<?xml version="1.0"?>
<metadata xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:dc="http://purl.org/dc/elements/1.1/"><dc:title>Performance of triple-cation perovskite solar cells under different indoor operating conditions</dc:title><dc:creator>Jošt,	Marko	(Avtor)
	</dc:creator><dc:creator>Ajdič,	Žan	(Avtor)
	</dc:creator><dc:creator>Topič,	Marko	(Avtor)
	</dc:creator><dc:subject>photovoltaics</dc:subject><dc:subject>perovskite solar cells</dc:subject><dc:subject>indoor operation</dc:subject><dc:subject>LED light sources</dc:subject><dc:subject>detailed balance limit</dc:subject><dc:subject>bandgap tuning</dc:subject><dc:subject>stability</dc:subject><dc:subject>diodes</dc:subject><dc:subject>electrical conductivity</dc:subject><dc:subject>power conversion efficiency</dc:subject><dc:subject>solar cells</dc:subject><dc:description>We systematically analyze triple-cation perovskite solar cells for indoor applications. A large number of devices with different bandgaps from 1.6 to 1.77 eV were fabricated, and their performance under 1-sun AM1.5 and indoor white light emitting diode (LED) light was compared. We find that the trends agree well with the detailed balance limit; however, the devices near the optimal bandgap (1.77 eV) perform worse due to the lower perovskite quality. Instead, we achieve the highest power conversion efficiency (PCE) of 34.0% under 870 lx with 1.67 eV and Al$_2$O$_3$ passivation. The perovskite with a bandgap of 1.71 eV is not far behind, with a high $V_{OC}$ of 1.02 V. Measurements under different white LED color temperatures confirm that the highest PCE is achieved under the warmest colors. All measurements were carried out in a dedicated indoor setup that ensures the diffuse light typical of indoor environments and allows both short- and long-term measurements. In the best case, we observe no degradation during the 33-day test under simulated office conditions with regular switching on and off of the light and a $T_{80}$ of 30 days under continuous illumination. The results were obtained from multiple batches, which corroborates our findings and gives them statistical relevance.</dc:description><dc:date>2024</dc:date><dc:date>2024-11-18 12:31:12</dc:date><dc:type>Članek v reviji</dc:type><dc:identifier>164941</dc:identifier><dc:identifier>UDK: 621.383.51:549.641</dc:identifier><dc:identifier>ISSN pri članku: 1944-8252</dc:identifier><dc:identifier>DOI: 10.1021/acsami.4c14736</dc:identifier><dc:identifier>COBISS_ID: 215382531</dc:identifier><dc:language>sl</dc:language></metadata>
