🟢 Modern physics · Class 11–12 · Boards + AP + Olympiad

A bright red lamp does nothing a dim violet one cannot

E = hf · KEmax = hf − φ · and the end of light as only a wave

Shine red light on caesium as brightly as you like and not one electron leaves. Shine the faintest violet and they come off at once. No wave theory can produce that result, and the experiment that showed it is where the quantum century begins.

One packet
E = hf, all or nothing
One cost
The work function φ
One surprise
Brightness sets how many, never how fast
Photon · E = hfEscape · φLeftover · KE = hf − φh · 4.14 × 10⁻¹⁵ eV·s
What you'll learn

Why light had to be counted, not just measured

This page covers the four observations a wave picture cannot explain, the photon that explains all four at once, the work function of a metal, and the straight line whose gradient is Planck's constant. By the end you'll be able to:

  • State the four results and say exactly which one each wave prediction fails.
  • Use KEmax = hf − φ in either direction, in joules or electronvolts.
  • Find a threshold frequency and explain why brightness cannot get past it.
  • Read a stopping voltage and say what it measures and what it does not.
  • Drive the Photocell Bench and watch the brightness slider move the current and nothing else.
Why it matters · where it's tested

The experiment that bought Einstein a Nobel Prize

Not relativity — this. It is also the operating principle of every solar panel, camera sensor and automatic door in the world:

CBSE · Class 12 — Dual nature of radiation and matter ICSE — Modern physics IGCSE · Cambridge — Quantum physics Edexcel — Photoelectricity AP Physics 2 — Quantum physics Olympiad — NSEP · IPhO foundations

Searched as: photoelectric effect explanation, work function, threshold frequency, stopping potential, einstein photoelectric equation, why wave theory fails.

Formulas at a glance

Depth guide: 🟢 Class 11–12 must-know · 🟡 useful · 🔴 extension
FormulaMeaningUnitLevel
E = hfTHE PHOTON — light arrives in packets, one per electron
this single line is what the whole chapter rests on
joule or eV🟢
KEmax = hf − φEINSTEIN'S EQUATION — what arrives, minus what it costs to get outeV🟢
φ = hf₀The work function, written as a threshold frequencyeV🟢
λ₀ = hc/φThe longest wavelength that still works at allm🟢
eVs = KEmaxThe stopping voltage measures the fastest electronsvolt🟡
E = hc/λPhoton energy straight from wavelength — 1240 eV·nm is worth memorisingeV🟡
p = h/λA photon carries momentum too, which is what Compton measuredkg·m/s🔴

See it live

Predict the stopping voltage, lock it, then drag the brightness from one end to the other and watch what refuses to move. 🟢 real KE = hf − φ engine

Photocell Bench

Photon energy3.02 eV
Escape cost2.10 eV
Electrons per second5 units
Stopping voltage0.92 V
Predict first: what stopping voltage will this setting give, in volts?

Guess, then lock — the bench waits until you commit.

Which metal
KE = hf − φ → 0.92 eV
→One photon arrives
→One electron absorbs all of it
→It pays φ to get out
→Whatever is left is its speed

Set a wavelength and a metal, then drag the brightness across its whole range and watch what does not move.

What decides this?

Six results from the laboratory. For each one, decide whether the frequency, the brightness or the metal is responsible — that is the whole argument.

Observation 1 of 6
Named: 0 of 6

Bright red light shone on caesium, and nothing at all comes off. What decides this?

Ask whether the change is about how much energy each photon carries, or simply how many of them arrive.

ObservationWhat decides itWhy

A wave picture gets three of these six exactly backwards, which is why the experiment mattered.

Hit the stopping voltage

A caesium photocell, and a target stopping voltage. Choose a wavelength that delivers it — 3 attempts.

3 tries
Attempts left: 3

Set the wavelength, then shine it. eVₛ = hf − φ.

Impossible results — what is wrong?

Each claim breaks something the experiment actually shows. Tap the broken idea.

What is impossible?

An electron absorbs one photon or none. If a single red photon carries less than the work function, no number of them will help, and the threshold is absolute rather than gradual.

What is impossible?

Speed comes from the energy of the single photon each electron absorbs, and brightness does not change what one photon carries. Doubling it doubles the NUMBER of electrons and leaves the stopping voltage exactly where it was.

What is impossible?

The measured delay is under a nanosecond however dim the light is. A wave picture predicts minutes of accumulation for a faint source, and that delay has never been observed — emission is immediate or it does not happen.

Always · Sometimes · Never

Thinking beats memorising. Sort every claim about the photoelectric effect into three boxes.

