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de Broglie waves and uncertainty principle

Learning objectives

  • Outcome

    Calculate the de Broglie wavelength of a particle from its momentum or speed using λ=h/p\lambda = h/p.

  • Outcome

    Compare de Broglie wavelengths for an electron, a proton, and a macroscopic body, and explain why wave behaviour is observable only for microscopic particles.

  • Outcome

    Estimate the minimum momentum spread and minimum kinetic energy of a particle confined to a region of size Δx\Delta x using Δx Δp≥ℏ/2\Delta x\,\Delta p \ge \hbar/2.

  • Outcome

    Explain why the uncertainty relation is not an instrument error but a property of a quantum state.

Understand the idea

de Broglie Waves and the Uncertainty Principle

Text

Momentum pp is the central quantity: it is momentum, not speed or mass alone, that sets the wave behaviour of a particle. de Broglie postulated that a particle of momentum pp is described by a wave of wavelength

λ=hp,\lambda = \frac{h}{p},

where h=6.626×10−34h = 6.626\times10^{-34} J·s is the Planck constant. Because, by the impulse law Δp⃗=F⃗ Δt\Delta \vec p = \vec F\,\Delta t (from mechanics), a force changes the momentum vector, any interaction that changes the magnitude ∣p∣|p| also changes λ\lambda: accelerating a particle along its motion shortens its wave. A force perpendicular to the momentum changes only its direction, not ∣p∣|p|, so λ=h/∣p∣\lambda = h/|p| stays the same. For macroscopic bodies the momentum is large and λ\lambda is negligible (of order 10−3410^{-34} m), whereas an electron with v∼106v \sim 10^{6} m/s gives λ∼0.7\lambda \sim 0.7 nm — comparable to atomic spacings, so an electron beam diffracts from a crystal. The de Broglie wave is a probability-amplitude wave, not a vibration of a medium: its intensity at a point is proportional to the probability of finding the particle there. A quantum state cannot have a sharp position and a sharp momentum at the same time: Δx Δp≥ℏ/2\Delta x\,\Delta p \ge \hbar/2, where ℏ=h/2π\hbar = h/2\pi. This is not a measurement error but a property of the state itself: confining a particle to a region Δx\Delta x forces a non-zero spread of momenta, hence a non-zero kinetic energy — which is why atoms have a finite size and are stable.

Worked examples

Direct

Problem

An electron moves with speed v=1.0×106v = 1.0\times10^{6} m/s. The electron mass is me=9.11×10−31m_e = 9.11\times10^{-31} kg. Find the de Broglie wavelength of the electron.

Solution

Step 1. Momentum.

p=mev=(9.11×10−31)(1.0×106)=9.11×10−25 kg⋅m/s.p = m_e v = (9.11\times10^{-31})(1.0\times10^{6}) = 9.11\times10^{-25}\ \text{kg}\cdot\text{m/s}.

Step 2. Wavelength.

λ=hp=6.626×10−349.11×10−25=7.3×10−10 m.\lambda = \frac{h}{p} = \frac{6.626\times10^{-34}}{9.11\times10^{-25}} = 7.3\times10^{-10}\ \text{m}.

Step 3. Conclusion. λ≈0.73\lambda \approx 0.73 nm, comparable to the spacing between atoms in a crystal (about 0.20.2–0.50.5 nm), so such an electron beam produces an observable diffraction pattern.

Application

Problem

An electron is accelerated from rest through a potential difference U=100U = 100 V. Find its de Broglie wavelength and compare it with the interatomic spacing in a crystal (d≈0.2d \approx 0.2 nm). Electron charge e=1.60×10−19e = 1.60\times10^{-19} C, mass me=9.11×10−31m_e = 9.11\times10^{-31} kg.

Solution

Step 1. Kinetic energy. The field does work eUeU, all of it becoming kinetic energy:

K=eU=(1.60×10−19)(100)=1.60×10−17 J.K = eU = (1.60\times10^{-19})(100) = 1.60\times10^{-17}\ \text{J}.

Step 2. Momentum. Since K=p2/(2me)K = p^2/(2m_e), for a non-relativistic electron

p=2meK=2(9.11×10−31)(1.60×10−17)=5.4×10−24 kg⋅m/s.p = \sqrt{2m_e K} = \sqrt{2(9.11\times10^{-31})(1.60\times10^{-17})} = 5.4\times10^{-24}\ \text{kg}\cdot\text{m/s}.

Step 3. Wavelength.

λ=hp=6.626×10−345.4×10−24=1.2×10−10 m≈0.12 nm.\lambda = \frac{h}{p} = \frac{6.626\times10^{-34}}{5.4\times10^{-24}} = 1.2\times10^{-10}\ \text{m} \approx 0.12\ \text{nm}.

