PV Efficiency Explorer

PhotoVoltaics

Explore photovoltaic technology developments, individual PV cell records, and PV module performance data.

Background

FOUNDATIONS

Light, photons and photovoltaic bandgaps

Light is electromagnetic radiation. A solar cell responds to the energy carried by its photons, not simply to whether the light looks bright to the human eye.

Light can be described as an electromagnetic wave with wavelength λ and frequency ν, related by c = λν. It also arrives in discrete packets called photons. The energy of one photon is Eph = hν = hc/λ, so shorter-wavelength light has higher-energy photons. Sunlight at Earth's surface extends beyond the visible rainbow into ultraviolet and infrared wavelengths.

A semiconductor's bandgap Eg is the energy separation between its valence and conduction bands. A photon can generate an electron–hole pair only if it is absorbed and Eph ≥ Eg. A lower-energy photon normally passes through a simple absorber; a much higher-energy photon can be absorbed, but energy above the bandgap is rapidly lost as heat while the carrier relaxes towards the band edge.

Photon energy: Eph = hν = hc/λ

Absorption threshold: Eph ≥ Eg

Approximate cut-off: λg [nm] ≈ 1240 / Eg [eV]

The bandgap therefore sets a material's longest usable wavelength, but it does not alone determine how strongly or how deeply light is absorbed. Optical thickness, direct or indirect transitions, reflection and material quality also matter. Intensity controls how many photons arrive per unit area and time; wavelength controls the energy of each photon.

A single-junction cell cannot use every photon energy perfectly. A lower bandgap captures more of the spectrum but generally limits voltage, while a higher bandgap can support more voltage but misses longer wavelengths. Tandem and multijunction cells stack different bandgaps so high-energy photons are absorbed first and lower-energy photons can reach a narrower-bandgap cell beneath.

Scientific references: NASA electromagnetic-spectrum fundamentals, U.S. DOE photovoltaic-cell basics, and DOE wavelength and PV-loss overview.

How light wavelength, photon energy and semiconductor bandgap govern photovoltaic absorption The electromagnetic spectrum runs from higher-energy ultraviolet through visible light to lower-energy infrared. Three band diagrams show that sub-bandgap photons transmit, photons at or above the bandgap create electron-hole pairs, and excess photon energy becomes heat. Example semiconductor bandgaps and approximate cut-off wavelengths are listed.
Bandgap is an energy threshold, not a wavelength band that the cell “absorbs”. Values are representative room-temperature bandgaps and rounded cut-off wavelengths. Actual spectral response also depends on absorption coefficient, thickness, reflection, recombination and collection.

Photovoltaic cell layer

Cell layer

Explanation level