Intuition What this page is for
The parent note gave you the tool λ = h / p . But a formula is only as good as your ability to spot which version to use in each situation. This page hunts down every kind of problem the topic can throw at you — tiny particles, huge baseballs, "speed given," "voltage given," "energy given," "temperature given," even the edge cases where the naive formula breaks — and solves one of each, slowly.
By the end you will never meet a de Broglie question whose type you haven't already seen.
Before anything, let us pin down every symbol we will lean on, so nothing sneaks in undefined.
Definition The cast of symbols
λ (Greek "lambda") — the wavelength : the length of one full ripple of the matter wave, measured in metres. Picture the distance from one wave-crest to the next.
p — momentum : "how much motion" a thing carries. For slow objects p = m v (mass times velocity). Units: kg⋅m/s .
m — mass in kilograms; v — speed in metres per second.
K — kinetic energy , the energy of motion , in joules (J).
E — total energy carried by a particle, also in joules (J). For a photon (light particle) all of its energy is this E ; there is no separate "rest" part because it has no mass. We meet E in the photon example (Cell H).
c = 3 × 1 0 8 m/s — the speed of light in a vacuum, the fixed top speed of the universe. It appears whenever light or relativity enters (Cells H and I).
h = 6.626 × 1 0 − 34 J⋅s — Planck's constant , the fixed number that scales the whole quantum world.
q or e — electric charge ; for an electron e = 1.6 × 1 0 − 19 C (coulombs).
V — accelerating voltage in volts.
γ (Greek "gamma") — the relativistic factor γ = 1/ 1 − v 2 / c 2 , always ≥ 1 ; it measures how much fast motion (near c ) inflates momentum. Built in Cell I.
1 A ˚ ("angstrom") = 1 0 − 10 m — a handy tiny ruler, roughly the size of an atom.
We will use exactly four "faces" of the same one formula. Which face you pick depends on what the problem hands you .
Every de Broglie problem falls into one of these cells. The rest of the page fills each one.
Cell
What's given
Which face
Watch out for
Example
A
mass + speed, small particle
h / m v
keep SI units
Ex 1
B
mass + speed, macroscopic object
h / m v
answer absurdly tiny — that's correct
Ex 2
C
electron + voltage V
12.27/ V Å
this shortcut is electrons only
Ex 3
D
kinetic energy K (any particle)
h / 2 m K
never use h / m v if you only know K
Ex 4
E
temperature T (thermal particle)
K = 2 3 k B T then face D
K is average , not exact
Ex 5
F
ratio / comparison, same K
λ ∝ 1/ m
which quantity is held fixed?
Ex 6
G
ratio / comparison, same v
λ ∝ 1/ m
different from cell F!
Ex 7
H
photon (massless) — degenerate case
λ = h / p , p = E / c
h / m v is forbidden (m = 0 )
Ex 8
I
relativistic (speed near light) — limiting case
p = γ m v
h / m v fails , must correct
Ex 9
J
exam twist: λ given, find V or K
invert a face
algebra runs backward
Ex 10
The two "danger cells" are H (mass is zero, so the h / m v face literally divides by zero) and I (speed so high that p = m v ). We will look those two straight in the eye.
Worked example Ex 1 · An electron moving at
2 × 1 0 6 m/s
Find its de Broglie wavelength. Electron mass m e = 9.11 × 1 0 − 31 kg .
Forecast: electrons are famously "wavy." Guess: will λ come out around an atom's size (∼ 1 A ˚ = 1 0 − 10 m ), or vanishingly small? Hold your guess.
Compute momentum p = m e v = ( 9.11 × 1 0 − 31 ) ( 2 × 1 0 6 ) = 1.822 × 1 0 − 24 kg⋅m/s .
Why this step? We know mass and speed, and the speed is small compared to light, so cell A's face h / m v applies — and its heart is p = m v .
Divide λ = p h = 1.822 × 1 0 − 24 6.626 × 1 0 − 34 = 3.64 × 1 0 − 10 m .
Why this step? This is λ = h / p itself — the master face.
In angstroms: 3.64 × 1 0 − 10 m = 3.64 A ˚ .
Verify: units check — kg⋅m/s J⋅s = kg⋅m/s kg⋅m 2 / s 2 ⋅ s = m . ✓ And 3.6 A ˚ is a few atom-widths — exactly the "wavy on the atomic scale" our forecast hoped for. ✓
0.05 kg golf ball at 30 m/s
Find λ .
Forecast: same formula as Ex 1 — but the mass is ∼ 1 0 29 times bigger. Guess the order of magnitude of λ before computing.
Momentum p = m v = ( 0.05 ) ( 30 ) = 1.5 kg⋅m/s .
