de Broglie Wavelength — Worked Problems

de Broglie Wavelength — Worked Problems

7 min read

The Core Idea

In 1924, Louis de Broglie proposed that every moving particle behaves like a wave with wavelength λ=h/p\lambda = h/p, where pp is the particle’s momentum and hh is Planck’s constant. This wave-particle duality unified the dual nature of light (photons) with matter (electrons, neutrons, atoms). It directly led to Schrödinger’s wave equation and the entire framework of quantum mechanics.

For Class 12 boards, JEE Main, and NEET, the de Broglie wavelength shows up in problems about electrons accelerated through potential differences, neutrons of given kinetic energy, and protons in particle accelerators. The math is short — a single formula plus careful unit handling. The conceptual subtlety lies in connecting kinetic energy, momentum, and accelerating voltage.

We’ll walk through the derivations once, drill three standard problem types, and flag the unit traps that catch students out.

Key Terms & Definitions

de Broglie wavelength: The wavelength associated with the matter wave of a particle of momentum pp:

λ=hp\lambda = \frac{h}{p}

where h=6.626×1034h = 6.626 \times 10^{-34} J s.

Momentum-Energy Relation (non-relativistic): For kinetic energy KK and mass mm:

p=2mKp = \sqrt{2 m K}

So the de Broglie wavelength becomes:

λ=h2mK\lambda = \frac{h}{\sqrt{2 m K}}

Accelerating Potential: When a charged particle of charge qq is accelerated through a potential difference VV, it gains kinetic energy K=qVK = qV. So p=2mqVp = \sqrt{2 m q V} and:

λ=h2mqV\lambda = \frac{h}{\sqrt{2 m q V}}

For an electron specifically, this simplifies to a memorable formula:

λ (in A˚)=150V\lambda \text{ (in Å)} = \sqrt{\frac{150}{V}}

when VV is in volts. So V=150V = 150 V gives λ=1\lambda = 1 Å.

Methods & Concepts

Three Standard Problem Setups

Type 1: Given speed. Use p=mvp = m v directly, then λ=h/(mv)\lambda = h/(mv). Straightforward.

Type 2: Given kinetic energy. Compute p=2mKp = \sqrt{2mK}, then λ=h/p\lambda = h/p. Watch units — convert KK to joules if you’re using hh in SI.

Type 3: Given accelerating potential. Use K=qVK = qV, then proceed as Type 2. For electrons, the 150/V\sqrt{150/V} shortcut saves time.

λ=hp=hmv=h2mK=h2mqV\lambda = \frac{h}{p} = \frac{h}{m v} = \frac{h}{\sqrt{2 m K}} = \frac{h}{\sqrt{2 m q V}}

For electrons accelerated through VV volts: λ150/V\lambda \approx \sqrt{150/V} Å.

Why the Wavelength is So Small for Macroscopic Objects

Plug in a 11 kg ball moving at 11 m/s: λ=h/p=6.6×1034\lambda = h/p = 6.6 \times 10^{-34} m. That’s 101910^{19} times smaller than the radius of an atomic nucleus. The wave nature is utterly undetectable — that’s why classical mechanics works for everyday objects.

For an electron at 10610^6 m/s: λ=7.3×1010\lambda = 7.3 \times 10^{-10} m, comparable to atomic spacing. That’s why electron diffraction works and why electrons in atoms must be treated as waves.

Solved Examples

Easy (CBSE)

Find the de Broglie wavelength of an electron moving at v=106v = 10^6 m/s. (me=9.1×1031m_e = 9.1 \times 10^{-31} kg.)

λ=6.63×10349.1×1031×106=6.63×10349.1×10257.28×1010 m\lambda = \frac{6.63 \times 10^{-34}}{9.1 \times 10^{-31} \times 10^6} = \frac{6.63 \times 10^{-34}}{9.1 \times 10^{-25}} \approx 7.28 \times 10^{-10} \text{ m}

That’s 7.287.28 Å, comparable to atomic dimensions.

Medium (JEE Main)

An electron is accelerated from rest through a potential difference of 100100 V. Find its de Broglie wavelength.

Use the shortcut: λ=150/V\lambda = \sqrt{150/V} Å =1.51.225= \sqrt{1.5} \approx 1.225 Å.

Or the long way: K=qV=1.6×1019×100=1.6×1017K = qV = 1.6 \times 10^{-19} \times 100 = 1.6 \times 10^{-17} J. Then p=2mK=2×9.1×1031×1.6×10175.4×1024p = \sqrt{2 m K} = \sqrt{2 \times 9.1 \times 10^{-31} \times 1.6 \times 10^{-17}} \approx 5.4 \times 10^{-24} kg m/s. So λ=h/p1.23×1010\lambda = h/p \approx 1.23 \times 10^{-10} m =1.23= 1.23 Å. Same answer.

Hard (JEE Advanced)

A proton and an alpha particle are accelerated through the same potential difference VV. Find the ratio of their de Broglie wavelengths.

