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dc.contributor.author | Popov V. | |
dc.date.accessioned | 2018-09-19T20:51:47Z | |
dc.date.available | 2018-09-19T20:51:47Z | |
dc.date.issued | 2016 | |
dc.identifier.issn | 1063-7761 | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/143355 | |
dc.description.abstract | © 2016, Pleiades Publishing, Inc.A method for detecting dark matter axions in which a dc SQUID serves as a detector is proposed. The SQUID is shown to be able to detect the magnetic field perturbations induced by its interaction with axions. The resonance signal appears as a current step in the SQUID current–voltage characteristic. The voltage of the step corresponds to the axion mass, while its height depends on the axion energy density in near-Earth space. The proposed method is aimed at detecting axions with masses ma ≲ 10–4 eV, which are of interest for both cosmology and particle physics. | |
dc.relation.ispartofseries | Journal of Experimental and Theoretical Physics | |
dc.title | Resonance detection of dark matter axions using a DC SQUID | |
dc.type | Article | |
dc.relation.ispartofseries-issue | 2 | |
dc.relation.ispartofseries-volume | 122 | |
dc.collection | Публикации сотрудников КФУ | |
dc.relation.startpage | 236 | |
dc.source.id | SCOPUS10637761-2016-122-2-SID84962374476 |