实际的光子带隙结构用于高频轴向光镜.
D Goulart1, A M Sindhwad1, H M Jackson1
1Department of Nuclear Engineering, University of California, Berkeley, Berkeley, California 94720, USA.
The Review of scientific instruments
|September 8, 2025
概括
未来的暗物质动力搜索面临着5GHz以上的共振器设计的挑战. 一种新的光子带隙结构抑制了不需要的模式,使得在后膨胀的轴动质量范围内能够进行敏感的搜索.
科学领域:
- 实验物理学的实验物理.
- 粒子天体物理学 粒子天体物理学
- 光子学是指光子学的使用方法.
背景情况:
- 搜索暗物质轴子利用共振转换到磁场内的光子.
- 高频 (≥5 GHz) 共振器的设计受到横向电 (TE) 模式的扩散的阻碍.
- 这些TE模式干扰了所需的横向磁性 (TM010) 模式,使轴向检测复杂化.
研究的目的:
- 为了应对高频轴突检测共振器中TE模式扩散的挑战.
- 为了使可调节的共振器的设计,未来的暗物质轴子搜索.
- 探索新的共振器几何形状,以提高后膨胀轴动质量范围的灵敏度.
主要方法:
- 设计和模拟光子带隙 (PBG) 结构.
- 将PBG结构集成到一个圆形共振器几何结构中.
- 分析PBG结构对横向电 (TE) 和横向磁 (TM) 模式光谱的影响.
主要成果:
- 使用PBG结构,证明了TE模式频谱的完全抑制.
- 在最小的格子周期 (两个或一个) 中实现了TE模式抑制,偏离了完美的格子对称性.
- 允许在体积高效的圆形几何形状下设计可调节的共振器.
结论:
- 光子带隙结构为高频轴子探测器中TE模式扩散提供了可行的解决方案.
- 这种方法有助于开发灵敏,可调节的共振器,用于未来的暗物质动力搜索.
- 拟议的方法为有效地探索后膨胀轴的质量范围开辟了道路.
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