High-frequency gravitational waves detection with the BabyIAXO haloscopes

José Reina Valero, Jose R. Navarro Madrid, Diego Blas, Alejandro Díaz Morcillo, Igor García Irastorza, Benito Gimeno, Juan Monzó Cabrera
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Abstract

We present the first analysis using RADES-BabyIAXO cavities as detectors of high-frequency gravitational waves (HFGWs). In particular, we discuss two configurations for distinct frequency ranges of HFGWs: Cavity 1, mostly sensitive at a frequency range of 252.8 - 333.2 MHz, and Cavity 2, at 2.504 - 3.402 GHz, which is a scaled down version of Cavity 1. We find that Cavity 1 will reach sensitivity to strains of the HFGWs of order $h_1\sim 10^{-21}$, while Cavity 2 will reach $h_2\sim 10^{-20}$. These represent the best estimations of the RADES-BabyIAXO cavities as HFGWs detectors, showing how this set-up can produce groundbreaking results in axion physics and HFGWs simultaneously.
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利用 BabyIAXO 光镜进行高频引力波探测
我们首次分析了使用 RADES-BabyIAXO 腔作为高频引力波(HFGW)探测器的情况。我们特别讨论了针对不同频率范围的高频引力波的两种配置:腔体 1(对 252.8 - 333.2 MHz 频率范围最为敏感)和腔体 2(对 2.504 - 3.402 GHz 频率范围最为敏感),后者是腔体 1 的缩小版。我们发现,腔体 1 对 HFGW 应变的灵敏度将达到 $h_1\sim 10^{-21}$,而腔体 2 将达到 $h_2\sim 10^{-20}$。这代表了RADES-BabyIAXO空腔作为HFGW探测器的最佳估计值,显示了这种设置如何能够同时在轴子物理和HFGW方面产生突破性的结果。
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