High-frequency gravitational waves detection with the BabyIAXO haloscopes
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arXiv
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| Autores principales: | , , , , , , |
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| Formato: | Preprint |
| Publicado: |
2024
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| _version_ | 1866916524406603776 |
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| author | Valero, José Reina Madrid, Jose R. Navarro Blas, Diego Morcillo, Alejandro Díaz Irastorza, Igor García Gimeno, Benito Cabrera, Juan Monzó |
| author_facet | Valero, José Reina Madrid, Jose R. Navarro Blas, Diego Morcillo, Alejandro Díaz Irastorza, Igor García Gimeno, Benito Cabrera, Juan Monzó |
| contents | 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. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2407_20482 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | High-frequency gravitational waves detection with the BabyIAXO haloscopes Valero, José Reina Madrid, Jose R. Navarro Blas, Diego Morcillo, Alejandro Díaz Irastorza, Igor García Gimeno, Benito Cabrera, Juan Monzó High Energy Physics - Experiment 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. |
| title | High-frequency gravitational waves detection with the BabyIAXO haloscopes |
| topic | High Energy Physics - Experiment |
| url | https://arxiv.org/abs/2407.20482 |