radiative efficiency limit → όριο ικανότητας ακτινοβόλησης, όριο ακτινοβολιακής ικανότητας
In physics, the radiative efficiency limit (also known as the detailed balance limit, Shockley–Queisser limit, Shockley Queisser Efficiency Limit or SQ Limit) is the maximum theoretical efficiency of a solar cell using a single p-n junction to collect power from the cell where the only loss mechanism is radiative recombination in the solar cell. It was first calculated by William Shockley and Hans-Joachim Queisser at Shockley Semiconductor in 1961, giving a maximum efficiency of 30% at 1.1 eV. The limit is one of the most fundamental to solar energy production with photovoltaic cells, and is considered to be one of the most important contributions in the field.
Shockley–Queisser limit - WikipediaWilliam Shockley pronunciation: How to pronounce William Shockley in EnglishPronunciations for Queisser