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GRADE 11 · QUANTUM PHYSICS

Photons and the photoelectric effect

Photon energy and momentum, the photoelectric equation and the threshold wavelength.

30 minutes27 theory cards
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Understanding step by step

In an ordinary experiment, red light cannot release electrons from some metals however much its intensity is increased. Weaker light of higher frequency may produce a current. Why does the energy in one portion matter, as well as the total energy delivered?

Brightness is not enoughbright redno electrons emittedweak violetelectrons emittedWhy is brightness not the key?
Bright red light may release no electrons from a metal, while weak light of another frequency does so immediately. The total energy flux is therefore not the deciding factor.

Light transfers energy in portions

When light is absorbed, it transfers energy in discrete portions. A photon is a quantum of electromagnetic radiation; complete absorption transfers its whole energy. Frequency ν, in hertz, sets the energy of one portion. This does not remove wave behaviour: light still interferes and diffracts. Do not picture a photon as a small, cut-off fragment of a wave. Quantum theory connects how light propagates with how it exchanges energy.

p = E / cE = hνm₀ = 0The wavy line is a symbol
In vacuum, a photon travels at c and carries energy hν and momentum E/c. Its invariant rest mass is zero; E/c² is only the mass equivalent of energy.

The energy of one photon

The relation is E=h\nu=hc/\lambda. E is in joules, and the Planck constant h≈6,63·10⁻³⁴ Дж·с sets the size of an energy quantum. Here c≈3·10⁸ м/с and λ is the vacuum wavelength in metres. Doubling frequency doubles photon energy; doubling λ halves it. The units J·s times s⁻¹ give J. Do not combine a wavelength in matter with vacuum c without accounting for the medium's refractive index.

E = h ν = h c / λknown frequencyE = h νknown wavelengthE = h c / λh ≈ 6,63·10⁻³⁴ Дж·сenergy is in joulesuse the vacuum wavelength
Find photon energy from frequency or vacuum wavelength, using the Planck constant to connect them. The result is in joules.

Frequency and brightness

Keep frequency fixed and increase the light flux. More photons cross the same area in the same time, but each still has energy hν. Increasing frequency instead changes the energy of each portion. These two experiments can deliver the same total energy with different photon numbers and energies. This distinction explains the photoelectric threshold: one portion may be insufficient for an electron even when the whole beam carries plenty of energy.

Brighter — more photonsweak lightbright lightsame photons, just more of themfrequency νenergy Efrequency 2νenergy 2Efrequency sets the quantum's energy
At one frequency, brighter light brings more identical quanta, each with unchanged energy. Changing frequency changes the energy of a quantum.

A convenient energy unit

For electron energies, the electronvolt is convenient: approximately 1\,\text{эВ}=1{,}60\cdot10^{-19}\,\text{Дж}. It is the energy associated with an elementary charge crossing a potential difference of 1 V. By definition |e|≈1,60·10⁻¹⁹ Кл is positive; the electron charge is −|e|. An electronvolt is not a voltage: energy is charge times potential difference. The numerical connection for one electron does not make the units interchangeable.

−vFCathode +Anode −Uз
An electron leaves the illuminated cathode towards the anode. A negative anode voltage produces a force opposing electron motion. At the stopping potential even the fastest electrons fail to reach the anode: Eк,max = eUз.

Momentum without rest mass

A photon transfers momentum as well as energy: in vacuum p=E/c=h/\lambda, with p in kg·m/s. Doubling frequency doubles momentum; doubling λ halves it. A photon's rest mass m₀ is zero. There is no contradiction: the familiar p=mv applies to a slow massive object and is not a universal definition of momentum. Momentum transfer by light can exert pressure on an absorber.

p = E / c = h / λγpm₀ = 0nonzero momentumdo not apply p = m vto a photonuse wavelength in vacuum
A photon has zero rest mass but carries energy and momentum. Find its momentum from energy and light speed, or from its vacuum wavelength.

The mass equivalent of energy

We can formally express photon energy in mass units: m_\gamma=E/c^2. This is the mass equivalent of energy, in kilograms, not a nonzero rest mass. The equivalent grows with energy while the photon's invariant mass stays zero. A photon has no rest frame: we cannot come to rest beside it as we could beside a moving trolley. Without this qualification, the historical notation suggests a misleading picture of a massive light particle.

