José Reina Valero, Jose R. Navarro Madrid, Diego Blas, Alejandro Díaz Morcillo, Igor García Irastorza, Benito Gimeno, Juan Monzó Cabrera
{"title":"High-frequency gravitational waves detection with the BabyIAXO haloscopes","authors":"José Reina Valero, Jose R. Navarro Madrid, Diego Blas, Alejandro Díaz Morcillo, Igor García Irastorza, Benito Gimeno, Juan Monzó Cabrera","doi":"arxiv-2407.20482","DOIUrl":null,"url":null,"abstract":"We present the first analysis using RADES-BabyIAXO cavities as detectors of\nhigh-frequency gravitational waves (HFGWs). In particular, we discuss two\nconfigurations for distinct frequency ranges of HFGWs: Cavity 1, mostly\nsensitive at a frequency range of 252.8 - 333.2 MHz, and Cavity 2, at 2.504 -\n3.402 GHz, which is a scaled down version of Cavity 1. We find that Cavity 1\nwill reach sensitivity to strains of the HFGWs of order $h_1\\sim 10^{-21}$,\nwhile Cavity 2 will reach $h_2\\sim 10^{-20}$. These represent the best\nestimations of the RADES-BabyIAXO cavities as HFGWs detectors, showing how this\nset-up can produce groundbreaking results in axion physics and HFGWs\nsimultaneously.","PeriodicalId":501181,"journal":{"name":"arXiv - PHYS - High Energy Physics - Experiment","volume":"45 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-07-30","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - High Energy Physics - Experiment","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2407.20482","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
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.