Photoelectric Effect
Also known as: Einstein's Photoelectric Equation
A photon gives all its energy to one electron; the work function is the minimum escape cost.
Einstein's photoelectric equation running live: photon energy hf (color = true wavelength) versus work function φ. Below the threshold frequency f₀ = φ/h, no electrons leave no matter how intense the light; above it, electrons exit with exactly KE = hf − φ, and their speed on screen scales with the real √KE.
Equivalent forms
A linear equation that toppled the wave-only view of light.
Unit systems
Where it holds
Dimensional analysis
Einstein's explanation of Hertz/Lenard's observations won him the 1921 Nobel Prize and proved light quantization.
Why does dim blue light eject electrons but bright red light can't?
Electrons are only ejected from metal if the photon frequency exceeds a threshold. What is the max KE of photoelectrons from sodium (work function 2.28 eV) under 400 nm light?
- Photomultiplier tubes
- CCD and CMOS image sensors
- Night vision devices
- Solar cells and photodiodes
- ARPES for condensed matter research
- Intensity does NOT affect K_max, only photon count — a classical wave theory would predict otherwise
- The emission is effectively instantaneous (< 10 fs), not delayed as a wave energy-buildup model would require
- The work function is a property of the metal surface, not the bulk
Limiting cases
What if…
Twice as many electrons come out per second, but K_max is unchanged.
No emission from single-photon process. With extreme intensity two-photon absorption can kick in (non-linear regime).
Work function drops slightly (surface contamination raises phi); small but measurable shift in threshold.
Sodium under 400 nm light
- lambda:
- 4e-7
- phi eV:
- 2.28
- K_\max = 3.10 - 2.28 = 0.82\,\mathrm{eV} = 1.31e-19\,\mathrm{J}
Threshold frequency for cesium (phi = 2.1 eV)
- phi eV:
- 2.1