Always

  • One electron absorbs one photon, whole or not at all
  • The maximum kinetic energy is hf minus the work function
  • Emission begins immediately or not at all

Sometimes

  • Electrons come off — only above the threshold frequency
  • Brightness matters — for the current, never for the speed
  • Visible light is enough — caesium yes, zinc no

Never

  • Brightness getting past the threshold frequency
  • A measurable delay while energy accumulates
  • A brighter lamp raising the stopping voltage

More light, or more energy?

One change is made to the experiment. Say whether the current goes up, the maximum kinetic energy goes up, or neither does.

Read the change
Score: 0 of 0
After this change,

Ask whether the change alters the energy of each photon or only how many arrive.

Choose the metal

A photocell answers to everything shorter than its own cut-off wavelength. Pick a job, then pick a work function that matches it.

Building: a sensor that responds to ordinary room light
Not this one

λ₀ = hc/φ — a bigger work function means a shorter cut-off.

Everyday detective

Read the scene. All three are the same threshold, wearing ordinary clothes.

Why is no solar panel anywhere near a hundred per cent efficient?

Silicon has a threshold around 1.1 eV, so every infrared photon below it passes through without freeing anything, and every photon well above it wastes the surplus as heat. Those two losses together cap a simple silicon cell at about a third, before any manufacturing issue is considered.

Why does sunlight burn your skin when a very bright desk lamp does not?

It is a threshold, exactly like the photoelectric one. Breaking a chemical bond in skin needs a photon above a certain energy, and visible photons fall short however many arrive. The ultraviolet in sunlight clears it, which is why a lamp a hundred times brighter still cannot burn you.

Why does a photograph taken in very dim light look grainy?

Each pixel counts the electrons freed by arriving photons. When only a handful arrive, the count naturally varies between neighbouring pixels, and that variation is the grain. You are looking at the discreteness of light itself.

What's going on

In plain terms: light does not deliver its energy smoothly. It arrives in countable packets, one electron takes one packet, and everything strange about this experiment follows from that.

One photon, one electron

A photon carries E = hf, and an electron absorbs one of them entirely or not at all. It cannot save up two half-payments. That single rule explains why a threshold exists: if one photon is short of the escape cost, a billion of them are still each short of it, and the metal stays quiet however bright the lamp.

The escape cost, and what is left

Getting out of a metal costs a minimum amount of energy called the work function, φ, which differs from metal to metal — 2.1 eV for caesium, 5.65 for platinum. Whatever the photon brought beyond that becomes kinetic energy, so KEmax = hf − φ. It says maximum because electrons starting deeper in the metal lose more on the way out.

Why this broke the wave picture

A wave spreads its energy smoothly, so a faint wave should free electrons slowly rather than not at all, and a brighter wave should free them faster. The experiment says the opposite on both counts: emission is instant or absent, and brightness changes only the number. Four separate results, and the photon explains all four with one line of arithmetic.

Edge cases worth knowing

The stopping voltage measures the fastest electrons, not the average, which is why the formula carries the word maximum. A graph of KE against frequency is a straight line of gradient h for every metal, with only the intercept changing — which is how Millikan measured Planck's constant. And light still diffracts and interferes, so this experiment did not replace the wave picture; it proved one picture was never going to be enough.

Solve it with me, step by step 🟢 Class 11–12

Exams reward the method. Work it one step at a time — read the thought, predict the line, then reveal it.

See the maths

Three small labs. The middle one is the one that ended the argument.

1 · Energy against frequency

A straight line that starts at the threshold. Its gradient is Planck's constant, measurable with a ruler.
KE
1.21 eV
KE = hf − φ · caesium, φ = 2.10 eV

2 · What brightness does, and does not

The dark line is the current and it climbs. The amber line is the maximum energy, and it does not move at all.
KE
1.40 eV
brightness sets the count, never the energy

3 · Cut-off wavelength against work function

Where a metal stops responding. The dashed lines mark the edges of what your eye can see.
λ₀
590 nm
λ₀ = hc/φ · hc = 1240 eV·nm

How light became countable

1887

Hertz notices something odd

While proving radio waves exist, Hertz found that ultraviolet light made a spark gap fire more easily. He reported it and moved on; nobody could explain it.

1900

Planck introduces h

Planck found that treating energy as coming in small fixed amounts fixed the equations for radiation from hot objects. He regarded it as a mathematical device.

1905

Einstein takes the packets seriously

He proposed that light itself really does arrive as packets of energy hf, and wrote down KE = hf − φ. The idea was rejected by almost everyone, including Planck.

1916

Millikan fails to disprove it

Ten years of precise measurement intended to refute Einstein produced a perfect straight line of gradient h. Millikan published the result and said plainly that the equation held.

1921

The Nobel Prize

Einstein received it for this, not for relativity. The committee wanted something experimentally settled, and by then this was.

In the real world

A solar panel

Photons above the threshold free charge carriers; the rest pass through or waste their surplus as heat, which is why efficiency has a ceiling.

