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Photoelectric Effect.

Try releasing electrons with longer-wavelength light before increasing photon flux.

Interactive experimentintuitiveField note ·
INTERACTIVE EXPERIMENT / P05

Photoelectric Effect

Try releasing electrons with longer-wavelength light before increasing photon flux.

TEST THE MECHANISM

Each incident photon has energy approximately 1240 divided by wavelength in nm, measured in eV. An ideal surface has an adjustable work function and one-electron-per-absorbed-photon yield above threshold.

200800
010
14
e⁻ →e⁻ →e⁻ →e⁻ →e⁻ →
Photon energy (eV)
2.07
Maximum energy if emitted (eV)
0.07
Emission now
Allowed

Try the longest wavelength first and raise flux: more below-threshold photons do not release electrons here. Particle icons represent relative flux, not a measured current or emission rate.

An ideal one-electron yield is assumed. Icons encode relative flux, not a measured rate; surface physics, collection voltage and efficiency are omitted.

THE SHORT VERSION

Photoelectric Effect, explained.

The photoelectric effect is electron emission after absorption of photons energetic enough to overcome a material’s work function.

01 / THE MECHANISM

Why it happens

Photon energy is approximately 1240/λ eV for λ in nm. Above threshold the maximum kinetic energy is photon energy minus work function; increased photon flux changes potential emission count rather than energy per photon.

The photoelectric effect is electron emission after absorption of photons energetic enough to overcome a material’s work function.

Read the result

The maximum electron energy is conditional on emission. Positive available energy with zero photon flux does not imply electrons are currently arriving.

02 / FOLLOW IT THROUGH

A worked example

Energy threshold versus photon flux

  1. Set work function to two eV and wavelength to eight hundred nm.

  2. Raise photon flux and observe that below-threshold photons still produce no emission here.

  3. Shorten wavelength to four hundred nm, giving photon energy 3.1 eV and maximum kinetic energy 1.1 eV.

OPTIONAL DEEPER DETAILGo deeper: inside the model

Inside this model

Photon energy is approximately 1240/λ eV for λ in nm. Above threshold the maximum kinetic energy is photon energy minus work function; increased photon flux changes potential emission count rather than energy per photon.

03 / BEYOND THE EXPERIMENT

Where this idea is useful

A practical use

Distinguish the role of a light source’s photon energy from its supplied photon flux.

CHECK YOUR INTUITION

A common misconception

THE TEMPTING CONCLUSION

“Enough weak photons always accumulate to release an electron in this model.”

THE MORE USEFUL DISTINCTION

The ideal one-photon account requires each absorbed photon to exceed the work function; increasing below-threshold flux does not change that energy.

What this explanation leaves out

  • An ideal one-electron yield is assumed. Icons encode relative flux, not a measured rate; surface physics, collection voltage and efficiency are omitted.
ONE MORE QUESTION

Are the electron icons a calibrated current?

No. Their count encodes relative photon flux under a declared ideal yield, not a measured emission rate.

TAKE THE IDEA WITH YOU

Did you change energy per quantum or the number of incident quanta?

Associated thinkers

Associated withAlbert Einstein ↗

Associations marked provisional are awaiting source review.

Further reading

Explore the original research or the teaching reference behind this experiment.