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Shockley–Queisser Limit

1961
  • William Shockley
  • Hans-Joachim Queisser
Research laboratory analyzing single p-n junction solar cell efficiency based on Shockley–Queisser Limit.

(generated image for illustration only)

The Shockley–Queisser limit is the maximum theoretical efficiency for a single p-n junction solar cell. It considers only radiative recombination and black-body radiation losses. For a single-junction cell with an optimal bandgap of 1.34 eV under standard solar illumination (AM1.5G), the maximum efficiency is approximately 33.7%. This fundamental limit guides solar cell research and design.

The Shockley–Queisser (SQ) limit, also known as the detailed balance limit, provides a foundational ceiling on the energy conversion efficiency of solar cells. It is derived by analyzing the thermodynamic balance between the energy absorbed from the sun and the energy lost by the cell. The model makes several key assumptions: the cell is a single p-n junction, it operates at a standard temperature (300 K), and it is illuminated by unconcentrated sunlight (AM1.5G spectrum).

The calculation accounts for several unavoidable loss mechanisms. First, photons with energy less than the semiconductor’s bandgap (\(E_g\)) pass through the cell without being absorbed, contributing nothing to the current. Second, for photons with energy greater than the bandgap, the excess energy (\(E_{photon} – E_g\)) is quickly lost as heat through thermalization, as the excited electron relaxes to the bottom of the conduction band. The voltage is thus limited by the bandgap, not the photon energy. The most significant loss mechanism considered in the SQ limit is radiative recombination. This is the reverse process of absorption, where an electron and hole recombine and emit a photon. In an ideal cell, this is the only recombination pathway. The cell, being at a non-zero temperature, also radiates energy as a black body.

By balancing the incoming photon flux from the sun with the outgoing flux from radiative recombination and black-body radiation, Shockley and Queisser derived the current-voltage characteristic of an ideal cell. The maximum power point on this curve defines the maximum efficiency. The efficiency is a strong function of the bandgap energy, peaking at ~33.7% for a bandgap of 1.34 eV, which is close to that of Gallium Arsenide (GaAs). For silicon (\(E_g \approx 1.12\) eV), the limit is around 32%.

UNESCO Nomenclature: 2210
– Physics

Type

Theoretical Limit

Disruption

Foundational

Usage

Widespread Use

Precursors

  • planck’s law of black-body radiation
  • einstein’s work on the photoelectric effect and stimulated emission
  • semiconductor p-n junction theory
  • thermodynamics principles, particularly the second law

Applications

  • benchmark for single-junction solar cell performance
  • design of multi-junction solar cells to overcome the limit
  • research into hot-carrier and upconversion/downconversion solar cells
  • economic modeling of solar energy costs

Patents:

NA

Potential Innovations Ideas

  • solar cells using quantum dots with tunable bandgaps to perfectly match the sq peak
  • thermo-photovoltaic systems that convert waste heat back into narrow-band light for a matched solar cell
  • dynamic bandgap materials that adjust to changing solar spectrum throughout the day
  • luminescent solar concentrators that shift uv light to the optimal sq wavelength
  • photonic crystal designs that enhance absorption just above the bandgap while rejecting sub-bandgap photons
  • hybrid solar cells that use hot-carrier extraction for high-energy photons and a standard p-n junction for lower-energy ones
  • metamaterials that angularly restrict cell emission to reduce radiative recombination losses
  • ai-driven discovery of new semiconductor alloys with ideal sq bandgaps and material properties
Related to: shockley-queisser limit, solar cell efficiency, thermodynamic limit, radiative recombination, bandgap, detailed balance, single-junction, black-body radiation.

Historical Context

Shockley–Queisser Limit

1960
1960
1960
1961
1962
1963
1965
1960
1960
1960
1960-05-16
1962
1963
1964
1968

(if date is unknown or not relevant, e.g. "fluid mechanics", a rounded estimation of its notable emergence is provided)

10th year anniversary

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