Step 4. Comparison. λ≈0.12\lambda \approx 0.12 nm and d≈0.2d \approx 0.2 nm are of the same order, so the diffraction condition is satisfied. This is the classic Davisson–Germer situation: the crystal acts as a diffraction grating for electrons.

Transfer

Problem

An electron is confined to a region of size Δx=0.10\Delta x = 0.10 nm (the order of an atomic size). Using the uncertainty relation Δx Δp≥ℏ/2\Delta x\,\Delta p \ge \hbar/2, estimate the minimum momentum spread and the minimum kinetic energy of the electron. Compare the result with the hydrogen ionization energy 13.613.6 eV.

Solution

Step 1. Momentum spread. With Δx=1.0×10−10\Delta x = 1.0\times10^{-10} m,

Δp≥ℏ2Δx=1.055×10−342(1.0×10−10)=5.3×10−25 kg⋅m/s.\Delta p \ge \frac{\hbar}{2\Delta x} = \frac{1.055\times10^{-34}}{2(1.0\times10^{-10})} = 5.3\times10^{-25}\ \text{kg}\cdot\text{m/s}.

Step 2. Energy estimate. Estimate pp by Δp\Delta p and substitute into the non-relativistic formula:

Kmin≈(Δp)22me=(5.3×10−25)22(9.11×10−31)=1.5×10−19 J.K_{min} \approx \frac{(\Delta p)^2}{2m_e} = \frac{(5.3\times10^{-25})^2}{2(9.11\times10^{-31})} = 1.5\times10^{-19}\ \text{J}.

Step 3. Convert to electron-volts.

Kmin=1.5×10−191.60×10−19≈0.95 eV≈1 eV.K_{min} = \frac{1.5\times10^{-19}}{1.60\times10^{-19}} \approx 0.95\ \text{eV} \approx 1\ \text{eV}.

Step 4. Comparison and meaning. This value is an order of magnitude below 13.613.6 eV but on the same scale as electron binding energies in atoms. So an electron cannot sit at rest inside an atom: confinement itself demands non-zero kinetic energy. The estimate is approximate — we replaced Δp\Delta p by a characteristic momentum and ignored the exact shape of the wave function — so expect an order of magnitude, not an exact number.

Practice

Text

Goal: see how λ=h/p\lambda = h/p spans dozens of orders of magnitude and how the uncertainty relation works.

Safety: calculations and an on-screen model only; no radiation sources or high voltage are needed. In particular, neither an electron source nor an accelerating voltage is required — all data come from the problem statement.

Part 1. Spreadsheet table. Create columns mm, vv, p=mvp = mv, λ=h/p\lambda = h/p. Fill in the rows:

  • electron, me=9.11×10−31m_e = 9.11\times10^{-31} kg, v=1.0×106v = 1.0\times10^{6} m/s;
  • the same electron at v=1.0×107v = 1.0\times10^{7} m/s (compare λ\lambda);
  • proton, mp=1.67×10−27m_p = 1.67\times10^{-27} kg, v=1.0×106v = 1.0\times10^{6} m/s;
  • baseball, m=0.145m = 0.145 kg, v=40v = 40 m/s.

Part 2. Graph. Plot lg⁡λ\lg\lambda against lg⁡p\lg p — from λ=h/p\lambda = h/p this should be a straight line of slope −1-1. Check that all four points fall on one line.

Part 3. Confinement. For Δx=1.0\Delta x = 1.0 nm, 0.100.10 nm, and 0.0100.010 nm, compute Δp≥ℏ/(2Δx)\Delta p \ge \hbar/(2\Delta x) and Kmin≈(Δp)2/(2me)K_{min} \approx (\Delta p)^2/(2m_e). Plot KminK_{min} versus Δx\Delta x and state the conclusion: the tighter the region, the larger the energy.

Part 4 (optional). Open an interactive quantum-wave interference model (for example, an electron double-slit simulation) and check that shrinking the de Broglie wavelength brings the fringes on the screen closer together.

Visual reference

Purpose

Show two ideas at once: (1) the de Broglie wavelength is inversely proportional to momentum and differs by many orders of magnitude between microscopic and macroscopic objects; (2) the more tightly a particle is localized, the wider its spread of momenta.

Representation

Two panels.

