Quantum Physics
Heisenberg Uncertainty Principle
You can't simultaneously know exact position and momentum — Δx · Δp ≥ ℏ/2
The Heisenberg uncertainty principle (1927) — for any quantum particle, the product of position and momentum uncertainties is at least ℏ/2: Δx · Δp ≥ ℏ/2. Not measurement limitation but fundamental property of quantum systems. Same applies to energy-time, angular momentum components. Foundation of quantum mechanics; why electrons don't fall into nuclei; why quantum tunneling happens.
- Position-momentumΔx · Δp ≥ ℏ/2
- Energy-timeΔE · Δt ≥ ℏ/2
- Reduced Planck constantℏ = h/(2π) ≈ 1.055 × 10⁻³⁴ J·s
- DiscoveredWerner Heisenberg, 1927
- NOT measurement limitFundamental property of quantum systems
- Doesn't matter at large scalesMacroscopic objects have x and p known to absurd precision relative to ℏ
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Statement
For any quantum state, the standard deviations (uncertainties) of position and momentum satisfy:
Δx · Δp ≥ ℏ / 2
where ℏ = h/(2π) ≈ 1.055 × 10⁻³⁴ J·s.
This is fundamental — not due to measurement disturbance, but a property of quantum states themselves.
Other uncertainty relations
| Pair | Relation |
|---|---|
| Position - Momentum | Δx · Δp ≥ ℏ/2 |
| Energy - Time | ΔE · Δt ≥ ℏ/2 |
| Angular momentum - Angle | ΔL · Δθ ≥ ℏ/2 |
| Number - Phase (photons) | ΔN · Δφ ≥ 1/2 |
General — for any non-commuting observables [A, B] ≠ 0, exact simultaneous knowledge impossible.
Numerical examples
| System | Δx | Min Δp | Min Δv |
|---|---|---|---|
| Electron in atom (~1 Å) | 10⁻¹⁰ m | 5.3 × 10⁻²⁵ kg·m/s | ~6 × 10⁵ m/s |
| Electron in nucleus (~10⁻¹⁵ m) | 10⁻¹⁵ m | 5.3 × 10⁻²⁰ kg·m/s | ~6 × 10¹⁰ m/s (relativistic!) |
| Bullet (1 cm precision) | 10⁻² m | 5.3 × 10⁻³³ kg·m/s | ~5.3 × 10⁻³¹ m/s (negligible) |
| Excited atom (10 ns lifetime) | — | — | ΔE ≥ 5.3 × 10⁻²⁶ J ≈ 3 × 10⁻⁷ eV (linewidth) |
JavaScript — uncertainty calculations
const h_bar = 1.055e-34;
// Position-momentum: minimum Δp for given Δx
function minMomentumUncertainty(deltaX) {
return h_bar / (2 * deltaX);
}
// Velocity uncertainty for particle of mass m
function minVelocityUncertainty(deltaX, mass) {
return minMomentumUncertainty(deltaX) / mass;
}
// Electron localized to atom (~1 Å)
const m_e = 9.11e-31;
console.log(`Electron in atom: Δv ≥ ${(minVelocityUncertainty(1e-10, m_e)).toExponential(2)} m/s`);
// ~5.8e5 m/s — comparable to actual orbital velocity
// Electron in nucleus
console.log(`Electron in nucleus: Δv ≥ ${(minVelocityUncertainty(1e-15, m_e)).toExponential(2)} m/s`);
// ~5.8e10 m/s — much greater than c! Means electron CAN'T be confined to nucleus
// Energy-time uncertainty
function minEnergyUncertainty(deltaT) {
return h_bar / (2 * deltaT); // J
}
const eV = 1.602e-19;
function minEnergyEv(deltaT) { return minEnergyUncertainty(deltaT) / eV; }
// Excited atom with 1 ns lifetime
console.log(`1 ns excited state: ΔE ≥ ${minEnergyEv(1e-9).toExponential(2)} eV`);
// ~3.3e-7 eV — natural linewidth
// Hydrogen 2p → 1s lifetime ~ 1.6 ns; gives Lyman-α natural linewidth
console.log(`H Lyman-α linewidth: ${minEnergyEv(1.6e-9).toExponential(2)} eV`);
// Macroscopic check: 1 kg ball localized to 1 mm
const m_ball = 1; // kg
console.log(`1 kg ball Δv: ${(minVelocityUncertainty(1e-3, m_ball)).toExponential(2)} m/s`);
// 5.3e-32 m/s — utterly negligible
// Compton wavelength: when uncertainty starts requiring relativity
function comptonWavelength(mass) {
return h_bar / (mass * 3e8);
}
console.log(`Electron Compton: ${(comptonWavelength(m_e) * 1e12).toFixed(2)} pm`);
// ~ 0.4 pm — at this scale, relativistic effects become important
// Confinement energy: minimum KE for particle in box
function confinementEnergy(L, mass) {
// From uncertainty: p ~ ℏ/L, KE ~ p²/(2m)
const p = h_bar / L;
return p * p / (2 * mass);
}
// Electron in 1 nm box
console.log(`Electron in 1 nm box: KE ~ ${(confinementEnergy(1e-9, m_e) / eV).toFixed(2)} eV`);
// Atomic radius from uncertainty + Coulomb
function bohrRadiusEstimate() {
// Confinement energy = Coulomb at atom radius
// ℏ²/(2m·a²) = ke²/a → a = ℏ²/(m·k·e²) ≈ 5.3 × 10⁻¹¹ m
return h_bar * h_bar / (m_e * 8.99e9 * 1.602e-19 * 1.602e-19);
}
console.log(`Bohr radius from uncertainty: ${(bohrRadiusEstimate() * 1e10).toFixed(2)} Å`);
Where uncertainty matters
- Atomic structure. Why electrons don't collapse to nucleus; sets atom size.