For both, λ=h/2mqV\lambda = h/\sqrt{2 m q V}. So λ1/mq\lambda \propto 1/\sqrt{m q}. For proton: mpm_p, q=eq = e. For alpha: mα=4mpm_\alpha = 4 m_p, q=2eq = 2e. So mαqα=8mpem_\alpha q_\alpha = 8 m_p e.

λpλα=mαqαmpqp=8=22\frac{\lambda_p}{\lambda_\alpha} = \sqrt{\frac{m_\alpha q_\alpha}{m_p q_p}} = \sqrt{8} = 2\sqrt{2}

The proton’s wavelength is 222.832\sqrt{2} \approx 2.83 times larger.

Exam-Specific Tips

For JEE Main: The shortcut λ=150/V\lambda = \sqrt{150/V} Å for electrons saves you 30 seconds per problem. Memorise it and recognise when to apply it.

For NEET: Often combined with the photoelectric effect. A typical problem: “Light of wavelength λp\lambda_p ejects electrons with KE KK. Find their de Broglie wavelength λe\lambda_e.” You’ll need to compute K=hc/λpϕK = h c/\lambda_p - \phi, then λe=h/2mK\lambda_e = h/\sqrt{2 m K}.

For CBSE Boards: Derivation of the relation λ=h/2mqV\lambda = h/\sqrt{2 m q V} is a 3-mark question. Practice the algebra cleanly.

Common Mistakes to Avoid

Mistake 1: Using p=mvp = mv even when speeds approach cc. For relativistic particles (high-energy electrons in accelerators), use p=γmvp = \gamma m v or p=E2/c2m2c2p = \sqrt{E^2/c^2 - m^2 c^2} instead. JEE rarely asks this, but flag it.

Mistake 2: Confusing wavelength of the photon (λ=hc/E\lambda = hc/E) with the de Broglie wavelength of a particle (λ=h/p\lambda = h/p). Photons are massless — different formula.

Mistake 3: Forgetting to convert eV to joules when using hh in SI. 11 eV =1.6×1019= 1.6 \times 10^{-19} J.

Mistake 4: Plugging VV into 150/V\sqrt{150/V} in non-volts (e.g., kV without conversion). The formula needs VV in volts and gives λ\lambda in angstroms.

Mistake 5: Treating mq\sqrt{m q} wrong for an alpha particle. Alpha is doubly charged (q=2eq = 2e) and four times heavier (m=4mpm = 4m_p). Both factors enter.

Practice Questions

Q1. An electron has kinetic energy 5050 eV. Find its de Broglie wavelength.

λ=150/50\lambda = \sqrt{150/50} Å =31.73= \sqrt{3} \approx 1.73 Å.

Q2. A neutron has kinetic energy 0.0250.025 eV (thermal energy at room temperature). Find λ\lambda. (mn1.67×1027m_n \approx 1.67 \times 10^{-27} kg.)

K=4×1021K = 4 \times 10^{-21} J, p=2mK1.16×1024p = \sqrt{2 m K} \approx 1.16 \times 10^{-24} kg m/s, λ1.79\lambda \approx 1.79 Å. Comparable to atomic spacing — that’s why thermal neutrons are used in crystallography.

Q3. Two electrons have de Broglie wavelengths in ratio 2:12:1. What’s the ratio of their kinetic energies?

λ1/K\lambda \propto 1/\sqrt{K}, so K1/λ2K \propto 1/\lambda^2. Ratio is 1:41:4.

Q4. A proton accelerated through V=1000V = 1000 V. Find its de Broglie wavelength.

λ=h/2mqV\lambda = h/\sqrt{2 m q V}. For proton, m=1.67×1027m = 1.67 \times 10^{-27} kg, q=eq = e. λ9.06×1013\lambda \approx 9.06 \times 10^{-13} m =9.06×103= 9.06 \times 10^{-3} Å. Much smaller than electron’s at same voltage — because proton is much heavier.

Q5. A photon and an electron have the same wavelength. Compare their momenta.

Both satisfy p=h/λp = h/\lambda. So momenta are equal — even though their energies are vastly different.

FAQs

Why don’t we see matter waves for cricket balls? The wavelength is so small (1034\sim 10^{-34} m) that no detector can resolve it. Wave behaviour is completely masked by classical motion.

Is the de Broglie wavelength a real wave? It’s a probability amplitude wave — the modulus squared gives the probability density of finding the particle. It’s not a vibration in a medium.

How was de Broglie’s hypothesis verified? By Davisson-Germer in 1927, who observed electron diffraction off a nickel crystal. The diffraction pattern matched the predicted wavelength exactly.

Does the de Broglie wavelength change in different reference frames? Yes — momentum is frame-dependent, so λ\lambda is too. But the formula λ=h/p\lambda = h/p holds in any frame.

Why is hh so small? It’s a fundamental constant of nature, 1034\sim 10^{-34} J s. If hh were larger, quantum effects would be visible at human scales — and the world would look very strange.