Left — a log–log graph: horizontal axis pp (from 10−2610^{-26} to 10110^{1} kg·m/s), vertical axis λ=h/p\lambda = h/p (from 10−3410^{-34} to 10−910^{-9} m). A straight line of slope −1-1 carries the marked points "electron at 10610^{6} m/s", "electron at 100100 eV", "proton", "baseball"; a horizontal dashed line at 0.20.2 nm is labelled "interatomic spacing d≈0.2d \approx 0.2 nm" — wave effects in a crystal are observable when λ≈d\lambda \approx d (for a first-order diffraction maximum λ≤2d\lambda \le 2d), not for every wavelength above that line. Points near the line (electron at 100100 eV: λ≈0.12\lambda \approx 0.12 nm) correspond to observable diffraction; the "baseball" point far below the line shows no observable wave effects.

Right — a sketch: a wave packet (several sine periods under a Gaussian envelope) of width Δx\Delta x; below it a horizontal double-headed arrow labelled "Δx\Delta x". Beside it a fan of momentum arrows: a narrow envelope gives a wide fan (large Δp\Delta p), a wide envelope gives a narrow fan; the caption reads Δx Δp≥ℏ/2\Delta x\,\Delta p \ge \hbar/2.

Real-world examples

A football in flight

Scenario

A football of mass m=0.43m = 0.43 kg leaves a boot at v=25v = 25 m/s, so its momentum is p=mv=0.43×25=10.8p = mv = 0.43 \times 25 = 10.8 kg·m/s. Its de Broglie wavelength is λ=h/p=6.63×10−34/10.8≈6×10−35\lambda = h/p = 6.63\times10^{-34}/10.8 \approx 6\times10^{-35} m. A proton is about 1.7×10−151.7\times10^{-15} m across, so the ball's matter wave is roughly 102010^{20} times shorter than a single proton.

Connection

This is the de Broglie relation λ=h/p\lambda = h/p in its simplest form: wavelength shrinks as momentum grows. Diffraction and interference appear only when λ\lambda is comparable to the size of the obstacle or slit; for the ball λ\lambda is 102010^{20} times smaller than any gap it could pass through, so its wave nature is unobservable and Newtonian mechanics is enough.

Electrons that see a virus: the electron microscope

Scenario

In an electron microscope an electron is accelerated through U=100U = 100 V and gains kinetic energy Ek=eU=100E_k = eU = 100 eV =1.60×10−17= 1.60\times10^{-17} J. From Ek=p2/2mE_k = p^2/2m its momentum is p=2meEk=2×9.11×10−31×1.60×10−17≈5.4×10−24p = \sqrt{2 m_e E_k} = \sqrt{2 \times 9.11\times10^{-31} \times 1.60\times10^{-17}} \approx 5.4\times10^{-24} kg·m/s, so λ=h/p≈6.63×10−34/5.4×10−24≈1.2×10−10\lambda = h/p \approx 6.63\times10^{-34}/5.4\times10^{-24} \approx 1.2\times10^{-10} m =0.12= 0.12 nm. That is exactly the spacing between atoms in a crystal, so a thin sample diffracts such a beam.

Connection

The de Broglie relation λ=h/p\lambda = h/p together with the kinetic-energy link Ek=p2/2mE_k = p^2/2m converts an accelerating voltage into a wavelength. The resolving power is set by that wavelength: a 0.120.12 nm wave reveals details finer than the roughly 550550 nm green light used in a light microscope.

Why electrons in a phone's chip do not fall into the nucleus

Scenario

In the silicon of a phone chip an electron is bound inside an atom about 1×10−101\times10^{-10} m across, so the uncertainty in its position is at most Δx≈1×10−10\Delta x \approx 1\times10^{-10} m. The uncertainty principle demands Δp≥ℏ/(2Δx)=1.055×10−34/(2×10−10)≈5.3×10−25\Delta p \ge \hbar/(2\Delta x) = 1.055\times10^{-34}/(2\times10^{-10}) \approx 5.3\times10^{-25} kg·m/s. Even the calmest electron allowed by that momentum carries kinetic energy Δp2/(2me)≈(5.3×10−25)2/(2×9.11×10−31)≈1.5×10−19\Delta p^2/(2m_e) \approx (5.3\times10^{-25})^2/(2\times9.11\times10^{-31}) \approx 1.5\times10^{-19} J ≈1\approx 1 eV.

Connection

This is the position–momentum form of the uncertainty principle Δx Δp≥ℏ/2\Delta x\,\Delta p \ge \hbar/2. Squeezing the electron into a smaller Δx\Delta x forces a larger Δp\Delta p and therefore more kinetic energy, so an electron cannot lie still on top of the nucleus. The resulting energy is of the same order as the few-electron-volt energies of chemical bonds, and the balance between this kinetic energy and the pull of the nucleus is what gives atoms their ∼1×10−10\sim1\times10^{-10} m size.