4.8 Article

Chemically Localized Resonant Excitons in Silver-Pnictogen Halide Double Perovskites

Journal

JOURNAL OF PHYSICAL CHEMISTRY LETTERS
Volume 12, Issue 8, Pages 2057-2063

Publisher

AMER CHEMICAL SOC
DOI: 10.1021/acs.jpclett.0c03579

Keywords

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Funding

  1. Theory FWP at the Lawrence Berkeley National Laboratory - U.S. Department of Energy, Office of Science, Basic Energy Sciences, Materials Sciences and Engineering Division [DE-C02-05CH11231]
  2. Office of Science, Office of Basic Energy Sciences, of the US DOE [DE-AC02-5CH11231]
  3. Bavarian State Ministry of Science and the Arts through the Collaborative Research Network Solar Technologies go Hybrid (SolTech)
  4. Elite Network Bavaria
  5. German Research Foundation (DFG) [SFB840]
  6. DFG program [GRK1640]
  7. John Fell Oxford University Press (OUP) Research Fund

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Halide double perovskites with alternating silver and pnictogen cations are emerging photoabsorber materials with robust stability and band gaps in the visible range. Calculations show that these materials exhibit strongly localized resonant excitons, different from lead-based perovskites.
Halide double perovskites with alternating silver and pnictogen cations are an emerging family of photoabsorber materials with robust stability and band gaps in the visible range. However, the nature of optical excitations in these systems is not yet well understood, limiting their utility. Here, we use ab initio many-body perturbation theory within the GW approximation and the Bethe-Salpeter equation approach to calculate the electronic structure and optical excitations of the double perovskite series Cs2AgBX6, with B = Bi3+, Sb3+ and X = Br-, Cl-. We find that these materials exhibit strongly localized resonant excitons with energies from 170 to 434 meV below the direct band gap. In contrast to lead-based perovskites, the Cs2AgBX6 excitons are computed to be non-hydrogenic with anisotropic effective masses and sensitive to local field effects, a consequence of their chemical heterogeneity. Our calculations demonstrate the limitations of the Wannier-Mott and Elliott models for this class of double perovskites and contribute to a detailed atomistic understanding of their light-matter interactions.

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