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  2. Shockley–Queisser limit - Wikipedia

    en.wikipedia.org/wiki/ShockleyQueisser_limit

    The Shockley–Queisser limit for the efficiency of a solar cell, without concentration of solar radiation. The curve is wiggly because of absorption bands in the atmosphere. In the original paper, [1] the solar spectrum was approximated by a smooth curve, the 6000K blackbody spectrum. As a result, the efficiency graph was smooth and the values ...

  3. Thermodynamic efficiency limit - Wikipedia

    en.wikipedia.org/wiki/Thermodynamic_efficiency_limit

    The Shockley-Queisser limit for the efficiency of a single-junction solar cell under unconcentrated sunlight. This calculated curve uses actual solar spectrum data, and therefore the curve is wiggly from IR absorption bands in the atmosphere. This efficiency limit of about 34% can be exceeded by multijunction solar cells.

  4. Intermediate band photovoltaics - Wikipedia

    en.wikipedia.org/wiki/Intermediate_band...

    They assumed no carriers were collected at the IB and that the device was under full concentration. [1] They found the maximum efficiency to be 63.2%, for a bandgap of 1.95eV with the IB 0.71eV from either the valence or conduction band. [1] Under one sun illumination the limiting efficiency is 47%. [2]

  5. Multiple exciton generation - Wikipedia

    en.wikipedia.org/wiki/Multiple_exciton_generation

    Breakdown of the causes for the Shockley-Queisser limit. The black height is Shockley-Queisser limit for the maximum energy that can be extracted as useful electrical power in a conventional solar cell. However, a multiple-exciton-generation solar cell can also use some of the energy in the green area (and to a lesser extent the blue area ...

  6. Solar-cell efficiency - Wikipedia

    en.wikipedia.org/wiki/Solar-cell_efficiency

    The Shockley–Queisser limit for the efficiency of a single-junction solar cell under unconcentrated sunlight at 273 K. This calculated curve uses actual solar spectrum data, and therefore the curve is wiggly from IR absorption bands in the atmosphere. This efficiency limit of ~34% can be exceeded by multijunction solar cells.

  7. Perovskite solar cell - Wikipedia

    en.wikipedia.org/wiki/Perovskite_solar_cell

    The Shockley–Queisser limit radiative efficiency limit, also known as the detailed balance limit, [105] [106] is about 31% under an AM1.5G solar spectrum at 1000 W/m 2, for a Perovskite bandgap of 1.55 eV. [107] This is slightly smaller than the radiative limit of gallium arsenide of bandgap 1.42 eV which can reach a radiative efficiency of 33%.

  8. Shockley diode equation - Wikipedia

    en.wikipedia.org/wiki/Shockley_diode_equation

    Later he gives a corresponding equation for current as a function of voltage under additional assumptions, which is the equation we call the Shockley ideal diode equation. [3] He calls it "a theoretical rectification formula giving the maximum rectification", with a footnote referencing a paper by Carl Wagner , Physikalische Zeitschrift 32 , pp ...

  9. Talk:Shockley–Queisser limit - Wikipedia

    en.wikipedia.org/wiki/Talk:ShockleyQueisser_limit

    The rottenness of their methodology is proven beyond a doubt by the fact that they claim a quantum efficiency of 18 (Fig. 3c), which is completely impossible under these circumstances (with photon energy a bit higher than the bandgap, the limit is 1 under normal circumstances or maybe 2 or 3 if there are exotic intermediate energy bands).

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