- Quantum tunneling. Energy-time uncertainty enables tunneling through barriers.
- Particle physics. Virtual particles (very short Δt → large ΔE allows them); particle widths.
- Atomic clocks. Linewidth limits precision; cool atoms to reduce velocity uncertainty.
- Heisenberg microscope thought experiment. Pedagogical aid for understanding measurement disturbance.
- Quantum cryptography. Eavesdropping disturbs states; can't be done without detection (BB84 protocol).
- Cosmology. Vacuum fluctuations from energy-time uncertainty; quantum origin of structure in Big Bang.
Common mistakes
- Treating it as measurement limitation. NO — it's intrinsic. Quantum states can't have arbitrarily precise x AND p simultaneously.
- Using ℏ instead of ℏ/2. Strict bound is ℏ/2 (Heisenberg's original was ~ℏ; Robertson tightened to ℏ/2).
- Confusing Δx with measurement error. Δx is standard deviation of position distribution — even if measured perfectly, the state has spread.
- Applying to macroscopic. ℏ so small that uncertainty is negligible at human scales.
- Misusing energy-time form. ΔE·Δt ≥ ℏ/2 has subtle interpretation — t isn't an observable but a "duration" parameter. Different from x-p which both have operators.
- Treating it as "nature is fuzzy." Quantum systems have well-defined states (with their own uncertainty). It's not vagueness, it's a precise mathematical structure.
Frequently asked questions
Why does uncertainty exist?
Quantum particles are described by wave functions Ψ(x). A localized wave (precise x) requires many frequency components (broad p spread). A pure-frequency wave (precise p) extends infinitely (broad x spread). Mathematical fact about Fourier transforms — applies to any wave-based description, including quantum matter waves. NOT a measurement issue.
How does Δx·Δp ≥ ℏ/2 keep electrons out of nuclei?
If electron were confined to nuclear size (~10⁻¹⁵ m), Δp ~ ℏ/(2·Δx) ~ 5 × 10⁻²⁰ kg·m/s. Kinetic energy: KE = p²/(2m) ~ 10⁻⁹ J = 10¹¹ eV — far more than nuclear binding energy. So electron can't be confined that tightly. Spreads to ~ atomic size (~10⁻¹⁰ m) where KE matches Coulomb attraction.
What's the energy-time uncertainty?
ΔE · Δt ≥ ℏ/2. Slightly different — t isn't an observable but a parameter. Means: short-lived states have energy uncertainty (e.g., excited atomic states have linewidth ΔE = ℏ/τ where τ is lifetime). Vacuum can have energy fluctuations at very short times (virtual particles). Underpins quantum field theory.
Is this just a measurement limitation?
NO. It's a fundamental property of quantum states. Even before measurement, x and p don't both have precise values simultaneously. The wave function literally CAN'T be a delta function in both x and p. This is the deepest quantum vs classical difference.
How is uncertainty important for tunneling?
A particle with energy E facing a barrier of height V > E classically can't pass. Quantum mechanically — wave function leaks through. Energy-time uncertainty allows particle to "borrow" energy ΔE for time Δt ≤ ℏ/(2·ΔE) — long enough to traverse the barrier. Tunneling rate exponentially depends on barrier and particle parameters.
Does uncertainty disappear at macroscopic scales?
ℏ is so small that for everyday objects, uncertainty is utterly negligible. A 1 kg object localized to 1 mm has Δp ≥ 5 × 10⁻³² kg·m/s = 5 × 10⁻³² m/s velocity uncertainty. Over billions of years, position uncertainty < mm. Macroscopically classical.
How is the principle stated mathematically?
Heisenberg-Robertson: σ_A · σ_B ≥ |⟨[A,B]⟩|/2 for any two observables A, B. For position and momentum: [x, p] = iℏ → σ_x·σ_p ≥ ℏ/2. For non-commuting observables, exact simultaneous knowledge impossible. Commuting observables (like x and y) can be measured simultaneously.