Intuition What this page is for
The parent note gave you the formula λ = h / p and three examples. Here we hunt down every kind of question an exam can build from that one formula: known speed, known kinetic energy, known voltage, a photon (the limiting case), a giant slow object, a tricky unit trap, and a "compare two particles" twist. If you can do all of these, no de Broglie question can surprise you.
Before anything, three constants we will reuse. Each is just a number with units — memorise the units, not the digits.
Definition The toolkit numbers
Planck's constant: h = 6.626 × 1 0 − 34 J s (joule-seconds — energy × time).
Electron mass: m e = 9.11 × 1 0 − 31 kg .
Charge on one electron: e = 1.602 × 1 0 − 19 C (also the value of 1 eV in joules).
Speed of light: c = 3.00 × 1 0 8 m/s (only for photons!).
Every de Broglie problem is one of these cells. The Formula to reach for column tells you which face of the master result to use.
#
Case class
What you're given
Formula to reach for
Example
A
Direct: speed known
m , v
λ = m v h
Ex 1
B
Kinetic energy known
m , K E
λ = 2 m K E h
Ex 2
C
Accelerating voltage
charge q , V
λ = 2 m q V h
Ex 3
D
Photon (limiting case, m 0 = 0 )
wavelength or energy
λ = p h = E h c
Ex 4
E
Degenerate: macroscopic / slow
big m , ordinary v
λ = m v h (see it vanish)
Ex 5
F
Unit trap (eV, kV, grams)
mixed units
convert first, then B or C
Ex 6
G
Comparison / ratio twist
two particles' m , K E
take ratio λ 2 λ 1
Ex 7
H
Real-world word problem
thermal / everyday
pick the right cell
Ex 8
We cover A–H below, each labelled with its cell.
The picture above is the whole page in one glance: as momentum p climbs (heavier or faster), the wavelength λ falls along that curve. Every example is just a dot on this curve . Watch where each lands.
Worked example Ex 1 — Cell A (direct, speed known)
A proton moves at v = 3.0 × 1 0 5 m/s . Mass m p = 1.67 × 1 0 − 27 kg . Find λ .
Forecast: A proton is ~1800× heavier than an electron but slower here than the parent's electron. Guess: will λ be bigger or smaller than the electron's 0.73 nm? (Bigger m v ⇒ smaller λ , so guess smaller.)
Compute momentum p = m p v = ( 1.67 × 1 0 − 27 ) ( 3.0 × 1 0 5 ) .
Why this step? λ depends only on p ; get that single number first.
p = 5.01 × 1 0 − 22 kg m/s
Divide h by p .
Why this step? That is the de Broglie relation — nothing else needed.
λ = 5.01 × 1 0 − 22 6.626 × 1 0 − 34 = 1.32 × 1 0 − 12 m
Verify: Units: kg m/s J s = kg m/s kg m 2 /s = m ✓. And indeed 1.3 pm ≪ 0.73 nm — smaller, as forecast, because m v is larger.
Worked example Ex 2 — Cell B (kinetic energy known)
An electron has kinetic energy K E = 50 eV . Find its de Broglie wavelength.
Forecast: 50 eV is a modest energy. Will λ land near the atomic (~0.1 nm) scale? Guess yes.
Convert energy to joules: 50 eV × 1.602 × 1 0 − 19 = 8.01 × 1 0 − 18 J .
Why this step? The formula uses SI joules; eV is a disguise for joules.
We don't know v directly, so use the KE form. Why this form? Because p = 2 m K E lets us skip solving for v .
λ = 2 m e K E h
Compute the denominator: 2 ( 9.11 × 1 0 − 31 ) ( 8.01 × 1 0 − 18 ) = 1.459 × 1 0 − 47 = 3.82 × 1 0 − 24 .
Why this step? This is p in kg m/s.
Divide: λ = 3.82 × 1 0 − 24 6.626 × 1 0 − 34 = 1.73 × 1 0 − 10 m = 0.173 nm .
