About Photovoltaic cell efficiency limit
In physics, theradiative 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.
In a traditional such as , a solar cell is made from two doped crystals, one an , which has extra free .
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The Shockley–Queisser limit is calculated by examining the amount of electrical energy that is extracted per photon of incoming sunlight.
It is important to note that the analysis of Shockley and Queisser was based on the following assumptions:1. One electron–hole pair excited per incoming photon .
• , using thesoftware program. This code was used to calculate all the graphs in this article.• Luque, Antonio, and Antonio Martí. "Chapter 4: Theoretical Limits of Photovoltaic.
The factors affectingwere expounded in a landmark paper byandin 1961.See for more detail. If one has a source of heat at temperature Ts and cooler heat sink at temperature Tc, the maximum theoretically possible value for the ratio of wor. The maximum theoretical efficiency calculated is 86.8% for a stack of an infinite number of cells, using the incoming concentrated sunlight radiation. When the incoming radiation comes only from an area of the sky the size of the sun, the efficiency limit drops to 68.7%.
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