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  2. Shockley–Queisser limit - Wikipedia

    en.wikipedia.org/wiki/ShockleyQueisser_limit

    The ShockleyQueisser 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. Solar-cell efficiency - Wikipedia

    en.wikipedia.org/wiki/Solar-cell_efficiency

    The ShockleyQueisser 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.

  5. Talk:Shockley–Queisser limit - Wikipedia

    en.wikipedia.org/wiki/Talk:ShockleyQueisser_limit

    The numbers are normally not similar as you suggest. But in any case, f c cannot be more than 1, and the upper limit (the Shockley-Queisser limit) requires taking f c = 1. Eric Kvaalen 19:05, 6 September 2016 (UTC) Yes, virtually all above-gap photons come from recombination, but not all recombinations create above-bandgap photons.

  6. Perovskite solar cell - Wikipedia

    en.wikipedia.org/wiki/Perovskite_solar_cell

    The ShockleyQueisser 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%.

  7. Third-generation photovoltaic cell - Wikipedia

    en.wikipedia.org/wiki/Third-generation...

    Third-generation photovoltaic cells are solar cells that are potentially able to overcome the ShockleyQueisser limit of 31–41% power efficiency for single bandgap solar cells. This includes a range of alternatives to cells made of semiconducting p-n junctions ("first generation") and thin film cells ("second generation").

  8. Dye-sensitized solar cell - Wikipedia

    en.wikipedia.org/wiki/Dye-sensitized_solar_cell

    The high conversion efficiency of the cell was sustained after heating for 1,000 h at 80 °C, maintaining 94% of its initial value. After accelerated testing in a solar simulator for 1,000 h of light-soaking at 55 °C (100 mW cm −2) the efficiency had decreased by less than 5% for cells covered with an ultraviolet absorbing polymer film ...

  9. File:ShockleyQueisserVOC.svg - Wikipedia

    en.wikipedia.org/wiki/File:ShockleyQueisserVOC.svg

    English: Black curve: The limit for the maximum open-circuit current of a solar cell within the Shockley-Queisser model. The x-axis is the bandgap of the solar cell in electron volts, the y-axis is the highest possible open-circuit voltage in volts.

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