Excitation wavelength dependent interfacial charge transfer dynamics in a CH3NH3PbI3 perovskite film
(2018) In Journal of Photopolymer Science and Technology 31(5). p.633-642- Abstract
Elucidation of interfacial charge separation and recombination mechanisms is crucial to improve performance of organic-inorganic metal halide perovskite solar cells. Here, we have investigated influence of initially populated electron and hole potential levels in a perovskite conduction band (CB) and valence band (VB), respectively, by altering an excitation wavelength on interfacial charge separation and recombination dynamics in a CH3NH3PbI3 perovskite film sandwiched by a mesoporous TiO2 structure as an electron transport material (ETM) and a spiro-OMeTAD film as a hole transport material (HTM). Multi-phasic electron injection reactions are observed over <1.2 to several tens of... (More)
Elucidation of interfacial charge separation and recombination mechanisms is crucial to improve performance of organic-inorganic metal halide perovskite solar cells. Here, we have investigated influence of initially populated electron and hole potential levels in a perovskite conduction band (CB) and valence band (VB), respectively, by altering an excitation wavelength on interfacial charge separation and recombination dynamics in a CH3NH3PbI3 perovskite film sandwiched by a mesoporous TiO2 structure as an electron transport material (ETM) and a spiro-OMeTAD film as a hole transport material (HTM). Multi-phasic electron injection reactions are observed over <1.2 to several tens of nanoseconds, while most of holes are injected to a spiro-OMeTAD layer within the transient emission spectroscopy instrument response time (1.2 ns). In contrast, interfacial charge recombination rates are slower (from 5 ms to 1.3 s) with the increase of the excitation wavelength. These kinetics suggest that as long as low excitation intensity is employed, e.g. 10 nJ/cm2 or 1 sun (100 mW/cm2), the APCE of ~100% can be expected at any excitation wavelength for the solar cells based on FTO/c-TiO2/m-TiO2/MAPbI3/OMeTAD films.
(Less)
- author
- Liu, Maning
LU
; Endo, Masaru ; Shimazaki, Ai ; Wakamiya, Atsushi and Tachibana, Yasuhiro
- publishing date
- 2018
- type
- Contribution to journal
- publication status
- published
- subject
- keywords
- CHNHPbI perovskite film, Electron injection, Excitation wavelength dependence, Hole injection, Interfacial charge recombination
- in
- Journal of Photopolymer Science and Technology
- volume
- 31
- issue
- 5
- pages
- 10 pages
- publisher
- Tokai University
- external identifiers
-
- scopus:85053283083
- ISSN
- 0914-9244
- DOI
- 10.2494/photopolymer.31.633
- language
- English
- LU publication?
- no
- id
- 97915f78-7c73-41df-8063-8981f13d2367
- date added to LUP
- 2023-08-24 12:38:50
- date last changed
- 2023-08-28 10:48:57
@article{97915f78-7c73-41df-8063-8981f13d2367, abstract = {{<p>Elucidation of interfacial charge separation and recombination mechanisms is crucial to improve performance of organic-inorganic metal halide perovskite solar cells. Here, we have investigated influence of initially populated electron and hole potential levels in a perovskite conduction band (CB) and valence band (VB), respectively, by altering an excitation wavelength on interfacial charge separation and recombination dynamics in a CH<sub>3</sub>NH<sub>3</sub>PbI<sub>3</sub> perovskite film sandwiched by a mesoporous TiO<sub>2</sub> structure as an electron transport material (ETM) and a spiro-OMeTAD film as a hole transport material (HTM). Multi-phasic electron injection reactions are observed over <1.2 to several tens of nanoseconds, while most of holes are injected to a spiro-OMeTAD layer within the transient emission spectroscopy instrument response time (1.2 ns). In contrast, interfacial charge recombination rates are slower (from 5 ms to 1.3 s) with the increase of the excitation wavelength. These kinetics suggest that as long as low excitation intensity is employed, e.g. 10 nJ/cm<sup>2</sup> or 1 sun (100 mW/cm<sup>2</sup>), the APCE of ~100% can be expected at any excitation wavelength for the solar cells based on FTO/c-TiO<sub>2</sub>/m-TiO<sub>2</sub>/MAPbI<sub>3</sub>/OMeTAD films.</p>}}, author = {{Liu, Maning and Endo, Masaru and Shimazaki, Ai and Wakamiya, Atsushi and Tachibana, Yasuhiro}}, issn = {{0914-9244}}, keywords = {{CHNHPbI perovskite film; Electron injection; Excitation wavelength dependence; Hole injection; Interfacial charge recombination}}, language = {{eng}}, number = {{5}}, pages = {{633--642}}, publisher = {{Tokai University}}, series = {{Journal of Photopolymer Science and Technology}}, title = {{Excitation wavelength dependent interfacial charge transfer dynamics in a CH<sub>3</sub>NH<sub>3</sub>PbI<sub>3</sub> perovskite film}}, url = {{http://dx.doi.org/10.2494/photopolymer.31.633}}, doi = {{10.2494/photopolymer.31.633}}, volume = {{31}}, year = {{2018}}, }