Search for dark matter axions with CAST-CAAP
dc.authorid | Serkant Ali Çetin / 0000-0001-5050-8441 | en_US |
dc.authorid | Aydın Özbey / 0000-0001-7097-4044 | en_US |
dc.authorid | Kaan Özbozduman / 0000-0002-4713-7296 | en_US |
dc.authorscopusid | Serkant Ali Çetin / 34567544400 | |
dc.authorscopusid | Kaan Özbozduman / 57202033822 | |
dc.authorscopusid | Aydın Özbey / 55978024600 | |
dc.authorwosid | Serkant Ali Çetin / AGF-0147-2022 | en_US |
dc.authorwosid | Aydın Özbey / V-1388-2017 | en_US |
dc.authorwosid | Kaan Özbozduman / JDW-1875-2023 | en_US |
dc.contributor.author | Adair, C. M. | |
dc.contributor.author | Altenmuller, K. | |
dc.contributor.author | Anastassopoulos, V | |
dc.contributor.author | Cuendis, S. Arguedas | |
dc.contributor.author | Baier, J. | |
dc.date.accessioned | 2022-11-07T07:29:36Z | |
dc.date.available | 2022-11-07T07:29:36Z | |
dc.date.issued | 2022 | en_US |
dc.department | Ä°stinye Ãœniversitesi | en_US |
dc.description.abstract | The CAST-CAPP axion haloscope, operating at CERN inside the CAST dipole magnet, has searched for axions in the 19.74 mu eV to 22.47 mu eV mass range. The detection concept follows the Sikivie haloscope principle, where Dark Matter axions convert into photons within a resonator immersed in a magnetic field. The CAST-CAPP resonator is an array of four individual rectangular cavities inserted in a strong dipole magnet, phase-matched to maximize the detection sensitivity. Here we report on the data acquired for 4124 h from 2019 to 2021. Each cavity is equipped with a fast frequency tuning mechanism of 10 MHz/ min between 4.774 GHz and 5.434 GHz. In the present work, we exclude axion-photon couplings for virialized galactic axions down to g(a gamma gamma) = 8 x 10(-14) GeV-1 at the 90% confidence level. The here implemented phase-matching technique also allows for future large-scale upgrades. | en_US |
dc.identifier.citation | Adair, C.M., Altenmüller, K., Anastassopoulos, V. et al. Search for Dark Matter Axions with CAST-CAPP. Nat Commun 13, 6180 (2022). https://doi.org/10.1038/s41467-022-33913-6 | en_US |
dc.identifier.doi | 10.1038/s41467-022-33913-6 | en_US |
dc.identifier.issn | 2041-1723 | en_US |
dc.identifier.issue | 1 | en_US |
dc.identifier.scopus | 2-s2.0-85140246106 | en_US |
dc.identifier.scopusquality | Q1 | en_US |
dc.identifier.uri | https://doi.org/10.1038/s41467-022-33913-6 | |
dc.identifier.uri | https://hdl.handle.net/20.500.12713/3245 | |
dc.identifier.volume | 13 | en_US |
dc.identifier.wos | WOS:000870431200029 | en_US |
dc.identifier.wosquality | Q1 | en_US |
dc.indekslendigikaynak | Web of Science | en_US |
dc.indekslendigikaynak | Scopus | en_US |
dc.indekslendigikaynak | PubMed | en_US |
dc.institutionauthor | Çetin, Serkant Ali | |
dc.institutionauthor | Özbey, Aydın | |
dc.institutionauthor | Özbozduman, Kaan | |
dc.language.iso | en | en_US |
dc.publisher | NATURE PORTFOLIO | en_US |
dc.relation.ispartof | NATURE COMMUNICATIONS | en_US |
dc.relation.publicationcategory | Makale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı | en_US |
dc.rights | info:eu-repo/semantics/openAccess | en_US |
dc.title | Search for dark matter axions with CAST-CAAP | en_US |
dc.type | Article | en_US |