Why this step? Slow, heavy object → cell B, still p = m v .
Wavelength λ = 1.5 6.626 × 1 0 − 34 = 4.42 × 1 0 − 34 m .
Why this step? Master face again.
Verify: 1 0 − 34 m is about 1 0 24 times smaller than an atomic nucleus. No slit or object in the universe is that small, so no diffraction is ever observable — the golf ball is "purely classical." This is why wave nature hides for big things: large p forces a microscopic λ . ✓ (Compare parent note's cricket-ball result ∼ 1 0 − 34 m — same regime. ✓)
Intuition Why voltage even gives a wavelength
An electron sitting still is put in an electric field created by a voltage V . The field pushes it, doing work q V on it. All that work becomes kinetic energy: K = q V . So "give me a voltage" secretly means "give me a kinetic energy" — and kinetic energy gives momentum gives λ . The 12.27/ V shortcut just bundles all those steps for the electron once and for all.
Worked example Ex 3 · Electron through
V = 54 V (the Davisson–Germer value!)
Find λ . This is the actual voltage used in the Davisson–Germer experiment .
Forecast: the parent note's 100 V electron gave 1.23 A ˚ . We're using a smaller voltage, so expect a larger λ . Guess a number above 1.23 A ˚ .
Apply the electron shortcut λ = V 12.27 A ˚ = 54 12.27 A ˚ .
Why this step? Cell C, and the particle is specifically an electron, so the ready-made constant 12.27 is legal.
54 = 7.35 , so λ = 7.35 12.27 = 1.67 A ˚ .
Verify: 1.67 > 1.23 A ˚ — larger, as forecast (lower voltage ⇒ less momentum ⇒ longer wave). ✓ And 1.67 A ˚ matches the nickel crystal spacing that produced the famous diffraction peak. ✓
Common mistake The trap this cell exists to prevent
Why it feels right: "I know K , I'll find v from K = 2 1 m v 2 , then use h / m v ." The trap: that's two extra steps where you can slip. Fix: go straight through p = 2 m K — because p 2 = m 2 v 2 = 2 m ( 2 1 m v 2 ) = 2 m K . One clean route.
Worked example Ex 4 · A proton with
K = 1.0 MeV
Find λ . Proton mass m p = 1.673 × 1 0 − 27 kg ; 1 MeV = 1.6 × 1 0 − 13 J .
Forecast: protons are ~1836× heavier than electrons, so at a given energy they carry more momentum and should be less wavy than an electron. Expect λ well below 1 A ˚ .
Convert energy K = 1.0 MeV = 1.6 × 1 0 − 13 J .
Why this step? The formula demands joules; MeV is just a nickname.
Momentum p = 2 m p K = 2 ( 1.673 × 1 0 − 27 ) ( 1.6 × 1 0 − 13 ) .
Inside: 2 ( 1.673 × 1 0 − 27 ) ( 1.6 × 1 0 − 13 ) = 5.35 × 1 0 − 40 , so p = 5.35 × 1 0 − 40 = 2.31 × 1 0 − 20 kg⋅m/s .
Why this step? Cell D's face — energy in, momentum out, no detour through v .
Wavelength λ = 2.31 × 1 0 − 20 6.626 × 1 0 − 34 = 2.87 × 1 0 − 14 m .
Verify: 2.87 × 1 0 − 14 m = 2.87 × 1 0 − 4 A ˚ — thousands of times smaller than an atom, as forecast for a heavy, energetic proton. ✓ Is 1 MeV ≪ m p c 2 ≈ 938 MeV ? Yes, so the non-relativistic 2 m K is valid here (contrast cell I). ✓
Intuition Temperature is disguised kinetic energy
A gas at temperature T is a swarm of particles jiggling. Their average kinetic energy is K = 2 3 k B T , where k B = 1.38 × 1 0 − 23 J/K is Boltzmann's constant — the conversion rate between "degrees" and "joules of jiggle." So a temperature problem is a cell-D problem wearing a costume.
Worked example Ex 5 · A thermal neutron at
T = 300 K (room temperature)
Find λ . Neutron mass m n = 1.675 × 1 0 − 27 kg .
Forecast: neutron diffraction is a real lab technique, which only works if λ ≈ crystal spacing ≈ 1 A ˚ . So we expect an answer near 1 A ˚ .
Average KE K = 2 3 k B T = 1.5 ( 1.38 × 1 0 − 23 ) ( 300 ) = 6.21 × 1 0 − 21 J .
Why this step? Convert the temperature into the kinetic energy the formula wants.
Momentum p = 2 m n K = 2 ( 1.675 × 1 0 − 27 ) ( 6.21 × 1 0 − 21 ) .
