Photovoltaic physics
A photovoltaic (PV) cell is a semiconductor diode that converts incident photons into an electric current. The conversion has three steps:
- A photon hits the semiconductor and is absorbed if its energy exceeds the material's bandgap .
- The absorbed photon excites an electron from the valence band to the conduction band, creating an electron-hole pair.
- The pair is separated by the built-in electric field of the p-n junction, driving current through an external circuit.
The physics implies two structural inefficiencies:
- Photons with are not absorbed at all. Their energy passes through the cell.
- Photons with are absorbed but the excess energy is wasted as heat.
The Shockley–Queisser limit (1961) computes the maximum efficiency of a single-junction PV cell under standard sunlight as a function of bandgap. The optimum bandgap is around 1.34 eV; the resulting limit is ~33.7%.
Real single-junction silicon cells reach ~26–27% in production today, with laboratory records pushing higher. The remaining gap to Shockley-Queisser comes from imperfect light trapping, recombination losses, and series resistance.
To exceed Shockley-Queisser, multi-junction cells stack semiconductors with different bandgaps, each absorbing a different part of the spectrum. Multi-junction cells reach ~47% efficiency under concentrated sunlight in laboratory measurements, but the manufacturing complexity confines them to specialized applications (satellites, concentrator PV). Commercial flat-panel PV remains single-junction or close to it.
