🏠 Home
FractionRush AQA A-Level Physics 2

💡 Photons & the Photoelectric Effect

Discover how light quanta interact with electrons in metals

AQA A-Level Physics 2
📦Define the photon and calculate photon energy E = hf
🚪Define work function and threshold frequency
Apply Einstein's photoelectric equation
🛑Explain stopping potential and its significance
🔬Explain observations of the photoelectric effect
📏Convert between eV and joules for photon energies

Photons and Photon Energy

Light and all electromagnetic radiation consists of discrete packets of energy called photons. This was proposed by Einstein in 1905. A photon is a quantum of electromagnetic radiation.

E = hf = hc/λ
h = 6.63 × 10⁻³⁴ J s (Planck's constant)
f = frequency (Hz); λ = wavelength (m); c = 3.00 × 10⁸ m s⁻¹
Electronvolt (eV): The energy gained by an electron accelerated through a potential difference of 1 volt. 1 eV = 1.60 × 10⁻¹⁹ J. Useful for expressing energies of photons and particles at atomic scales.
Type of EM radiationTypical frequency / HzPhoton energy / eV
Radio10⁶4 × 10⁻⁹
Visible light~5 × 10¹⁴~2
UV10¹⁵~4
X-rays10¹⁸~4000

The Photoelectric Effect

When electromagnetic radiation of sufficient frequency shines on a metal surface, electrons are emitted. This is the photoelectric effect. Key observations:

The classical wave model of light cannot explain these observations. It predicts that any frequency would eventually emit electrons given enough time/intensity. The photon model explains all observations correctly.

Work Function and Einstein's Equation

Work function φ: The minimum energy needed to remove an electron from the surface of a metal. It is a property of the metal.
Threshold frequency f₀: The minimum frequency of light that will cause photoelectric emission: φ = hf₀, so f₀ = φ/h.
Einstein's photoelectric equation:
hf = φ + E_k(max)
E_k(max) = hf − φ = hf − hf₀ = h(f − f₀)

The photon gives all its energy to one electron. Some energy φ is used to free the electron from the metal surface. Any remaining energy appears as kinetic energy of the emitted electron. The maximum KE is for electrons emitted from the surface with no energy lost within the metal.

This is a one-photon-one-electron interaction. The photon is absorbed entirely, not split between electrons. This is why intensity (more photons, same energy each) increases photocurrent but not maximum KE.

Stopping Potential

Stopping potential V_s: The minimum negative potential applied to the collector to stop all emitted electrons from reaching it, even the fastest ones.
eV_s = E_k(max) = hf − φ
So: V_s = (hf − φ) / e

Stopping potential is measured by applying a reverse voltage and finding the value at which photocurrent just reaches zero. Plotting V_s against f gives a straight line:

V_s = (h/e)f − φ/e
Gradient = h/e; y-intercept = −φ/e
This graph gives an experimental method to determine Planck's constant h. The gradient of V_s vs f = h/e = 6.63 × 10⁻³⁴ / 1.60 × 10⁻¹⁹ = 4.14 × 10⁻¹⁵ V s.
Light of wavelength 250 nm shines on a sodium surface (work function φ = 2.28 eV). Calculate the maximum kinetic energy of emitted electrons in joules and eV.
1E_photon = hc/λ = (6.63 × 10⁻³⁴ × 3.00 × 10⁸) / (250 × 10⁻⁹) = 7.956 × 10⁻¹⁹ J
2Convert to eV: 7.956 × 10⁻¹⁹ / 1.60 × 10⁻¹⁹ = 4.97 eV
3E_k(max) = hf − φ = 4.97 − 2.28 = 2.69 eV
4In joules: 2.69 × 1.60 × 10⁻¹⁹ = 4.30 × 10⁻¹⁹ J
E_k(max) = 2.69 eV = 4.30 × 10⁻¹⁹ J
Find the threshold frequency for zinc, which has a work function of 4.31 eV.
1Convert φ to joules: 4.31 × 1.60 × 10⁻¹⁹ = 6.896 × 10⁻¹⁹ J
2φ = hf₀ → f₀ = φ/h = 6.896 × 10⁻¹⁹ / 6.63 × 10⁻³⁴
3f₀ = 1.040 × 10¹⁵ Hz
f₀ = 1.04 × 10¹⁵ Hz (UV range — visible light cannot cause emission from zinc)
A stopping potential of 1.20 V is measured for light of frequency 6.80 × 10¹⁴ Hz. Calculate Planck's constant from this data.
1eV_s = hf − φ. We need another frequency to find h graphically, but with a known work function we can use a single measurement. Assume φ for caesium = 2.00 eV = 3.20 × 10⁻¹⁹ J.
2eV_s = hf − φ → h = (eV_s + φ) / f
3h = (1.60 × 10⁻¹⁹ × 1.20 + 3.20 × 10⁻¹⁹) / 6.80 × 10¹⁴
4h = (1.92 × 10⁻¹⁹ + 3.20 × 10⁻¹⁹) / 6.80 × 10¹⁴ = 5.12 × 10⁻¹⁹ / 6.80 × 10¹⁴ = 7.53 × 10⁻³⁴ J s
h ≈ 7.5 × 10⁻³⁴ J s (differs from 6.63 × 10⁻³⁴ due to approximate φ used)
Explain, using the photon model, why doubling the intensity of light below the threshold frequency still produces no photoelectrons.
1Intensity is proportional to the number of photons per second per unit area — more photons, but each photon has the same energy E = hf.
2Below threshold: hf < φ, so no single photon has enough energy to free an electron from the surface.
3The interaction is one-photon-one-electron. Two low-energy photons cannot combine to release one electron.
More photons → more collisions, but each carries insufficient energy → no emission regardless of intensity

1. Which variable determines whether photoelectric emission occurs?

2. Light of frequency 8.0 × 10¹⁴ Hz has what photon energy? (h = 6.63 × 10⁻³⁴ J s)

3. A metal has a work function of 3.0 eV. What is the threshold frequency? (h = 6.63 × 10⁻³⁴ J s)

4. If intensity of light above f₀ is doubled, what happens to the maximum kinetic energy of emitted electrons?

5. A stopping potential of 0.80 V is needed for light of wavelength 400 nm on a metal. Find the work function in eV. (hc = 1.99 × 10⁻²⁵ J m)

1. A student plots stopping potential V_s (y-axis) against frequency f (x-axis) for several different metals and frequencies. The graph is a straight line. The gradient is 4.0 × 10⁻¹⁵ V s and the x-intercept is 5.5 × 10¹⁴ Hz. Find: (a) Planck's constant h, (b) the work function φ in eV.

2. A photon of 5.0 eV strikes a metal with work function 3.5 eV. (a) Calculate the maximum speed of emitted electrons. (b) Calculate the de Broglie wavelength of these electrons. (m_e = 9.11 × 10⁻³¹ kg, h = 6.63 × 10⁻³⁴ J s)

3. A laser of power 2.0 mW emits light at 500 nm. Calculate the number of photons emitted per second.