Photoelectric Effect — Einstein's Equation

easy CBSE JEE-MAIN JEE-ADVANCED NCERT Class 12 4 min read

Question

A metal surface has a work function of 2.0 eV. Light of wavelength 400 nm falls on it. Find:

  1. The maximum kinetic energy of emitted photoelectrons
  2. The stopping potential

Given: h=6.626×1034h = 6.626 \times 10^{-34} J·s, c=3×108c = 3 \times 10^8 m/s, 11 eV =1.6×1019= 1.6 \times 10^{-19} J


Solution — Step by Step

We need the energy of one photon hitting the surface. Use E=hc/λE = hc/\lambda.

E=hcλ=6.626×1034×3×108400×109E = \frac{hc}{\lambda} = \frac{6.626 \times 10^{-34} \times 3 \times 10^8}{400 \times 10^{-9}} E=1.988×10254×107=4.97×1019 JE = \frac{1.988 \times 10^{-25}}{4 \times 10^{-7}} = 4.97 \times 10^{-19} \text{ J}

Converting to eV: E=4.97×10191.6×10193.1 eVE = \dfrac{4.97 \times 10^{-19}}{1.6 \times 10^{-19}} \approx \mathbf{3.1 \text{ eV}}

Einstein’s equation tells us that the photon’s energy goes into two parts: knocking the electron free (work function ϕ\phi) and giving it kinetic energy.

KEmax=hνϕ=EphotonϕKE_{max} = h\nu - \phi = E_{photon} - \phi KEmax=3.1 eV2.0 eV=1.1 eVKE_{max} = 3.1 \text{ eV} - 2.0 \text{ eV} = \mathbf{1.1 \text{ eV}}

The electron uses 2.0 eV just to escape the metal — the leftover 1.1 eV becomes kinetic energy.

Stopping potential V0V_0 is the voltage needed to bring the fastest electron to rest. We equate electrical work done against the electron to its kinetic energy.

eV0=KEmaxeV_0 = KE_{max} V0=KEmaxe=1.1 eVe=1.1 VV_0 = \frac{KE_{max}}{e} = \frac{1.1 \text{ eV}}{e} = \mathbf{1.1 \text{ V}}

This step is almost trivial once you’re in eV — numerically, stopping potential in volts equals KEmaxKE_{max} in eV. Remember this shortcut for MCQs.


Why This Works

Einstein proposed that light comes in discrete packets called photons, each carrying energy E=hνE = h\nu. When a photon hits the metal, it interacts with one electron — all or nothing. The electron needs a minimum energy ϕ\phi (the work function) just to escape the surface. Whatever’s left over becomes kinetic energy.

This is why intensity doesn’t matter for the threshold — shining more light just sends more photons, but if each photon is below threshold energy, no electrons come out regardless of brightness. Frequency is what counts. This was the key experimental observation that classical wave theory could never explain, and it won Einstein the 1921 Nobel Prize (not relativity — that’s a common misconception worth knowing for general awareness).

The stopping potential concept comes from the reverse setup: apply a retarding voltage until even the fastest electrons can’t reach the collector. At exactly V0V_0, current drops to zero.


Alternative Method

For quick MCQ solving, use the energy directly in eV without converting to joules.

For any visible/UV light, use the shortcut formula:

Ephoton (in eV)=1240λ (in nm)E_{photon} \text{ (in eV)} = \frac{1240}{\lambda \text{ (in nm)}}

For λ=400\lambda = 400 nm: E=1240/400=3.1E = 1240/400 = 3.1 eV — same answer, calculated in 5 seconds.

This hc=1240hc = 1240 eV·nm is a number worth memorising. It appears in JEE Main almost every year, including the 2023 Shift 2 paper.

Then directly: KEmax=3.12.0=1.1KE_{max} = 3.1 - 2.0 = 1.1 eV and V0=1.1V_0 = 1.1 V. No unit conversions needed.


Common Mistake

Confusing stopping potential units with energy units.

Students write V0=1.1×1.6×1019V_0 = 1.1 \times 1.6 \times 10^{-19} V — multiplying by the charge of an electron unnecessarily. The stopping potential is 1.1 V, not 1.76×10191.76 \times 10^{-19} V.

The relation eV0=KEmaxeV_0 = KE_{max} means: (charge in coulombs) × (voltage in volts) = energy in joules. If you already have KEmaxKE_{max} in eV, the numerical value is directly the stopping potential in volts. Don’t double-convert.


KEmax=hνϕ=hcλϕKE_{max} = h\nu - \phi = \frac{hc}{\lambda} - \phi eV0=KEmaxeV_0 = KE_{max} hcλthreshold=ϕ(at threshold, KEmax=0)\frac{hc}{\lambda_{threshold}} = \phi \quad \text{(at threshold, } KE_{max} = 0\text{)}

Shortcut: hc=1240hc = 1240 eV·nm

This is a high-weightage topic for both CBSE Class 12 boards and JEE Main. The boards often ask for stopping potential directly; JEE likes to combine this with de Broglie wavelength of the emitted electron — so once you’re comfortable here, the next step is finding λdB=h/2mKEmax\lambda_{dB} = h/\sqrt{2mKE_{max}} for the emitted electron.

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