Point Defect Impact on the Electronic Structure of Perovskite CH3NH3PbI3 from Fist Principles Quantum Calculations
Gregorio García a b, Perla Wahnón a b, Pablo Palacios a c, Eduardo Menendez-Proupin d, Ana Montejo-Alejo d, José Carlos Conesa e
a Universidad Politécnica de Madrid, Avenidad Complutense s/n, Madrid, 28040
b Instituto de Energía Solar, E.T.S.I. Telecomunicación, Universidad Politécnica de Madrid, Avenidad Complutense s/n, Madrid, 28040
c Dept. FAIAN, E.T.S.I. Aeronáutica y del Espacio, Avenidad Complutense s/n, Madrid, 28040
d Departamento de Física, Facultad de Ciencias, Universidad de Chile, Las Palmeras 3425, 780-0003 Ñuñoa, Santiago, Chile
e Instituto de Catálisis y Petroleoquímica, CSIC, Marie Curie 2, Madrid, 28049, Spain
nanoGe Perovskite Conferences
Proceedings of Perovskite Thin Film Photovoltaics (ABXPV17)
València, Spain, 2017 March 1st - 2nd
Organizers: Henk Bolink and David Cahen
Poster, Gregorio García, 081
Publication date: 18th December 2016

Organic-inorganic lead halide perovskites (mainly CH3NH3PbI3) are being extensively studied because their excellent photovoltaic properties, such as suitable bandgap, high optical absorption and long carrier lifetime. To improve their photovoltaic performance, it is important to understand the impact of point defects on their electronic structure. In this work, we report the electronic structure of new CH3NH3PbI3 perovskite derivatives, in which deep defects were obtained by replacing Pb+2 atoms. To deal with the bandgap underestimation problem of common DFT methods, quasiparticle calculations have been applied via the G0W0 approximation. Bandgap value based on GW has considerably improved theoretical results compared to experimental one for the native perovskite. The investigation of the electronic structure of new CH3NH3PbI3 perovskites suggests that the presence of point defects play an important role in the coupling of two low energy photons to achieve a higher energy electron excitation (like in the Z-scheme of photosynthesis), which would maximize the photovoltaic performance.

Acknowledgements. This work was partially supported by the Comunidad de Madrid project MADRID-PV (S2013/MAE/2780) and by the Ministerio de Economía y Competitividad through the project BOOSTER (ENE2013-46624-C4-2-R). The authors acknowledge the computer resources and technical assistance provided by the Centro de Supercomputación and Visualización de Madrid (CeSViMa).



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