Inside: 2.08 × 1 0 − 47 , so p = 4.56 × 1 0 − 24 kg⋅m/s .
Why this step? Now it's exactly cell D.
Wavelength λ = 4.56 × 1 0 − 24 6.626 × 1 0 − 34 = 1.45 × 1 0 − 10 m = 1.45 A ˚ .
Verify: ≈ 1.5 A ˚ — right at atomic-spacing scale, exactly why neutron diffraction is done at room temperature. ✓ Matches parent note's ≈ 1.4 A ˚ (rounding). ✓
The single most common exam trap: is the energy the same, or the speed the same? The proportionality flips.
Worked example Figure — reading the two panels
The blueprint figure above draws the actual wave-ripples of an electron (cyan) and a proton (amber), stacked so you can compare crest-to-crest spacing directly.
Left panel ("Same kinetic energy K "): both particles carry equal energy. The electron's cyan wave is drawn with a clearly longer crest-to-crest distance than the proton's amber wave. The double-headed white arrows mark one full wavelength of each — the electron's arrow is far wider. This visualizes λ ∝ 1/ m : since m p / m e = 1836 ≈ 42.8 , the electron's ripple is about 43× longer.
Right panel ("Same speed v "): now the speed is locked instead. The proton's amber wave is squeezed even tighter than in the left panel, because here λ ∝ 1/ m (no square root), giving a factor of 1836 . The electron's cyan wave is unchanged, so the gap between the two waves is dramatically bigger.
The takeaway you should read off the picture: the electron is wavier in both cases, but how much wavier depends entirely on what is held fixed — the right panel's gap is far larger than the left's. That difference is the whole lesson of Cells F and G.
Worked example Ex 6 · (Cell F) Electron vs proton at the
same kinetic energy K
Which is wavier, and by what factor?
Forecast: same K — the light one moves faster but which wins in momentum? Guess before reading.
Hold K fixed in λ = 2 m K h . Only m changes, so λ ∝ m 1 .
Why this step? With h , K constant, they're just constants; the mass is the only mover.
Take the ratio λ p λ e = m e m p = 1836 = 42.8 .
Why this step? Dividing kills every common constant, leaving a pure mass ratio.
Verify: the electron's wave is ≈ 43 × longer — the light particle is wavier at equal energy. Matches the left panel of the figure. ✓
Worked example Ex 7 · (Cell G) Electron vs proton at the
same speed v
Which is wavier, and by what factor?
Forecast: now the speed is locked, not the energy. Does the answer change? (Yes — that's the whole point.)
Hold v fixed in λ = m v h . Now λ ∝ m 1 (no square root!).
Why this step? With v constant, momentum m v scales linearly with mass.
Ratio λ p λ e = m e m p = 1836 .
Why this step? Linear this time, so the full mass ratio survives.
Verify: at equal speed the electron is 1836 × wavier — vastly more than the 43 × of Ex 6. Same two particles, different held-fixed quantity, different answer. The right panel of the figure shows this steeper gap. Always ask what is held constant. ✓
h / m v is illegal here
A photon has m = 0 . Plugging into λ = h / ( m v ) gives h /0 — division by zero, meaningless. The only valid face is the master one λ = h / p , with the photon's momentum p = E / c (from relativity, E = p c for a massless particle, where E is its total energy and c the speed of light). This is exactly the case the parent note built the whole hypothesis from.
Worked example Ex 8 · A photon of energy
E = 2.0 eV (visible light)
Find its wavelength. 1 eV = 1.6 × 1 0 − 19 J ; c = 3 × 1 0 8 m/s .
Forecast: 2 eV is roughly red-orange light, so expect λ around 600 nm = 6000 A ˚ — enormously bigger than any matter wave above, because photons carry so little momentum.
Energy in joules E = 2.0 ( 1.6 × 1 0 − 19 ) = 3.2 × 1 0 − 19 J .
Photon momentum p = c E = 3 × 1 0 8 3.2 × 1 0 − 19 = 1.067 × 1 0 − 27 kg⋅m/s .
Why this step? m = 0 blocks the mass face; p = E / c is the photon's proper momentum.
Wavelength λ = p h = 1.067 × 1 0 − 27 6.626 × 1 0 − 34 = 6.21 × 1 0 − 7 m = 621 nm .
