Transport Limitations and Defect-Mediated Recombination in Lead- Free Double Perovskite Cs₂AgSbI₆: Implications for Solar-Cell Design

Read the full article See related articles

Discuss this preprint

Start a discussion What are Sciety discussions?

Listed in

This article is not in any list yet, why not save it to one of your lists.
Log in to save this article

Abstract

Even though the defect-mediated recombination severely limits the photovoltaic performance of lead-free double perovskites, they have become a promising alternative to Pb-based absorbers. The transport mechanisms and the optoelectronic properties of Cs₂AgSbI₆ are systematically investigated in this work by combining impedance analysis, electrical transport, photoluminescence and optical spectroscopy. A highly disordered electronic structure dominated by nonradiative recombination is shown through a non-ideal charge transport, a strong photoluminescence quenching and a large Urbach energy (~ 90 meV). Based on SCAPS-1D, numerical simulations are carried out using a representative FTO/TiO₂/Cs₂AgSbI₆/Spiro-OMeTAD architecture in order to translate the experimentally observed limitations into a device-level framework. The Shockley–Read–Hall (SRH) recombination is consistently identified by the simulations as the dominant loss pathway, which results in limited photovoltaic parameters and reduced quasi-Fermi level splitting. Defect density is emphasized as the primary bottleneck in Cs₂AgSbI₆-based devices through the strong agreement between numerical trends and experimental material signatures. These results not only offer clear guidelines for defect mitigation strategies towards improved lead-free perovskite solar cells but also provide device-relevant losses, recombination and a coherent physical picture linking disorder.

Article activity feed