A camera sensor

Each pixel counts freed electrons. In very low light the grain you see is the random arrival of individual photons.

An automatic door

A beam keeps a photocell current flowing. Break the beam and the current stops, which is the signal to open.

From a radio photon to an X-ray 🟡

Drag the slider. Six photon energies, and what a single one of each can and cannot do.

radiomicroinfraredvisibleUVX-ray

A visible photon

about 2 eV

Twelve orders of magnitude of photon energy, and a threshold sitting somewhere in every material.

Build it yourself — science-fair projects

Each one is a build and a measurement — the measuring is what turns a demo into a project.

⚡Beginner

The zinc plate and the electroscope

Shows · the threshold is real

Build: a freshly cleaned zinc plate on a charged electroscope, lit first by a bright lamp and then by an ultraviolet source.

Measure: the time for the leaf to fall in each case. The lamp does nothing at all; the ultraviolet source discharges it in seconds.

🔅Beginner

A solar cell and a set of filters

Shows · colour matters more than brightness

Build: a small solar cell, a lamp, and coloured filters that pass roughly equal amounts of light.

Measure: the voltage for each colour at matched brightness, and see how it tracks the wavelength.

💡Intermediate

Measure h with coloured LEDs

Shows · Planck's constant, on a bench

Build: several LEDs of known wavelength, each on a variable supply with a meter.

Measure: the turn-on voltage of each, plot it against 1/λ, and the gradient gives hc/e to within a few per cent.

📈Intermediate

The stopping voltage graph

Shows · KE = hf − φ

Build: a school photocell with a variable retarding voltage and four narrow-band filters.

Measure: the stopping voltage for each filter, plot against frequency, and read h off the gradient and φ off the intercept.

📷Champion

Photograph the photon count

Shows · light is discrete

Build: a camera on manual, photographing an almost dark scene at rising ISO settings.

Measure: the pixel-to-pixel variation in a flat patch. It should grow as the square root of the count, which is what a countable arrival predicts.

🔬Champion

Find the cell's cut-off

Shows · the work function

Build: a photocell and a simple grating or prism spreading a lamp's light across it.

Measure: the longest wavelength that still gives a reading, then work backwards to φ = hc/λ₀ and identify the metal.

Glossary — the 10 words that unlock it

Photon

What it means
A single packet of light energy.
Why it matters
One electron absorbs one, whole or not at all.
Example
A green photon carries about 2.4 eV.
Key question
Can an electron take two?

E = hf

What it means
A photon's energy is its frequency times Planck's constant.
Why it matters
It ties colour directly to energy.
Example
1240 eV·nm divided by the wavelength.
Key question
What does brightness change?

Work function

What it means
The least energy needed to escape a metal.
Why it matters
It sets the threshold for that metal.
Example
Caesium 2.1 eV, platinum 5.65 eV.
Key question
Why does it differ between metals?

Threshold frequency

What it means
The lowest frequency that frees any electrons.
Why it matters
Below it, brightness is powerless.
Example
f₀ = φ/h.
Key question
Is it gradual or absolute?

Photoelectron

What it means
An electron freed by light.
Why it matters
Counting them is the current.
Example
What flows in a photocell.
Key question
Do they all have the same speed?

Intensity

What it means
How many photons arrive each second.
Why it matters
It sets the current and nothing else.
Example
Twice as bright, twice the current.
Key question
Does it change the stopping voltage?

Stopping voltage

What it means
The reverse voltage that just stops the current.
Why it matters
It measures the maximum kinetic energy directly.
Example
0.38 V means 0.38 eV.
Key question
Fastest electrons, or average?

Planck's constant

What it means
The number linking frequency to energy.
Why it matters
It is the gradient of the KE–frequency line.
Example
4.14 × 10⁻¹⁵ eV·s.
Key question
Does it change between metals?

Electronvolt

What it means
The energy one electron gains crossing one volt.
Why it matters
It makes these numbers human-sized.
Example
1 eV = 1.6 × 10⁻¹⁹ J.
Key question
Why not just use joules?

Wave–particle duality

What it means
Light behaves as a wave in some experiments and as particles in others.
Why it matters
Neither picture alone covers everything.
Example
Two slits against a photocell.
Key question
Which one is light really?
हिन्दी · key words Photon · फोटॉन Energy · ऊर्जा Frequency · आवृत्ति Electron · इलेक्ट्रॉन Threshold · दहलीज

The questions people ask

Straight answers, each one complete on its own:

Why does a bright red light free no electrons when a dim violet one does?
Why

Because an electron absorbs one photon or none, and cannot combine several. A red photon carries less energy than the metal's work function, so it cannot pay the escape cost no matter how many of its companions arrive. A violet photon carries more than the cost, so every one that is absorbed frees an electron, even if only a handful arrive each second.

