Optoelectronic Properties of Halide Perovskites with ab Initio Many-body Perturbation Theory
Linn Leppert a
a Institute of Physics, University of Bayreuth, Germany, Bayreuth, Germany
Materials for Sustainable Development Conference (MATSUS)
Proceedings of nanoGe Fall Meeting19 (NFM19)
#PERFuDe19. Halide perovskites: when theory meets experiment from fundamentals to devices
Berlin, Germany, 2019 November 3rd - 8th
Organizers: Claudine Katan, Wolfgang Tress and Simone Meloni
Oral, Linn Leppert, presentation 074
DOI: https://doi.org/10.29363/nanoge.nfm.2019.074
Publication date: 18th July 2019

Halide perovskites are a broad class of compounds featuring 3D materials like the hybrid organic-inorganic CH3NH3PbI3 and the all-inorganic double perovskite Cs2BiAgBr6, 2D layered Ruddlesden-Popper perovskites [1], quasi-0D materials like Cs3Bi2I9, and many more. They have shown great promise for photovoltaic applications with power conversion efficiencies of perovskite-based solar cells exceeding 23%. Accurately predicting their fundamental band gaps and excited state properties is challenging for first principles electronic structure methods because of the intricate coupling of structural and electronic degrees of freedom [2, 3], strong spin-orbit interactions, and the existence of strongly bound excitons in low-dimensional systems. In this contribution, I will discuss our recent progress in describing the optoelectronic properties of halide perovskites using Green’s function-based many-body perturbation theory. We investigate the predictive power of “one-shot” G0W0 calculations, with a focus on the impact of the density functional theory starting point, pseudopotentials, eigenvalue self-consistency, and the perovskite structure [4].  With our calculations, we assess whether there might be a “one size fits all” one-shot GW approach for this material class. Our findings have severe repercussions for the calculation of complex doped and defected systems [5], as well as for the calculation of excited states and exciton binding energies.

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