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arXiv 1506.02205cond-mat.mtrl-sci
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有机阳离子在CH3NH3PbI3过氧化物中的旋转动力学

Rotational Dynamics of Organic Cations in CH3NH3PbI3 Perovskite

T. Chen, B. J. Foley, B. Ipek, M. Tyagi, J. R. D. Copley, C. M. Brown, J. J. Choi, S. -H. Lee

摘要:

基于甲基铵碘化铅(CH 3 NH3 PbI 3)的太阳能电池已经显示出超过20%的令人印象深刻的功率转换效率。然而,高光伏性能的微观机制尚未完全理解。特别是,CH 3 NH3+阳离子的动力学及其对电荷复合和激子解离等相关过程的影响仍然知之甚少。在这里,使用弹性和准弹性中子散射技术和群论分析,我们研究了CH 3 NH3 PbI 3中CH 3 NH3+阳离子的转动模式。结果表明,在立方相(T > 327 K)和四方相(165 K < T <327 K)中,CH_3NH_3 ~+离子表现出C-N轴(C_4)的四重旋转对称性和C-N轴(C_3)的三重旋转对称性,而在正交相(T <165 K)中,只有C_3旋转对称性。在室温附近,发现C4旋转的特征弛豫时间为ps,而C3旋转的特征弛豫时间为ps。依赖的转动弛豫时间与Arkenius方程拟合,得到活化能。我们的数据表明,C4旋转模式和温度依赖的介电常数之间的密切相关性。我们的研究结果的旋转动力学的CH 3 NH3+和相关的偶极子理解低激子结合能和缓慢的电荷复合率CH 3 NH3 PbI 3这是直接相关的高太阳能电池的性能具有重要意义。

英文摘要:

Methylammonium lead iodide (CH3NH3PbI3) based solar cells have shown impressive power conversion efficiencies of above 20%. However, the microscopic mechanism of the high photovoltaic performance is yet to be fully understood. Particularly, the dynamics of CH3NH3+ cations and their impact on relevant processes such as charge recombination and exciton dissociation are still poorly understood. Here, using elastic and quasi-elastic neutron scattering techniques and group theoretical analysis, we studied rotational modes of the CH3NH3+ cation in CH3NH3PbI3. Our results show that, in the cubic (T > 327K) and tetragonal (165K < T < 327K) phases, the CH3NH3+ ions exhibit four-fold rotational symmetry of the C-N axis (C4) along with three-fold rotation around the C-N axis (C3), while in orthorhombic phase (T < 165K) only C3 rotation is present. Around room temperature, the characteristic relaxation times for the C4 rotation is found to be ps while for the C3 rotation ps. The -dependent rotational relaxation times were fitted with Arrhenius equations to obtain activation energies. Our data show a close correlation between the C4 rotational mode and the temperature dependent dielectric permittivity. Our findings on the rotational dynamics of CH3NH3+ and the associated dipole have important implications on understanding the low exciton binding energy and slow charge recombination rate in CH3NH3PbI3 which are directly relevant for the high solar cell performance.

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