Historical conventionm₀ = 0rest massmγ = E / c²energy equivalentsame name, different quantitiesa photon has no rest framea photon always travels at c
Energy divided by light speed squared is a historical mass equivalent, not rest mass. No reference frame exists in which the photon is at rest.

What is the external photoelectric effect?

In the external photoelectric effect, light releases electrons from a material into the space outside it. An electron is bound to the material. Escaping through the surface needs a minimum energy contribution: the work function A. It is measured in joules or electronvolts and depends on the material and surface condition. Changing the surface can change the threshold even with the same light source. Here work means the energy needed for release, not the duration of illumination.

Work functionmetalthresholdelectron emittedA — work functionA depends on the material and surface
To leave a material, an electron must receive at least a certain energy: the work function. This depends on the material and its surface condition.

The energy balance for one portion

In the single-photon model, one electron absorbs one photon. The balance h\nu=A+E_{\text{к,max}} says that the work function must be supplied first; the remainder can become kinetic energy. The maximum applies to electrons with no additional losses; others can emerge with less energy. Increasing hν at fixed A raises this upper limit by the same amount. If hν<A, a negative kinetic-energy result means emission is impossible, not motion with negative energy.

hνElectronMetalhν = Aвых + Eк,max
An absorbed photon transfers energy hν. Some is needed for the electron to leave the material; the rest is its maximum kinetic energy: hν = Aвых + Eк,max.

Why can weaker light work?

Imagine many photons, each falling just short of A. In the ordinary single-photon process considered here, increasing their number does not combine many portions into one emission event. Intensity therefore cannot overcome the frequency threshold. At sufficient frequency, a larger photon flux can release more electrons and increase the photocurrent. Multiphoton processes under other conditions lie outside this model and do not contradict its stated conclusion.

When a photon falls shorth ν<Amany low-energy quanta still fall shortraise frequency, not photon flux
If one photon has less energy than the work function, the electron is not released. Increasing the flux of these photons does not overcome the threshold.

Threshold frequency

At the emission threshold, the energy left for motion approaches zero: h\nu_0=A, so \nu_0=A/h. Threshold frequency, in hertz, increases with work function: stronger binding requires more energetic photons. For a fixed surface, ν must be at least ν₀ in the ideal threshold model. If A is in eV and h in J·s, first make the energy units consistent. Dividing numbers expressed in different energy units gives the wrong frequency.

No emissionElectron emittedhν < Aвыхhν > Aвых
Below the threshold frequency, no electron is emitted even with many photons in the ordinary single-photon regime. Photoemission is possible for hν ≥ Aвых; excess energy becomes electron kinetic energy.

Threshold wavelength

Since λ=c/ν in vacuum, the lowest allowed frequency corresponds to the longest allowed wavelength: \lambda_0=c/\nu_0=hc/A. This threshold wavelength λ₀ is measured in metres. Doubling A halves it, so shorter waves are needed. The traditional name red limit means the long-wavelength boundary; it need not lie in visible red light. For λ>λ₀ a photon lacks enough energy even if the source is bright.

λ₀ = h c / Aλλ₀photoemissionno emissionlonger wave — less energy per quantumthe red limit need not be visible
The work function determines the longest wavelength that can still cause photoemission. Longer waves carry less energy per quantum and cannot reach the threshold.

Measuring the maximum energy

How can we measure the electrons' maximum energy? Apply a field that slows them on their way to the collector. At the stopping potential Uз, even the most energetic electrons fail to reach it. Uз is the smallest voltage magnitude that achieves this, in volts. With charge in coulombs, E_{\text{к,max}}=|e|U_\text{з} gives energy in joules. Doubling the maximum energy requires twice Uз. The circuit polarity provides retardation; the energy equation uses the positive magnitude.

Stopping potentialcathodecollectorslows downEк,max = |e| Uз
A retarding field prevents photoelectrons reaching the collector. The stopping potential is the smallest voltage magnitude that stops even the fastest electrons.

