Abstract
Cs2AgBiBr6 is an emerging double perovskite semiconductor with robust stability. However, its potential for photovoltaics is limited by its indirect band gap and localized electronic structure featuring a resonant exciton with a large binding energy. Cs2AgBi(IxBr1-x)6 nanocrystals with iodide concentrations of up to 100% were recently demonstrated, but an atomistic understanding of how halide mixing affects the electronic and excited-state structure is missing. Here, we use first-principles GW and Bethe-Salpeter Equation calculations to show that halide mixing leads to a pronounced change in the band gap and character of optical excitations. Exciton binding energies are reduced by up to a factor of 5, with significantly more delocalized excitons in I-rich compounds. We further show that phase-pure bulk alloys with x ≤ 0.11 can be fabricated using mechanosynthesis and measure a red-shifted absorption in line with our calculations. Our study highlights that halide mixing in double perovskites can not only lead to significant band gap changes but may also be used for tuning excitonic properties.
| Original language | English |
|---|---|
| Pages (from-to) | 14767-14775 |
| Number of pages | 9 |
| Journal | Journal of Physical Chemistry C |
| Volume | 128 |
| Issue number | 35 |
| Early online date | 13 Aug 2024 |
| DOIs | |
| Publication status | Published - 2024 |
Bibliographical note
Publisher Copyright:© 2024 The Authors. Published by American Chemical Society.
Funding
L.L. acknowledges funding by the Dutch Research Council (NWO) through the grants OCENW.M20.337 and VI.Vidi.223.072. H.J.J. and E.M.H. are supported by the Advanced Research Center Chemical Building Blocks Consortium (ARC CBBC). This work was also supported by the NWO Domain Science for the use of supercomputing facilities.
| Funders | Funder number |
|---|---|
| Australian Research Council | |
| Advanced Research Center Chemical Building Blocks Consortium | |
| Nederlandse Organisatie voor Wetenschappelijk Onderzoek | OCENW.M20.337, VI.Vidi.223.072 |