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用于染料敏化太阳能电池的D-π-A有机染料的π间隔基效应的理论研究:一项密度泛函理论(DFT)和含时密度泛函理论(TD-BHandH)研究

Theoretical investigation on π-spacer effect of the D-π-A organic dyes for dye-sensitized solar cell applications: a DFT and TD-BHandH study.

作者信息

El Mzioui Souad, Bouzzine Si Mohamed, Sidir İsa, Bouachrine Mohammed, Bennani Mohamed Naciri, Bourass Mohamed, Hamidi Mohamed

机构信息

Equipe d'Electrochimie et Environnement, Faculté des Sciences et Techniques, Université Moulay Ismaîl, Errachidia, Morocco.

Centre Régional des Métiers d'Education et de la formation, BP 8, Errachidia, Morocco.

出版信息

J Mol Model. 2019 Mar 9;25(4):92. doi: 10.1007/s00894-019-3963-1.

Abstract

In this paper, we present a series of sensitizers to shed light on the influence of π-spacers on the performance of dye-sensitized solar cells. We have accurately calculated key properties in energy conversion, including sunlight absorption, electron injection, electron/hole reorganization energy, ionization potential (IP) and electronic affinity (EA). We chose a series of donor-π-acceptor dyes based on methyl-indole-carbazole as the electron donor group and cyano-acrylic acid as an acceptor with various π-conjugated systems. The results obtained show that, with incorporation of the thieno(3,4-b)pyrazine in the two π-spacer parts, D4 may be the best candidate among the dyes studied, due to its many advantages such as low gap energy, red-shift absorption spectra, large ΔG, low hole/electron reorganization energies, low IP and high EA, which indicate its better optoelectronic properties, which present more balanced transport rates and provide good injection ability. Graphical abstract Absorption spectra in gaz phase, obtained by CAM-B3LYP/6-31G(d,p) with solar spectrum.

摘要

在本文中,我们展示了一系列敏化剂,以阐明π间隔基对染料敏化太阳能电池性能的影响。我们精确计算了能量转换中的关键性质,包括太阳光吸收、电子注入、电子/空穴重组能、电离势(IP)和电子亲和势(EA)。我们选择了一系列基于甲基吲哚咔唑作为电子供体基团和氰基丙烯酸作为受体且具有各种π共轭体系的供体-π-受体染料。所得结果表明,由于D4具有诸如低能隙、红移吸收光谱、大的ΔG、低的空穴/电子重组能、低IP和高EA等诸多优点,在两个π间隔基部分引入噻吩并[3,4-b]吡嗪后,D4可能是所研究染料中的最佳候选者,这些优点表明其具有更好的光电性质,呈现出更平衡的传输速率并具有良好的注入能力。图形摘要 通过CAM-B3LYP/6-31G(d,p)方法结合太阳光谱获得的气相吸收光谱。

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