Verify: Cross-check with the voltage shortcut. 50 eV means an electron dropped through 50 V , so λ ≈ 50 1.226 = 0.173 nm ✓ — the two roads meet.
Worked example Ex 3 — Cell C (accelerating voltage)
An electron is accelerated from rest through V = 400 V . Find λ .
Forecast: Higher voltage than Ex 2's implicit 50 V ⇒ faster electron ⇒ shorter λ . Guess below 0.1 nm.
Energy gained: K E = q V = e V . Why this step? A charge q crossing a potential drop V gains exactly q V of kinetic energy (work-energy theorem).
Use the shortcut derived in the parent: λ ( nm ) = V 1.226 .
Why this step? It already bundles h , m e , e so we only feed in volts.
λ = 400 1.226 = 20 1.226 = 0.0613 nm
Verify: Full form: λ = 2 m e e V h = 2 ( 9.11 × 1 0 − 31 ) ( 1.602 × 1 0 − 19 ) ( 400 ) 6.626 × 1 0 − 34 . Denominator = 1.168 × 1 0 − 46 = 1.081 × 1 0 − 23 , so λ = 6.13 × 1 0 − 11 m = 0.0613 nm ✓. Shorter than Ex 2, as forecast.
Worked example Ex 4 — Cell D (photon: the limiting case)
Green light has wavelength 500 nm . (a) What is the photon's momentum? (b) Confirm λ = h / p still holds.
Forecast: A photon is the origin of the formula. So λ = h / p must hold exactly — it's not an approximation for light.
For a photon, p = λ h — just the master formula rearranged. Why this step? Photons are the one case where the formula was proved , not postulated.
p = 500 × 1 0 − 9 6.626 × 1 0 − 34 = 1.325 × 1 0 − 27 kg m/s
Now feed that p back: λ = h / p = 500 nm .
Why this step? Sanity loop — going forward and backward must return the input.
Verify: Photon energy E = p c = ( 1.325 × 1 0 − 27 ) ( 3.0 × 1 0 8 ) = 3.98 × 1 0 − 19 J = 2.48 eV , the familiar energy of green light ✓. Note: here we used c , not v — because a photon is the massless particle that travels at c . This is the exact case where the "use v not c " mistake does not apply.
Worked example Ex 5 — Cell E (degenerate / macroscopic)
A person of mass 60 kg walks at 1.5 m/s . Find λ and explain why nobody diffracts through doorways.
Forecast: Huge mass, ordinary speed. Guess a laughably tiny wavelength — far below anything physical.
Momentum p = m v = 60 × 1.5 = 90 kg m/s .
Why this step? Get p before dividing.
λ = 90 6.626 × 1 0 − 34 = 7.36 × 1 0 − 36 m .
Why this step? Direct Cell A formula — but watch the exponent.
Verify: A proton's diameter is ~1 0 − 15 m . Our λ is ∼ 1 0 − 21 times smaller than a proton . No doorway (or anything) is that narrow, so no diffraction ever occurs — the wave nature is real but utterly unobservable. This is the general truth for any macroscopic object: the mass in the denominator crushes λ to nothing.
Worked example Ex 6 — Cell F (unit trap)
A 2.0 g bullet moves at 500 m/s , and separately an electron has K E = 1.5 keV . Two traps at once. Find both wavelengths.
Forecast: Both traps are about not plugging in raw numbers. Guess: bullet gives a Cell-E-tiny λ ; electron gives a sub-atomic λ .
Bullet: convert grams to kilograms first — 2.0 g = 2.0 × 1 0 − 3 kg .
Why this step? SI demands kilograms; grams would inflate λ by 1000×.
p = ( 2.0 × 1 0 − 3 ) ( 500 ) = 1.0 kg m/s , λ = 1.0 6.626 × 1 0 − 34 = 6.63 × 1 0 − 34 m
Electron: convert 1.5 keV = 1500 eV = 1500 × 1.602 × 1 0 − 19 = 2.403 × 1 0 − 16 J .
