用于轴心暗物质搜索的可调光子带隙谐振器

Samantha M. Lewis, Dillon T. Goulart, Mirelys Carcana Barbosa, Alexander F. Leder, Aarav M. Sindhwad, Isabella Urdinaran, Karl van Bibber
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引用次数: 0

摘要

轴子是一种动机明确的暗物质候选粒子。哈洛普旨在通过测量轴子与强磁场相互作用产生的光子信号来探测银河系晕中的轴子。现有的哈洛镜主要以轴子质量为目标,轴子质量会产生微波范围的光子,并依靠微波谐振器来增强信号功率。只有有限的谐振器模式子集对这一过程有用,而且目前的圆柱形腔受到其他基本模式的模式混合和排挤的影响。使用光子带隙(PBG)谐振器可以消除大部分这些模式。这些结构的带隙行为使谐振器具有基于频率的模式选择性。我们展示了首个可调谐 PBG 谐振器的研究成果,这是一种概念验证设计,其占地面积与轴子光镜兼容。我们对该结构的两个反转的调谐范围进行了全面鉴定,并报告了成功限制了工作中的 TM$_{010}$ 模式并消除了调谐范围内的所有 TE 模式。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
A tunable photonic band gap resonator for axion dark matter searches
Axions are a well-motivated dark matter candidate particle. Haloscopes aim to detect axions in the galactic halo by measuring the photon signal resulting from axions interacting with a strong magnetic field. Existing haloscopes are primarily targeting axion masses which produce microwave-range photons and rely on microwave resonators to enhance the signal power. Only a limited subset of resonator modes are useful for this process, and current cylindrical-style cavities suffer from mode mixing and crowding from other fundamental modes. The majority of these modes can be eliminated by using photonic band gap (PBG) resonators. The band gap behavior of these structures allows for a resonator with mode selectivity based on frequency. We present results from the first tunable PBG resonator, a proof-of-concept design with a footprint compatible with axion haloscopes. We have thoroughly characterized the tuning range of two versions of the structure and report the successful confinement of the operating TM$_{010}$ mode and the elimination of all TE modes within the tuning range.
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