Bulletin of the American Physical Society
2018 Joint Fall Meeting of the Texas Sections of APS, AAPT and Zone 13 of the SPS
Volume 63, Number 18
Friday–Saturday, October 19–20, 2018; University of Houston, Houston, Texas
Session G01: Poster Session
7:50 PM,
Friday, October 19, 2018
TDECU Football Stadium
Room: Club Suite
Chair: Donna Stokes, University of Houston
Abstract ID: BAPS.2018.TSF.G01.31
Abstract: G01.00031 : First Principle Polaron Modeling in Hybrid Perovskites Using the GGA+U Method*
Presenter:
Eric Welch
(Texas State University)
Authors:
Eric Welch
(Texas State University)
Amanda Neukirch
(Los Alamos National Lab)
Sergei Tretiak
(Los Alamos National Lab)
Petr Obraztsov
(A. M. Prokhorov General Physics Institute, University of Eastern Finland)
Dmitry Lyashenko
(Texas State University)
Pavel Chizhov
(A. M. Prokhorov General Physics Institute)
Kuniaki Konishi
(University of Tokyo)
Natsuki Nemoto
(University of Tokyo)
Makoto Kuwata-Gonokami
(University of Tokyo)
Alexander Obraztsov
(M.V. Lomonsov Moscow State University, A. M. Prokhorov General Physics Institute)
Alex Zakhidov
(Texas State University)
Lead halide hybrid perovskites (HPs) are the benchmark, state-of-the-art materials in third generation perovskite solar cells, achieving a power conversion efficiency of over 22%. Yet, the underlying photo-physical properties of HPs are still under debate. Here we use density functional theory within the generalized gradient approximation with a Hubbard correction (GGA+U) to study structural properties, band structures, and charge carrier dynamics in HPs. Our preliminary DFT+U simulations reveal the formation of hole polarons in HPs with different halides, which have profound implications on device operation and stability. Moreover, we argue that polaron induced loss of inversion symmetry and enhanced Rashba splitting might be responsible for our recent experimentally observed room-temperature ultrafast photocurrent and free-space terahertz emission generation from unbiased CH3NH3PbI3 HPs. Polarization dependence of the observed photoresponse is consistent with the Bulk Photovoltaic Effect, which may enable next generation perovskite solar cells with efficiency above the Shockley–Queisser limit.
*RSF #17-72-10303; The Academy of Finland Grants #299059,#318596; PFBR Grant #16-52-10062; The ACS PRFG #56095-UNI6; The U.S. DoD Contract W911NF-16-1-0518; JSPS; MEXT
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.TSF.G01.31
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