Electron energy and speed

To find the emission speed of a nonrelativistic electron, use E_{\text{к,max}}=mv_{\max}^2/2, where m≈9,11·10⁻³¹ кг. Thus v_max grows as the square root of energy: quadrupling energy doubles speed. First check that v≪c. For electron energies that bring speed close to c, the classical formula is insufficient. Neither the photoelectric energy balance nor the definition of energy requires treating this approximation as exact outside its range.

Eк,max = m v²max / 2m ≈ 9,11·10⁻³¹ кгelectron massvmax in м/сenergy in joulesvalid for v much smaller than cfast electrons requirea relativistic expression
When electron speed is much smaller than light speed, the ordinary formula relates maximum kinetic energy to maximum speed. For relativistic electrons, that formula is no longer sufficient.

Let us work through an example

Photons of energy 3 eV fall on a metal with work function 2 eV. Find the electrons' maximum kinetic energy and the stopping potential.

What we knowE = 3 эВA = 2 эВelectronEк,max and Uз — ?
Photons of energy three electronvolts fall on a metal with work function two electronvolts. Find the maximum electron kinetic energy and stopping potential.

Let's look at an example · 1

The photons have energy 3 eV and the work function is 2 eV. Since 3 > 2, single-photon emission is energetically possible.

Compare with the threshold3 эВphoton2 эВwork function3 эВ > 2 эВ — photoemission is possible
Photon energy exceeds the work function, so single-photon photoemission is energetically possible.

Let's look at an example · 2

The maximum energy left for motion is Eк,max = E − A = 3 − 2 = 1 эВ.

What is left for the electron?total photon energyA = 2 эВ1 эВh ν = A + Eк,maxEк,max = 1 эВ
Subtract the work function from photon energy. The remainder is the electron's maximum kinetic energy.

Let's look at an example · 3

An electron loses 1 eV of kinetic energy when crossing a retarding potential difference of 1 V. Therefore Uз = 1 В.

Calculate Uз1 эВ equals |e| · 1 ВUз = 1 Вthis is why electronvolts are useful
An electron loses one electronvolt across a retarding potential difference of one volt, so the stopping potential is one volt.

Worked example · 4

The result describes the most energetic electrons. Electrons with extra losses have less energy and stop reaching the collector at a lower voltage.

What does maximum mean?1 эВfastestlessotherseven lesswith lossesUз stops even the fastest electrons
The calculated energy applies to the fastest electrons. Others emerge with less energy and are stopped sooner.

Check the result

Eк,max = 1 эВ, Uз = 1 В. Of each photon's energy, 2 eV is needed for release, leaving at most 1 eV for electron motion.

Key point · 1

Frequency sets the energy of one light quantum. At the same frequency, greater intensity means more quanta.

Key point · 2

Work function sets the threshold. The difference hν−A is the maximum photoelectron energy, not a common energy for all electrons.

Key point · 3

Photons have energy and momentum despite zero rest mass. E/c² is a separate mass equivalent of energy.

What comes next

Next we will explore binding energy and the statistical transformations of atomic nuclei.

Basic Concepts

3 concepts

Photon

A quantum of electromagnetic radiation that transfers energy and momentum.

A photon has no rest frame, and its rest mass is zero. Its energy is E = hν and its momentum is p = h/λ.

Photoelectric effect

The emission of electrons from a material under electromagnetic radiation.

One photon transfers energy to one electron. Frequency determines whether emission is possible and sets the electron energy; intensity controls the number of emitted electrons.

Photoelectric threshold

The lowest frequency, or longest wavelength, at which photoemission is still possible.

In the single-photon model, light below the threshold frequency cannot cause photoemission even if its intensity is increased.

Physical quantities

13 quantities

Photon energy

E

The energy of one quantum of electromagnetic radiation.

Unit: joule · \mathrm{Дж}

Planck constant

h

The proportionality constant relating photon energy to frequency.

Unit: joule-second · \mathrm{Дж}\cdot\mathrm{с}

Radiation frequency

\nu

The number of oscillations of the electromagnetic field per unit time.

Unit: hertz · \mathrm{Гц}

Mass equivalent of photon energy

m_{\gamma}

Photon energy divided by c². This is not rest mass, which is zero for a photon.

Unit: kilogram · \mathrm{кг}

Photon rest mass

m_0

A photon's invariant rest mass is zero. E/c² is not its rest mass.

