| Literature DB >> 32937784 |
Zhetao Xia1, Chenxi Zhang1, Zhiying Feng1, Zhixing Wu1, Zengbo Wang2, Xiaohong Chen1, Sumei Huang1.
Abstract
We report new structured perovskite solar cells (PSCs) using solution-processedEntities:
Keywords: Au nanorods; MgO passivation layer; longitudinal plasmon resonance; perovskite solar cells; plasmon enhancement; transverse plasmon resonance
Year: 2020 PMID: 32937784 PMCID: PMC7557864 DOI: 10.3390/nano10091830
Source DB: PubMed Journal: Nanomaterials (Basel) ISSN: 2079-4991 Impact factor: 5.076
Figure 1(a) J–V curves of perovskite solar cell (PSC) devices based on porous TiO2 without and with Au NRs and MgO coating. (b) FESEM image of as-deposited gold NRs. (c) Absorbance spectrum of Au NRs and Au spheres (about 20 nm in diameter) suspensions. (d) FESEM image of the top surface morphology of the porous TiO2 layer modified with Au NRs.
Photovoltaic parameters of the PSCs based on m-TiO2 with and without Au nanorods (NRs) and/or MgO.
| Parameters | FF | PCE (%) | ||
|---|---|---|---|---|
| Control | 1.02 | 20.10 | 0.72 | 14.7 |
| With pure Au NRs | 1.01 | 18.51 | 0.68 | 12.7 |
| With pure MgO | 1.04 | 21.30 | 0.74 | 16.4 |
| With Au NRs/MgO | 1.04 | 22.35 | 0.75 | 17.4 |
Figure 2UV–vis absorption of (a) p-TiO2 electron transport layers (ETLs) and (b) perovskite absorbers formed on porous TiO2 without and with Au NRs and MgO coating. (c) Steady-state photoluminescence (PL) spectra of perovskite absorbers without and with Au NRs and MgO coating.
Figure 3Nyquist plots of PSCs based on p-TiO2 without and with Au NRs and MgO overlayer under dark conditions at a 0.9 V applied bias.
Figure 4(a) External quantum efficiency (EQE) curves of the control (reference) device and the PSCs with Au NRs or MgO overlayer. (b) EQE enhancements of PSCs with Au NRs and MgO overlayer: EQE enhancement: ΔEQE/EQEref (ΔEQE, the difference between EQE values of the modified and the reference devices).
Figure 5(a–h) Simulated field |E| enhancement factor distribution around Au NR (40 nm in length and 11.6 nm in diameter) at different wavelengths, (i) color scale and (j) yz plane. The local field-enhancement factor distributions on yz planes at x = 0 nm. (k) Incident light beam propagation is along −z, and the light polarized direction.
Figure 6Calculated absorption (a) and scattering (b) cross-sections of an Au NR (40 nm in length and 11.6 nm in diameter) and sphere (20.06 nm in diameter) by a linear polarized plane wave in free space. The insert is the scattering diagram for the Au NR at a wavelength of 620 nm. (c) Maximal field intensity |E|2 enhancement factor around the Au NR at different wavelengths.