posted on 2020-06-30, 00:00authored byMichael C. Brennan
<p>Lead halide perovskite [APbX<sub>3</sub>; A=CH<sub>3</sub>NH<sub>3</sub><sup>+</sup>, CH(NH<sub>2</sub>)<sub>2</sub><sup>+</sup>, Cs<sup>+</sup>; X=Cl<sup>-</sup>, Br<sup>-</sup>, I<sup>-</sup>] thin films and colloidal nanocrystals (NCs) have taken a dominant position in the pursuit for next-generation photovoltaic and light-emitting devices. Improved knowledge of their fundamental properties and photostability are still required to realize large-scale commercialization. In particular, the origin of universally observed size-dependent Stokes shifts in perovskite NCs and the precise crystal structure assumed by CsPbBr<sub>3 </sub>NCs remain of fundamental interest. In terms of photostability, uniformly mixed halide perovskites [e.g., APb(I<sub>1-x</sub>Br<sub>x</sub>)<sub>3</sub>]<sub> </sub>thin films and NCs suffer dramatic changes to their underlying optical and structural properties during continuous visible or ultraviolet illumination. Elucidating the role played by defects (e.g. halide vacancies) as well as other photochemical processes (e.g. photoinduced I<sub>2</sub> sublimation) provides critical mechanistic insight into this phenomenon. Only by developing a truly comprehensive understanding of their fundamental properties and photostability can lead halide perovskites be successfully implemented into working devices.</p>
History
Date Modified
2020-07-17
Defense Date
2020-06-15
CIP Code
40.0501
Research Director(s)
Masaru Kuno
Committee Members
Marya Lieberman
Francesco Banfi
Luca Gavioli
Prashant Kamat