What exactly is the work function?
What

It is the minimum energy an electron needs to escape from the surface of a particular metal, and it is a property of that metal alone. Caesium's is about 2.1 electronvolts and platinum's about 5.65, which is why caesium responds to visible light and platinum needs deep ultraviolet. It is the amount subtracted in Einstein's equation.

Why does the equation say maximum kinetic energy?
Why

Because only electrons right at the surface escape having paid exactly the work function. Electrons starting deeper inside lose additional energy on the way out through collisions, so they emerge more slowly. The result is a spread of speeds from zero up to a maximum, and it is that maximum which hf minus φ predicts and which the stopping voltage measures.

What does the stopping voltage actually measure?
How

It is the reverse voltage just large enough to turn back even the fastest electron, so the current falls to zero. Since an electron crossing a potential difference V loses energy eV, the stopping voltage multiplied by the electron charge equals the maximum kinetic energy. In electronvolts the two are numerically the same, which is why the unit is so convenient here.

Does this prove light is not a wave?
Comparative

No. Light diffracts round edges and produces interference fringes, and only waves do that. It also arrives in countable packets with a hard energy threshold, and only particles do that. Both sets of experiments are reliable, so physics accepted that neither picture on its own is complete. That acceptance is what wave–particle duality means.

Why was the absence of a time delay so important?
Scenario

A wave spreads its energy over the whole surface, so a very faint wave would need a long time — minutes, on the arithmetic — for any one electron to accumulate enough to escape. Measurements found emission beginning within about a nanosecond however faint the source. That rules out accumulation entirely and points straight at a single concentrated packet doing the whole job at once.

Why is Planck's constant the same for every metal?
Why

Because it belongs to light rather than to the metal. Plot maximum kinetic energy against frequency for caesium, sodium and zinc and you get three parallel lines: the intercept shifts, because that is the work function, but the gradient is identical because it is h. Millikan used precisely that to measure h to within about half a per cent.

Why are solar panels only about twenty per cent efficient?
Scenario

Two losses, both from this chapter. Photons with less than the threshold energy pass straight through and contribute nothing, which throws away much of the infrared in sunlight. Photons with far more than the threshold free one carrier each and waste the surplus as heat. Together these cap a single-junction silicon cell at about a third even in theory, before any practical losses.

Common mistakes — and the fix 🟢 Class 11–12

Spot these before the exam does.

The slipThe fix
Saying brighter light gives faster electronsIt gives more electrons, at the same maximum speed
Expecting a delay with dim lightEmission is immediate or absent
Adding photon energies togetherOne electron takes one photon, whole or not at all
Mixing joules and electronvolts mid-questionPick one unit; 1 eV = 1.6 × 10⁻¹⁹ J
Reading the gradient as the work functionThe gradient is h; the intercept is −φ
Saying this disproves the wave nature of lightBoth are needed — duality

Test yourself — a mixed set

Seven question formats, the way LLOS.ai serves them — multiple choice, multiple-correct, fill-in-the-blank, match, sequence, read-think-connect, and write-your-own. Every question has layered hints: a quick nudge, the reasoning, then a deeper connection — so a wrong answer opens a door, never a dead end. 🟢 received from a board-tagged question bank · seed toward 2,000

Pick your board — the set re-tunes to its wording and emphasis. Competitive draws the JEE / NEET / Olympiad lane.

Loading the question bank…
Question 1 of 16
Multiple choice

Which gives the fastest electrons?

Four setups, four different lamps and metals. Tap them in order, fastest electrons first. Then read the arithmetic — one of them produces nothing at all.

Your ranking
Picked: 0 of 4
A · the bright red lamp

650 nm red, turned up as bright as the supply allows, on caesium.

B · the dim violet lamp

410 nm violet, barely visible in a dark room, on caesium.

C · the ultraviolet lamp

250 nm ultraviolet at moderate brightness, on zinc.

D · the green laser

532 nm green, bright and steady, on caesium.

Tap the four in the order you believe, fastest electrons first.

Key takeaways

  • One electron takes one photon, whole or not at all — and that single rule explains everything else.
  • KEmax = hf − φ — what arrives, minus what it costs to get out.
  • Below the threshold, brightness is powerless, which no wave picture can reproduce.
  • Brightness sets the current and never the speed.
  • Light is both — it still diffracts, and it still arrives in packets.

Where this lesson leads

This is the doorway into quantum physics, and every step after it uses the same packet idea:
✓The photon and E = hf
✓Work function and threshold
✓Einstein's equation
→Atomic spectra and energy levels
→Matter waves and de Broglie
→Quantum mechanics proper

Keep exploring

Millikan spent ten years trying to prove Einstein wrong about this and measured Planck's constant instead. That is what a good experiment does to a good argument.

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