Verify: 621 nm is orange visible light — exactly what 2 eV photons are. ✓ And it dwarfs every matter wavelength above, because tiny p ⇒ long λ . The mass face would have crashed; the momentum face sailed through. ✓
Intuition When "close to light speed" breaks the easy formula
p = m v is only the slow-speed approximation . As speed v climbs toward c (the speed of light, 3 × 1 0 8 m/s ), the true momentum is p = γ m v , where the relativistic factor γ = 1 − v 2 / c 2 1 is always ≥ 1 and blows up as v → c . Picture γ as a "stretch dial": at everyday speeds v / c ≈ 0 so γ ≈ 1 and nothing changes; near light speed v 2 / c 2 nearly equals 1 , the square root nears zero, and γ shoots up — inflating p . Ignoring γ makes p too small and therefore λ too large . Use the naive h / m v only when K ≪ m c 2 .
Worked example Ex 9 · An electron at
v = 0.9 c
Find λ , and compare with the wrong (naive) answer. Electron mass m e = 9.11 × 1 0 − 31 kg .
Forecast: the naive h / m v under estimates p (it drops the γ stretch), so it over estimates λ . The correct λ should therefore be shorter than the naive one — by roughly the factor γ .
Gamma factor γ = 1 − 0. 9 2 1 = 1 − 0.81 1 = 0.19 1 = 2.294 .
Why this step? At 0.9 c we are firmly relativistic; γ measures how big the correction is before we touch momentum.
Speed in SI v = 0.9 c = 0.9 × 3 × 1 0 8 = 2.7 × 1 0 8 m/s .
Why this step? The formula needs metres per second, not "0.9 c ."
Correct momentum p = γ m e v = ( 2.294 ) ( 9.11 × 1 0 − 31 ) ( 2.7 × 1 0 8 ) = 5.64 × 1 0 − 22 kg⋅m/s .
Why this step? Cell I's face — insert the γ stretch that the naive formula forgets.
Correct wavelength λ = p h = 5.64 × 1 0 − 22 6.626 × 1 0 − 34 = 1.17 × 1 0 − 12 m .
Naive (wrong) momentum p naive = m e v = ( 9.11 × 1 0 − 31 ) ( 2.7 × 1 0 8 ) = 2.46 × 1 0 − 22 , giving λ naive = 2.46 × 1 0 − 22 6.626 × 1 0 − 34 = 2.69 × 1 0 − 12 m .
Why this step? We compute the mistake on purpose, to see the size of the error.
Verify: the naive answer (2.69 pm ) is exactly γ = 2.294 times too big compared to the correct 1.17 pm : 2.69/1.17 = 2.30 ≈ γ . ✓ Ignoring relativity would have doubled your wavelength — always check K vs m c 2 first. ✓
Intuition Running the formula backwards
So far every problem handed us the physics and asked for λ . Exams love to flip it: they give you λ and ask for the voltage or energy that produced it. Nothing new is needed — you take whichever face fits and solve for the unknown with plain algebra. The only skill is not panicking when the arrow points the other way.
Worked example Ex 10 · You measure an electron's wavelength as
λ = 0.5 A ˚ . Through what voltage V was it accelerated?
Forecast: a short wavelength (0.5 A ˚ is shorter than the 1.23 A ˚ at 100 V ) means high momentum means high voltage. Expect V well above 100 V .
Start from the electron face λ = V 12.27 A ˚ and solve for V : rearrange to V = λ 12.27 , then square: V = ( λ 12.27 ) 2 with λ in Å.
Why this step? The forward formula runs V → λ ; we simply reverse the algebra so λ → V .
Plug in V = ( 0.5 12.27 ) 2 = ( 24.54 ) 2 = 602 V .
Why this step? Substitute the measured λ into the inverted formula.
Verify: 602 V > 100 V , as the forecast demanded. And check it forward: λ = 12.27/ 602 = 12.27/24.5 = 0.50 A ˚ . ✓ The round trip closes — always plug your answer back into the original formula. ✓
Recall Which face do I use? (self-test)
Given only a temperature , which face and what's the first step? ::: Face D (h / 2 m K ); first compute K = 2 3 k B T .
Why can't a photon use λ = h / m v ? ::: Its mass is zero, so h / ( m v ) = h /0 is undefined; use λ = h / p with p = E / c .
At equal kinetic energy, λ ∝ ? ::: 1/ m (so electron/proton ratio is 1836 ≈ 42.8 ).
At equal speed, λ ∝ ? ::: 1/ m (ratio 1836 , not 1836 ).
When does p = m v fail? ::: Near light speed; then p = γ m v with γ = 1/ 1 − v 2 / c 2 .
Given λ , how do you find the electron voltage? ::: Invert the face: V = ( 12.27/ λ ) 2 with λ in Å.
Mnemonic The decision rule
"What did they GIVE me?" — speed→h / m v , energy→h / 2 m K , voltage(electron)→12.27/ V , massless→h / ( E / c ) , near-c →multiply momentum by γ , λ given→invert the face.