Efficiency limits of quantum well solar cells

Physics – Condensed Matter – Mesoscale and Nanoscale Physics

Scientific paper

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Preprint for submission to the 19th EUPVSC, Paris, France, 2004, 4 pages pp. 355-359

Scientific paper

The quantum well solar cell (QWSC) has been proposed as a flexible means to ensuring current matching for tandem cells. This paper explores the further advantage afforded by the indication that QWSCs operate in the radiative limit because radiative contribution to the dark current is seen to dominate in experimental data at biases corresponding to operation under concentration. The dark currents of QWSCs are analysed in terms of a light and dark current model. The model calculates the spectral response (QE) from field bearing regions and charge neutral layers and from the quantum wells by calculating the confined densities of states and absorption coefficient, and solving transport equations analytically. The total dark current is expressed as the sum of depletion layer and charge neutral radiative and non radiative currents consistent with parameter values extracted from QE fits to data. The depletion layer dark current is a sum of Shockley-Read-Hall non radiative, and radiative contributions. The charge neutral region contribution is expressed in terms of the ideal Shockley radiative and non-radiative currents modified to include surface recombination. This analysis shows that the QWSC is inherently subject to the fundamental radiative efficiency limit at high currents where the radiative dark current dominates, whereas good homojunction cells are well described by the ideal Shockley picture where the limit is determined by radiative and non radiative recombination in the charge neutral layers of the cell.

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