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 E02: Condensed Matter Physics I
4:15 PM–5:15 PM,
Friday, October 19, 2018
Science and Engineering Classroom (SEC)
Room: 102
Chair: Oomman Varghese, University of Houston
Abstract ID: BAPS.2018.TSF.E02.3
Abstract: E02.00003 : Ultrafast nonlinear optical processes in CH3NH3PbI3 hybrid perovskite*
4:39 PM–4:51 PM
Presenter:
Alex Zakhidov
(Texas State Univ-San Marcos)
Authors:
Alex Zakhidov
(Texas State Univ-San Marcos)
Eric Welch
(Texas State Univ-San Marcos)
Mehedhi Hasan
(Texas State Univ-San Marcos)
Dmitry Lyashenko
(Texas State Univ-San Marcos)
Petr Obraztsov
(A. M. Prokhorov General Physics Institute)
Methylammonium lead iodide (MAPI) is a benchmark hybrid organic perovskite material, which is used for the low-cost, printed solar cells with over 23% power conversion efficiency. Yet, the nature of light-matter interaction in MAPI as well as the exact physical mechanism behind device operation is currently debated. Here we report room temperature, ultrafast photocurrent and free-space terahertz (THz) emission generation from unbiased MAPI thin films induced by 150 fs light pulses1. Polarization dependence of the observed photocurrents is consistent with the Bulk Photovoltaic Effect (BPVE) caused by a combination of injection and shift currents. We believe that this observation of can shed light on low recombination, and long carrier diffusion lengths due to indirect bandgap. Moreover, ballistic by nature shift and injection BPVE photocurrents may enable third generation perovskite solar cells with efficiency that exceed the Shockley–Queisser limit. Our observations also open new venues for perovskite spintronics and tunable THz sources.
[1]. P.A. Obraztsov, et al., Comm. Physics 1, 14 (2018).
*We thank NSF(#1721884, Dr. Anna Brady-Estevez), ACS PRF (#UNI656095-UNI6, Dr. AskarFahr), and ONR (#W911NF-16-1-0518, Dr. Paul Armistead) for partial support of this work.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.TSF.E02.3
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