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Search for ultralight axion dark matter in a side-band analysis of a
Ultra-low-mass axions are a viable dark matter candidate and may form a coherently oscillating classical field. Nuclear spins in experiments on Earth might couple to this oscillating axion dark-matter field, when propagating on Earth's trajectory through our Galaxy. This spin coupling resembles an oscillating pseudo-magnetic field which modulates the spin precession of nuclear spins. Here we report on the null result of a demonstration experiment searching for a frequency modulation of the free spin-precession signal of
dc.abstract.en | Ultra-low-mass axions are a viable dark matter candidate and may form a coherently oscillating classical field. Nuclear spins in experiments on Earth might couple to this oscillating axion dark-matter field, when propagating on Earth's trajectory through our Galaxy. This spin coupling resembles an oscillating pseudo-magnetic field which modulates the spin precession of nuclear spins. Here we report on the null result of a demonstration experiment searching for a frequency modulation of the free spin-precession signal of $^{199}$Hg in a 1 $\mu$T magnetic field. Our search covers the axion mass range 10$^{-16}$ eV $\lesssim$ m$_{a} \lesssim$ 10$^{-13}$ eV and achieves a peak sensitivity to the axion-nucleon coupling of g$_{aNN} \approx$ 3.5 $\times$ 10$^{-6}$ GeV$^{-1}$. | pl |
dc.affiliation | Wydział Fizyki, Astronomii i Informatyki Stosowanej : Instytut Fizyki im. Mariana Smoluchowskiego | pl |
dc.contributor.author | Abel, C. | pl |
dc.contributor.author | Ayres, N. J. | pl |
dc.contributor.author | Ban, G. | pl |
dc.contributor.author | Bison, G. | pl |
dc.contributor.author | Bodek, Kazimierz - 100562 | pl |
dc.contributor.author | Bondar, V. | pl |
dc.contributor.author | Chanel, E. | pl |
dc.contributor.author | Crawford, C. B. | pl |
dc.contributor.author | Daum, M. | pl |
dc.contributor.author | Dechenaux, B. | pl |
dc.contributor.author | Emmenegger, S. | pl |
dc.contributor.author | Flaux, P. | pl |
dc.contributor.author | Griffith, W. C. | pl |
dc.contributor.author | Harris, P. G. | pl |
dc.contributor.author | Kermaidic, Y. | pl |
dc.contributor.author | Kirch, K. | pl |
dc.contributor.author | Komposch, S. | pl |
dc.contributor.author | Koss, P. A. | pl |
dc.contributor.author | Krempel, J. | pl |
dc.contributor.author | Lauss, B. | pl |
dc.contributor.author | Lefort, T. | pl |
dc.contributor.author | MohanMurthy, Prajwal | pl |
dc.contributor.author | Naviliat Cuncic, Oscar | pl |
dc.contributor.author | Pais, D. | pl |
dc.contributor.author | Piegsa, F. M. | pl |
dc.contributor.author | Pignol, Guillaume | pl |
dc.contributor.author | Rawlik, M. | pl |
dc.contributor.author | Ries, D. | pl |
dc.contributor.author | Roccia, Stephanie | pl |
dc.contributor.author | Rozpędzik, Dagmara - 145490 | pl |
dc.contributor.author | Schmidt-Wellenburg, Philipp | pl |
dc.contributor.author | Severijns, N. | pl |
dc.contributor.author | Stadnik, Y. V. | pl |
dc.contributor.author | Thorne, J. A. | pl |
dc.contributor.author | Weis, A. | pl |
dc.contributor.author | Wursten, E. | pl |
dc.contributor.author | Zejma, Jacek - 100021 | pl |
dc.contributor.author | Zsigmond, Geza | pl |
dc.date.accessioned | 2023-09-28T10:28:22Z | |
dc.date.available | 2023-09-28T10:28:22Z | |
dc.date.issued | 2023 | pl |
dc.date.openaccess | 0 | |
dc.description.accesstime | w momencie opublikowania | |
dc.description.number | 2 | pl |
dc.description.version | ostateczna wersja wydawcy | |
dc.description.volume | 15 | pl |
dc.identifier.articleid | 058 | pl |
dc.identifier.doi | 10.21468/SciPostPhys.15.2.058 | pl |
dc.identifier.eissn | 2542-4653 | pl |
dc.identifier.uri | https://ruj.uj.edu.pl/xmlui/handle/item/320018 | |
dc.language | eng | pl |
dc.language.container | eng | pl |
dc.rights | Udzielam licencji. Uznanie autorstwa 4.0 Międzynarodowa | * |
dc.rights.licence | CC-BY | |
dc.rights.uri | http://creativecommons.org/licenses/by/4.0/legalcode.pl | * |
dc.share.type | otwarte czasopismo | |
dc.subtype | Article | pl |
dc.title | Search for ultralight axion dark matter in a side-band analysis of a $^{199}$Hg free-spin precession signal | pl |
dc.title.journal | SciPost Physics | pl |
dc.type | JournalArticle | pl |
dspace.entity.type | Publication |