Unit: kilogram · \mathrm{кг}

Photon momentum

p

The quantity describing a photon's translational motion.

Unit: kilogram-metre per second · \frac{\mathrm{кг}\cdot\mathrm{м}}{\mathrm{с}}

Work function

A

The minimum energy needed to remove an electron from a material's surface.

Unit: joule · \mathrm{Дж}

Photoelectron kinetic energy

E_{\text{к}}

The energy of motion of an electron after leaving a substance.

Unit: joule · \mathrm{Дж}

Photoelectron mass

m

The mass of an electron emitted during the photoelectric effect.

Unit: kilogram · \mathrm{кг}

Magnitude of electron charge

\lvert e\rvert

The positive magnitude of an electron's electric charge.

Unit: coulomb · \mathrm{Кл}

Stopping potential

U_{\text{з}}

The voltage at which even the fastest photoelectrons no longer reach the anode.

Unit: volt · \mathrm{В}

Threshold frequency

\nu_0

The minimum light frequency for photoemission.

Unit: hertz · \mathrm{Гц}

Threshold wavelength

\lambda_0

The longest wavelength of light that can cause photoemission.

Unit: metre · \mathrm{м}

Lesson formulas

11 formulas

Photon energy

E=h\nu=\frac{hc}{\lambda}

The energy of a photon increases with frequency and decreases with wavelength.

Conditions: For a photon in vacuum; the photon's rest mass is zero.

Mass equivalent of photon energy

m_{\gamma}=\frac{E}{c^2}

Photon energy can be assigned a mass equivalent, but this is not the photon's rest mass.

Photon momentum

p=\frac{E}{c}=\frac{h}{\lambda}

The momentum of a photon is determined by its energy or wavelength.

Conditions: For a photon in vacuum.

Planck constant

h\approx6{,}63\cdot10^{-34}\,\mathrm{Дж}\cdot\mathrm{с}

The Planck constant sets the quantum scale of action. In SI, h = 6,62607015·10⁻³⁴ Дж·с exactly; the displayed value is rounded to three significant figures.

Speed of light

c=3\cdot10^8\,\frac{\mathrm{м}}{\mathrm{с}}

The speed of light in vacuum is approximately three hundred million metres per second.

Electronvolts in joules

1\,\mathrm{эВ}=1{,}6\cdot10^{-19}\,\mathrm{Дж}

One electronvolt is the energy an electron gains or loses across a potential difference of one volt.

Einstein's photoelectric equation

E=A+E_{\text{к}}

Photon energy supplies the work function and the electron's kinetic energy.

Photoelectron kinetic energy

E_{\text{к}}=\frac{mv^2}{2}=\lvert e\rvert U_{\text{з}}

Maximum kinetic energy is related to electron speed and stopping potential.

Photoelectric threshold energy

h\nu_0=A

At the threshold, photon energy equals the work function.

Photoelectric threshold frequency

\nu_0=\frac{A}{h}

The minimum frequency is determined by the work function and Planck constant.

Threshold wavelength

\lambda_0=\frac{c}{\nu_0}

The longest allowed wavelength is related to light speed and the threshold frequency.

Test the relationship

Make a prediction first. The button changes the stated quantity; then compare the result and explore other values.

Photoelectric effect: frequency and brightness

hν = Aвых + Eк,max; ν₀ = Aвых/h

Single-photon photoelectric effect with a fixed surface. In this idealized model each absorbed photon above threshold yields one electron. Multiphoton processes are excluded.

At the same frequency, photon flux doubles. How will maximum photoelectron energy change?

Your prediction

Initial values

0-0.50443.750.79877.52.10211.253.405154.708Eк,max, эВν, 10¹⁴ Гц
Eк,max

Calculated result

hν
4.136 эВ
Eк,max
2.136 эВ
ν₀
4.836 10¹⁴ Гц
Jэл/J₀
1

Emission is possible

Explaining the result

Frequency sets each photon’s energy; flux sets the number of photons. Below threshold, increasing flux cannot start single-photon emission; above it, flux does not increase Eк,max.

Related formulas

The same formulas in the reference, with symbols and units.

Problems on this topic

Statements, answer options and the walkthrough.