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dc.contributor.authorLawson, Matthew
dc.contributor.authorMillar, Alexander J
dc.contributor.authorPancaldi, Matteo
dc.contributor.authorVitagliano, Edoardo
dc.contributor.authorWilczek, Frank
dc.date.accessioned2021-10-27T20:35:28Z
dc.date.available2021-10-27T20:35:28Z
dc.date.issued2019
dc.identifier.urihttps://hdl.handle.net/1721.1/136458
dc.description.abstract© 2019 authors. Published by the American Physical Society. We propose a new strategy for searching for dark matter axions using tunable cryogenic plasmas. Unlike current experiments, which repair the mismatch between axion and photon masses by breaking translational invariance (cavity and dielectric haloscopes), a plasma haloscope enables resonant conversion by matching the axion mass to a plasma frequency. A key advantage is that the plasma frequency is unrelated to the physical size of the device, allowing large conversion volumes. We identify wire metamaterials as a promising candidate plasma, wherein the plasma frequency can be tuned by varying the interwire spacing. For realistic experimental sizes, we estimate competitive sensitivity for axion masses of 35-400 μeV, at least.
dc.language.isoen
dc.publisherAmerican Physical Society (APS)
dc.relation.isversionof10.1103/PHYSREVLETT.123.141802
dc.rightsCreative Commons Attribution 4.0 International license
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.sourceAPS
dc.titleTunable Axion Plasma Haloscopes
dc.typeArticle
dc.contributor.departmentMassachusetts Institute of Technology. Center for Theoretical Physics
dc.relation.journalPhysical Review Letters
dc.eprint.versionFinal published version
dc.type.urihttp://purl.org/eprint/type/JournalArticle
eprint.statushttp://purl.org/eprint/status/PeerReviewed
dc.date.updated2021-07-08T17:51:08Z
dspace.orderedauthorsLawson, M; Millar, AJ; Pancaldi, M; Vitagliano, E; Wilczek, F
dspace.date.submission2021-07-08T17:51:09Z
mit.journal.volume123
mit.journal.issue14
mit.licensePUBLISHER_CC
mit.metadata.statusAuthority Work and Publication Information Needed


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