Why this step? "k" means ×1000, then eV→J. Two conversions stacked — the classic trap.
λ = 2 m e K E h = 2 ( 9.11 × 1 0 − 31 ) ( 2.403 × 1 0 − 16 ) 6.626 × 1 0 − 34 .
Denominator = 4.378 × 1 0 − 46 = 2.092 × 1 0 − 23 , so λ = 3.17 × 1 0 − 11 m = 0.0317 nm .
Verify: Voltage check for the electron: 1500 V ⇒ λ ≈ 1500 1.226 = 0.0317 nm ✓. Bullet λ is macroscopic-tiny as forecast.
Worked example Ex 7 — Cell G (comparison / ratio twist)
A proton and an electron are accelerated through the same voltage V . Which has the longer wavelength, and by what factor? (m p / m e = 1836 .)
Forecast: Same charge magnitude, same V , so same K E . Lighter particle ⇒ smaller p ⇒ longer λ . Guess the electron wins.
Both gain K E = q V with the same q (charge magnitude e ) and same V . Why this step? Equal K E is the whole trick — it makes the ratio clean.
λ = 2 m K E h , so with K E equal, λ ∝ m 1 .
Why this step? Everything except m cancels in the ratio.
λ p λ e = m e m p = 1836 = 42.8
Verify: The electron's wavelength is ~42.8 × longer than the proton's ✓. Sanity: lighter ⇒ longer, matches the forecast and the parent's "mass in the denominator" rule. Notice the exam-style beauty: no numbers for h , V , or q were needed — the ratio killed them all.
Worked example Ex 8 — Cell H (real-world word problem)
"Thermal" neutrons at room temperature (T = 300 K ) are used in materials research. Their average kinetic energy is K E = 2 3 k B T with k B = 1.38 × 1 0 − 23 J/K . Neutron mass m n = 1.675 × 1 0 − 27 kg . Find λ — and explain why neutrons "see" crystals.
Forecast: Neutrons are heavy but very slow (thermal). Guess λ lands near atomic spacing (~0.1 nm), which is why they're used for crystal studies.
Kinetic energy: K E = 2 3 ( 1.38 × 1 0 − 23 ) ( 300 ) = 6.21 × 1 0 − 21 J .
Why this step? The word "thermal at temperature T " is code for this energy — recognise the phrase.
Use Cell B (we have m and K E , not v ):
λ = 2 m n K E h = 2 ( 1.675 × 1 0 − 27 ) ( 6.21 × 1 0 − 21 ) 6.626 × 1 0 − 34
Denominator = 2.080 × 1 0 − 47 = 4.560 × 1 0 − 24 .
λ = 4.560 × 1 0 − 24 6.626 × 1 0 − 34 = 1.45 × 1 0 − 10 m = 0.145 nm .
Verify: Crystal atomic spacings are ~0.1 –0.3 nm. Our λ = 0.145 nm sits right in that window ✓ — so thermal neutrons diffract off crystals just like the electrons in the Davisson–Germer Experiment . Real, useful, forecast confirmed.
Recall Which formula for which cell?
Given speed ::: use λ = h / m v (Cell A).
Given kinetic energy ::: use λ = h / 2 m K E (Cell B).
Given accelerating voltage V for a charge q ::: use λ = h / 2 m q V , or 1.226/ V nm for electrons (Cell C).
A photon ::: use λ = h / p = h c / E and speed c , never v (Cell D).
Two particles, same voltage ::: λ ∝ 1/ m , take the ratio (Cell G).
"Thermal at temperature T " ::: means K E = 2 3 k B T , then Cell B (Cell H).
Mnemonic The three-question triage
"Speed? Energy? Volts?" — ask these in order. Speed ⇒ h / m v . Energy ⇒ h / 2 m K E . Volts ⇒ h / 2 m q V . Everything else (grams, keV, thermal) is just a conversion before one of these three doors.