dc.contributor.author | Kahn, Yonatan | |
dc.contributor.author | Safdi, Benjamin Ryan | |
dc.contributor.author | Thaler, Jesse | |
dc.date.accessioned | 2016-11-07T20:57:27Z | |
dc.date.available | 2016-11-07T20:57:27Z | |
dc.date.issued | 2016-09 | |
dc.date.submitted | 2016-03 | |
dc.identifier.issn | 0031-9007 | |
dc.identifier.issn | 1079-7114 | |
dc.identifier.uri | http://hdl.handle.net/1721.1/105237 | |
dc.description.abstract | When ultralight axion dark matter encounters a static magnetic field, it sources an effective electric current that follows the magnetic field lines and oscillates at the axion Compton frequency. We propose a new experiment to detect this axion effective current. In the presence of axion dark matter, a large toroidal magnet will act like an oscillating current ring, whose induced magnetic flux can be measured by an external pickup loop inductively coupled to a SQUID magnetometer. We consider both resonant and broadband readout circuits and show that a broadband approach has advantages at small axion masses. We estimate the reach of this design, taking into account the irreducible sources of noise, and demonstrate potential sensitivity to axionlike dark matter with masses in the range of 10[superscript -14]-10[superscript -6] eV. In particular, both the broadband and resonant strategies can probe the QCD axion with a GUT-scale decay constant. | en_US |
dc.description.sponsorship | Massachusetts Institute of Technology. Pappalardo Fellowship | en_US |
dc.description.sponsorship | United States. Dept. of Energy (Cooperative Research Agreement DE-SC- 00012567) | en_US |
dc.description.sponsorship | United States. Dept. of Energy (Early Career Research program DE-SC-0006389) | en_US |
dc.description.sponsorship | Alfred P. Sloan Foundation (Sloan Research Fellowship) | en_US |
dc.publisher | American Physical Society | en_US |
dc.relation.isversionof | http://dx.doi.org/10.1103/PhysRevLett.117.141801 | en_US |
dc.rights | Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. | en_US |
dc.source | American Physical Society | en_US |
dc.title | Broadband and Resonant Approaches to Axion Dark Matter Detection | en_US |
dc.type | Article | en_US |
dc.identifier.citation | Kahn, Yonatan, Benjamin R. Safdi, and Jesse Thaler. “Broadband and Resonant Approaches to Axion Dark Matter Detection.” Physical Review Letters 117.14 (2016): n. pag. © 2016 American Physical Society | en_US |
dc.contributor.department | Massachusetts Institute of Technology. Center for Theoretical Physics | en_US |
dc.contributor.mitauthor | Safdi, Benjamin Ryan | |
dc.contributor.mitauthor | Thaler, Jesse | |
dc.relation.journal | Physical Review Letters | en_US |
dc.eprint.version | Final published version | en_US |
dc.type.uri | http://purl.org/eprint/type/JournalArticle | en_US |
eprint.status | http://purl.org/eprint/status/PeerReviewed | en_US |
dc.date.updated | 2016-09-30T22:00:03Z | |
dc.language.rfc3066 | en | |
dc.rights.holder | American Physical Society | |
dspace.orderedauthors | Kahn, Yonatan; Safdi, Benjamin R.; Thaler, Jesse | en_US |
dspace.embargo.terms | N | en_US |
dc.identifier.orcid | https://orcid.org/0000-0001-9531-1319 | |
dc.identifier.orcid | https://orcid.org/0000-0002-2406-8160 | |
mit.license | PUBLISHER_POLICY | en_US |
mit.metadata.status | Complete | |