论文标题

沉积后退火和界面ALD ALD缓冲层SB $ _2 $ SE $ _3 $/CDS堆栈减少接口重组和增加的开路电压

Post-deposition annealing and interfacial ALD buffer layers of Sb$_2$Se$_3$/CdS stacks for reduced interface recombination and increased open-circuit voltages

论文作者

Weiss, Thomas Paul, Minguez-Bacho, Ignacio, Zuccalà, Elena, Melchiorre, Michele, Valle, Nathalie, Adib, Brahime El, Yokosawa, Tadahiro, Spiecker, Erdmann, Bachmann, Julien, Dale, Phillip J., Siebentritt, Susanne

论文摘要

目前,SB $ _2 $ SE $ _3 $薄膜作为太阳能电池吸收材料获得了相当大的研究兴趣。当完善设备堆栈中时,用于进一步改进设备的主要瓶颈是开路电压,这是此处介绍的工作的重点。多晶薄膜SB $ _2 $ SE $ _3 $吸收器和太阳能电池是在底物配置中制备的,并使用光致发光光谱和依赖温度依赖的电流 - 电气 - 电气振动特性研究了显性重组路径。发现在CDS缓冲层沉积后的沉积后退火可以有效地删除界面重组,因为主要重组路径的激活能量等于SB $ _2 $ _2 $ SE $ _3 $吸收器的带隙。增加的活化能伴随着增强的光致发光产量,即降低非辐射性重组。完成的SB $ _2 $ SE $ _3 $太阳能电池设备达到高达485 mV的开路电压。相反,这些设备的短路电流密度限制了沉积后退火后的效率。结果表明,原子层沉积了中间缓冲层,例如tio $ _2 $或sb $ _2 $ _2 $ se $ _3 $可以为克服此限制铺平道路。

Currently, Sb$_2$Se$_3$ thin films receive considerable research interest as a solar cell absorber material. When completed into a device stack, the major bottleneck for further device improvement is the open circuit voltage, which is the focus of the work presented here. Polycrystalline thin film Sb$_2$Se$_3$ absorbers and solar cells are prepared in substrate configuration and the dominant recombination path is studied using photoluminescence spectroscopy and temperature dependent current-voltage characteristics. It is found that a post-deposition annealing after the CdS buffer layer deposition can effectively remove interface recombination since the activation energy of the dominant recombination path becomes equal to the bandgap of the Sb$_2$Se$_3$ absorber. The increased activation energy is accompanied by an increased photoluminescence yield, i.e. reduced non-radiative recombination. Finished Sb$_2$Se$_3$ solar cell devices reach open circuit voltages as high as 485 mV. Contrarily, the short-circuit current density of these devices is limiting the efficiency after the post-deposition annealing. It is shown that atomic layer deposited intermediate buffer layers such as TiO$_2$ or Sb$_2$Se$_3$ can pave the way for overcoming this limitation.

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