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 |
|