K, kT = 0.36 meV, 16 times smaller, so the confinement energy dominates.
- Check the role of the mass: a free electron confined the same way would have a floor of only 0.38 meV. The small effective mass is what lifts the confinement energy 15-fold.
Answer. Δp ≥ 1.1 × 10⁻²⁶ kg m s⁻¹ and ⟨K⟩ ≥ 5.7 meV for that direction: below kT = 26 meV at 300 K, but 16 times kT at 4.2 K, so the confinement shows up only when the dot is cooled.
MediumExample 2
An electron gun emits 50.0 eV electrons in packets that start as unchirped Gaussians with Δx₀ = 0.40 nm along the beam. Find the central wavenumber, the group and phase velocities, and how far a packet travels before its width has doubled. Check that the narrow-band and non-relativistic approximations are safe.
Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.
0 of 5 steps revealed.
- Momentum from the kinetic energy: p = √(2mE) = √(2 × 9.109 × 10⁻³¹ kg × 50.0 × 1.602 × 10⁻¹⁹ J) = 3.82 × 10⁻²⁴ kg m s⁻¹, so k₀ = p/ħ = 3.62 × 10¹⁰ m⁻¹ = 36.2 nm⁻¹ (λ = 0.173 nm).
- Group velocity vg = ħk₀/m = p/m = 4.19 × 10⁶ m s⁻¹, the classical speed of a 50 eV electron. Phase velocity vₚ = ω₀/k₀ = ħk₀/2m = 2.10 × 10⁶ m s⁻¹, half as much.
- Approximations: Δk = 1/(2Δx₀) = 1.25 nm⁻¹, so Δk/k₀ = 0.035 and the band is narrow. E/mc² = 50.0 eV ÷ 511 keV = 9.8 × 10⁻⁵, so ω = ħk²/2m holds.
- Spreading: Δx(t) = Δx₀√(1 + (t/tₛ)²) with tₛ = 2mΔx₀²/ħ = 2 × 9.109 × 10⁻³¹ kg × (0.40 × 10⁻⁹ m)² ÷ 1.055 × 10⁻³⁴ J s = 2.76 × 10⁻¹⁵ s.
- The width doubles when 1 + (t/tₛ)² = 4, at t = √3 tₛ = 4.79 fs. In that time the envelope moves vg t = 4.19 × 10⁶ m s⁻¹ × 4.79 × 10⁻¹⁵ s = 2.0 × 10⁻⁸ m.
Answer. k₀ = 36.2 nm⁻¹, vg = 4.19 × 10⁶ m s⁻¹, vₚ = 2.10 × 10⁶ m s⁻¹; the width reaches 0.80 nm after 4.8 fs, when the packet is about 20 nm down the beam.
HardExample 3
An excited atomic level with mean lifetime τ = 25 ns emits at 650 nm. For t ≥ 0 model the emitted field as E₀ e(−t/2τ) e(−iω₀t), so the intensity falls as e(−t/τ). Integrate to find the line shape, give the natural linewidth in angular frequency, frequency, energy and wavelength, and decide whether a spectrometer of resolving power λ/Δλ = 1.0 × 10⁶ can see it.
Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.
0 of 6 steps revealed.
- The spectrum is the Fourier integral Ẽ(ω) = ∫₀^∞ E₀ e(−t/2τ) e(i(ω − ω₀)t) dt = E₀ / [1/(2τ) − i(ω − ω₀)], the upper limit contributing nothing because e(−t/2τ) → 0.
- The power spectrum is |Ẽ(ω)|² = E₀² / [(ω − ω₀)² + 1/(4τ²)], a Lorentzian centred on ω₀. It falls to half its peak where (ω − ω₀)² = 1/(4τ²), so its full width at half maximum is Δω = 1/τ = 4.0 × 10⁷ rad s⁻¹.
- In frequency Δf = 1/(2πτ) = 6.4 MHz. In energy Γ = ħΔω = ħ/τ = 6.582 × 10⁻¹⁶ eV s ÷ 2.5 × 10⁻⁸ s = 2.6 × 10⁻⁸ eV.
- The photon energy is hc/λ = 1239.8 eV nm ÷ 650 nm = 1.91 eV, so Γ/E = 1.38 × 10⁻⁸. The same fraction of the wavelength gives Δλ = 650 nm × 1.38 × 10⁻⁸ = 9.0 × 10⁻⁶ nm.
- A resolving power of 1.0 × 10⁶ resolves 650 nm ÷ 10⁶ = 6.5 × 10⁻⁴ nm, about 72 times the natural width, so the instrument sets the observed width. Seeing the natural width would need λ/Δλ ≈ 7 × 10⁷.
- Limits: as τ → ∞ the Lorentzian collapses to a spike at ω₀, the sharp energy of a stationary state. Its tails fall only as 1/(ω − ω₀)², so its rms width diverges, which is why the lifetime relation is stated as Γτ = ħ with a full width rather than as an rms inequality.
Answer. A Lorentzian with Δω = 1/τ = 4.0 × 10⁷ rad s⁻¹: Δf = 6.4 MHz, Γ = 2.6 × 10⁻⁸ eV and Δλ = 9.0 × 10⁻⁶ nm. A resolving power of 10⁶ is about 70 times too coarse to see it.
Quick check
Select an answer and explain it before checking.
Review & continue
A wave packet is a superposition of plane waves spanning a band of wavenumbers, localised because the components cancel away from its centre; its rms widths obey Δx Δk ≥ ½, and with p = ħk, Δx Δp ≥ ħ/2.
- Explain the relationship without looking at the equation.
- Check a sign, a unit and a model assumption in your working.
- Return to the lab or worked example if a step is still unclear.
Optional supporting lessons
These chapter resources can help with earlier ideas; they are not additional required Physics III completion tasks.