Fundamental and practical efficiency limits of selenium solar cells under outdoor and indoor illumination

Selenium (Se), particularly its trigonal phase, offers a wide-bandgap platform for outdoor and indoor photovoltaics. This work quantifies its spectrum-dependent efficiency limits using reciprocal optical absorption, radiative and nonradiative recombination, finite thickness, and electrical resistance, with separate module-temperature and degradation sensitivities. At a bandgap of 1.85 eV and 300 K, the one-sun air mass 1.5 global Shockley–Queisser limit is 26.10%; the nominal 500-lux limits are 52.86% for a white light-emitting diode (LED) and 53.16% for a compact fluorescent lamp. A representative experimental absorption spectrum gives one-micrometer-thick planar and textured radiative limits of 26.71% and 28.00%, respectively. A non-unique calibration reproduces three independent performance metrics of the certified 10.3% device. Parameter-conditioned advanced-target and practical-limit scenarios give 20.5%–26.9% outdoors and 26.5%–42.2% under the LED spectrum. These are isothermal, external-response-conditioned results, not forecasts of device performance. The full Shockley–Read–Hall expression and finite-doping calculations distinguish low-injection behavior from the intrinsic baseline. The radiative and recombination maps assume spatially uniform carrier densities and quasi-Fermi-level splitting through the absorber, together with complete extraction unless an empirical external-response factor is stated; they are zero-dimensional optical-recombination limits rather than drift–diffusion predictions for low-mobility Se films. Temperature-dependent optical-edge shifts are treated as illustrative sensitivities rather than calibrated material parameters. An ideal sub-bandgap reflector can reject 56.3% of incident solar power if an opaque module would otherwise absorb it, compared with only 1.30% under the modeled LED. The analysis identifies distinct outdoor and indoor priorities in absorption-edge quality, recombination, carrier extraction, leakage, and rear-stack optics, and provides reproducible parameter maps for interpreting future Se measurements.

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Publication Details

Journal
Journal of Applied Physics
Published
2026-11-11
DOI
https://doi.org/10.1063/5.0356816
Primary Topic
Chalcogenide Semiconductor Thin Films
Type
article
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article

Fundamental and practical efficiency limits of selenium solar cells under outdoor and indoor illumination

Seungwoo Lee
Journal of Applied Physics
Chalcogenide Semiconductor Thin Films
article

Fundamental and practical efficiency limits of selenium solar cells under outdoor and indoor illumination

Seungwoo Lee
article en

Abstract

Selenium (Se), particularly its trigonal phase, offers a wide-bandgap platform for outdoor and indoor photovoltaics. This work quantifies its spectrum-dependent efficiency limits using reciprocal optical absorption, radiative and nonradiative recombination, finite thickness, and electrical resistance, with separate module-temperature and degradation sensitivities. At a bandgap of 1.85 eV and 300 K, the one-sun air mass 1.5 global Shockley–Queisser limit is 26.10%; the nominal 500-lux limits are 52.86% for a white light-emitting diode (LED) and 53.16% for a compact fluorescent lamp. A representative experimental absorption spectrum gives one-micrometer-thick planar and textured radiative limits of 26.71% and 28.00%, respectively. A non-unique calibration reproduces three independent performance metrics of the certified 10.3% device. Parameter-conditioned advanced-target and practical-limit scenarios give 20.5%–26.9% outdoors and 26.5%–42.2% under the LED spectrum. These are isothermal, external-response-conditioned results, not forecasts of device performance. The full Shockley–Read–Hall expression and finite-doping calculations distinguish low-injection behavior from the intrinsic baseline. The radiative and recombination maps assume spatially uniform carrier densities and quasi-Fermi-level splitting through the absorber, together with complete extraction unless an empirical external-response factor is stated; they are zero-dimensional optical-recombination limits rather than drift–diffusion predictions for low-mobility Se films. Temperature-dependent optical-edge shifts are treated as illustrative sensitivities rather than calibrated material parameters. An ideal sub-bandgap reflector can reject 56.3% of incident solar power if an opaque module would otherwise absorb it, compared with only 1.30% under the modeled LED. The analysis identifies distinct outdoor and indoor priorities in absorption-edge quality, recombination, carrier extraction, leakage, and rear-stack optics, and provides reproducible parameter maps for interpreting future Se measurements.

Journal of Applied PhysicsVol. 140(18)
Korea University (KR)
Chalcogenide Semiconductor Thin Films
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