| Article | |
| Report number | arXiv:2306.03125 ; CERN-TH-2023-093 |
| Title | Symmetries and Selection Rules: Optimising Axion Haloscopes for Gravitational Wave Searches |
| Author(s) | Domcke, Valerie (CERN) ; Garcia-Cely, Camilo (Valencia U., IFIC) ; Lee, Sung Mook (CERN ; IPAP, Seoul) ; Rodd, Nicholas L. (CERN) |
| Publication | 2024-03-21 |
| Imprint | 2023-06-05 |
| Number of pages | 23 |
| Note | 28+23 pages, 3+2 figures; added appendix to address the concerns raised in 2307.14555 |
| In: | JHEP 2403 (2024) 128 |
| DOI | 10.1007/JHEP03(2024)128 |
| Subject category | hep-ex ; Particle Physics - Experiment ; gr-qc ; General Relativity and Cosmology ; astro-ph.IM ; Astrophysics and Astronomy ; astro-ph.CO ; Astrophysics and Astronomy ; hep-ph ; Particle Physics - Phenomenology |
| Abstract | In the presence of electromagnetic fields, both axions and gravitational waves (GWs) induce oscillating magnetic fields: a potentially detectable fingerprint of their presence. We demonstrate that the response is largely dictated by the symmetries of the instruments used to search for it. Focussing on low mass axion haloscopes, we derive selection rules that determine the parametric sensitivity of different detector geometries to axions and GWs, and which further reveal how to optimise the experimental geometry to maximise both signals. The formalism allows us to forecast the optimal sensitivity to GWs in the range of 100 kHz to 100 MHz for instruments such as ABRACADABRA, BASE, ADMX SLIC, SHAFT, WISPLC, and DMRadio. |
| Copyright/License | preprint: (License: CC BY 4.0) publication: © 2024-2025 The Authors (License: CC-BY-4.0), sponsored by SCOAP³ |
Corresponding record in: Inspire
記錄創建於2023-06-08，最後更新在2024-05-02
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