准周期近似数中的光子带间隙,考虑超均性
Nayuta Takemori1,2,3, Akiji Yamamoto4
1Department of Physics, Graduate School of Science, Osaka University, Toyonaka 560-0043, Japan.
概括
这项研究证实了正方形三角形和六边形船星 (HBS) 的完整光子带间隙. 引入二次气显著增加了这些差距,特别是在HBS结构中.
科学领域:
- 凝聚物质物理学 凝聚物质物理学
- 光子学 是一个光子学.
- 材料科学 材料科学 材料科学
背景情况:
- 二维半周期性板提供独特的结构性质.
- 光子带间隙对于控制光传播至关重要.
研究的目的:
- 调查阿曼-比肯,方形三角形和六角船星 (HBS) 的光子带隙特性.
- 探索增强这些频段间隙的方法.
主要方法:
- 平面波方法用于计算横向电 (TE) 和横向磁 (TM) 间隙.
- 对结构性特征的超均性的分析.
主要成果:
- 在正方形三角形和HBS地板上确认了完整的光子带间隙.
- HBS的板显示了第一个完整的缺口在一个10倍旋转对称的半周期结构.
- 二级气增强了带间隙,在阿曼 - 宾克中创造了一个小的间隙,并扩大了HBS间隙.
结论:
- 准周期结构,特别是HBS,可以表现出显著的光子带间隙.
- 高点密度和低结构复杂性是最佳带隙形成的关键.
- 这些发现使得更高效的光子装置设计成为可能.
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