2015
DOI: 10.1002/pssr.201510081
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On the assessment of CIGS surface passivation by photoluminescence

Abstract: An optimized test structure to study rear surface passivation in Cu(In,Ga)Se2 (CIGS) solar cells by means of photoluminescence (PL) is developed and tested. The structure – illustrated in the abstract figure – is examined from the rear side. To enable such rear PL assessment, a semi‐transparent ultra‐thin Mo layer has been developed and integrated in place of the normal rear contact. The main advantages of this approach are (i) a simplified representation of a rear surface passivated CIGS solar cell is possibl… Show more

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Cited by 19 publications
(15 citation statements)
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“…Broad emission is typical of Cu-poor CIGS polycrystalline solar cells, [59][60][61] however, for the case of the reference solar cell, the luminescence is significantly broader than that of the passivated cell. [64][65][66][67][68] However, a direct comparison of PL intensity from different samples should be done with caution due to the necessarily different optical alignments despite nominally equivalent experimental conditions and as in this work we do not have those capabilities and we do not perform that comparison here. [62,63] Regarding the passivated solar cell, the full width at half maximum (FWHM) is significantly lower (≈61 meV) than that of the reference solar cell (≈96 meV).…”
Section: Photoluminescencementioning
confidence: 99%
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“…Broad emission is typical of Cu-poor CIGS polycrystalline solar cells, [59][60][61] however, for the case of the reference solar cell, the luminescence is significantly broader than that of the passivated cell. [64][65][66][67][68] However, a direct comparison of PL intensity from different samples should be done with caution due to the necessarily different optical alignments despite nominally equivalent experimental conditions and as in this work we do not have those capabilities and we do not perform that comparison here. [62,63] Regarding the passivated solar cell, the full width at half maximum (FWHM) is significantly lower (≈61 meV) than that of the reference solar cell (≈96 meV).…”
Section: Photoluminescencementioning
confidence: 99%
“…In the literature, in addition to the shape of the PL emission at low temperature, to infer the effect of the passivation layer, quite often a comparison of the PL intensity is performed. [64][65][66][67][68] However, a direct comparison of PL intensity from different samples should be done with caution due to the necessarily different optical alignments despite nominally equivalent experimental conditions and as in this work we do not have those capabilities and we do not perform that comparison here. With the used excitation wavelength, 514.5 nm, penetration depth of the incident photons, ≈70 nm, is smaller than the CIGS thickness, 350 nm.…”
Section: Photoluminescencementioning
confidence: 99%
“…7 by means of photoluminescence (PL) measurements, where an elevated PL intensity by one order of magnitude was seen for passivated CIGS absorbers compared to unpassivated absorbers (i.e. no Al2O3 passivation layer) [30]. Such an improvement in cell performance can be attributed to (i) reduced recombination at the CIGS/Mo-back contact (i.e.…”
Section: Introductionmentioning
confidence: 99%
“…Various research groups have shown that Al2O3 is very suitable to passivate the rear of Cu(In,Ga)Se2 (CIGS) thin film solar cells, which can be explained by a combination of chemical and field effect passivation. Opto-electrical measurements can be used to screen interesting passivation layers, as is shown for Al2O3 grown on CIGS [3]. Even more, electrical measurements of similar structures show that the Al2O3 layers exhibit a high density of negative fixed charges (its field effect passivation) in combination with a reasonably low interface trap density (its chemical passivation) [4].…”
Section: Rear Surface Passivation Schemes For Cigsmentioning
confidence: 99%