I. G. Abdulsalam, A. K. Abubakar, M. Aliyu, S. R. Naidoo, A. Miller
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引用次数: 0
摘要
本文研究了银植入碳基薄膜(沉积在石英基底上)在 2.5 - 3.4 x 1016 离子/平方厘米范围内不同能量银离子通量下的光学响应。拉曼光谱用于观察 Ag:a-C 复合材料的微观结构特征。原子力显微镜(AFM)显示,在不同的通量下,薄膜的颗粒粒度和表面粗糙度显著增加。光学吸收光谱显示,原始银的表面等离子体共振(SPR)发生在约 428 纳米的可见光波长处,但在植入薄膜中却表现出蓝移(约 32 纳米)。经原子力显微镜证实,等离子体波长的蓝移是由于通量引起的银颗粒晶粒尺寸和密度的增加。原始碳膜的光带隙能()和厄巴赫参数()随着通量的增加分别从 2.89 eV 上升到 1.60 eV 和 3.60 eV 上升到 4.22 eV。观察到的光学活性参数有力地表明,这些复合材料是保留光子以提高太阳能电池效率的良好候选材料。
INVESTIGATION OF PHOTOVOLTAIC POTENTIALS OF A SILVER IMPLANTED DIAMOND-LIKE CARBON THIN FILM
This paper investigated the optical response of silver implanted carbon-based thin films (deposited on quartz substrates) due to varying fluence of energetic Ag ions in the range 2.5 - 3.4 x 1016 ions/cm2. Raman spectroscopy was used to observe the microstructural specifics of the Ag:a-C composites. Atomic force microscopy (AFM) revealed significant increase in particle grain size and surface roughness of the films at varying fluences. Optical absorption spectra showed that the Surface Plasmon Resonance (SPR) of pristine Ag occurs at visible wavelength of about 428 nm but exhibited a blue shifting (~ 32 nm) in the implanted films. The blue shift in plasmonic wavelength occurs due to the fluence-induced increase in grain size and density of the Ag particles as confirmed by AFM. Optical band gap energy () and Urbach parameter () of the pristine carbon film increased, with fluence, from 2.89 eV to 1.60 eV and 3.60 eV to 4.22 eV respectively. The observed optically active parameters strongly indicate that the composites would make good candidates for photon retention towards the enhancement of solar cells’ efficiency.