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Axion detection via Topological Casimir Effect

Cao, ChunJun and Zhitnitsky, Ariel (2017) Axion detection via Topological Casimir Effect. Physical Review D, 96 (1). Art. No. 015013. ISSN 2470-0010. https://resolver.caltech.edu/CaltechAUTHORS:20170209-150222935

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Abstract

We propose a new table-top experimental configuration for the direct detection of dark matter QCD axions in the traditional open mass window 10^(-6)  eV ≲ m_a ≲ 10^(-2)  eV using nonperturbative effects in a system with nontrivial spatial topology. Different from most experimental setups found in literature on direct dark matter axion detection, which relies on ˙θ or ⃗∇θ, we found that our system is in principle sensitive to a static θ ≥ 10^(-14) and can also be used to set limit on the fundamental constant θ_(QED) which becomes the fundamental observable parameter of the Maxwell system if some conditions are met. Furthermore, the proposed experiments can probe entire open mass window 10^(-6)  eV ≲ m_a ≲10^(-2)  eV with the same design, which should be contrasted with conventional cavity-type experiments being sensitive to a specific axion mass. Connection with Witten effect when the induced electric charge e′ is proportional to θ and the magnetic monopole becomes the dyon with nonvanishing e′ = -eθ/2π is also discussed.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1103/PhysRevD.96.015013DOIArticle
https://journals.aps.org/prd/abstract/10.1103/PhysRevD.96.015013PublisherArticle
http://arxiv.org/abs/1702.00012arXivDiscussion Paper
Additional Information:© 2017 American Physical Society. Received 27 April 2017; published 13 July 2017. We would like to thank Sean Carroll, Stephen Hsu, Zitao Wang, and Mark Wise for helpful discussions. One of us (AZ) is thankful to Cliff Burgess, Glenn Strakman, Mark Trodden and other participants of the MITP program “Quantum Vacuum and Gravitation”, Mainz, March, 2017, for very useful discussions related to the subject of the present work. AZ is also thankful to Giovanni Cantatore for long and very optimistic discussions on feasibility to experimentally test the TCE and its sensitivity to θ. This research was supported in part by the Natural Sciences and Engineering Research Council of Canada and by the Walter Burke Institute for Theoretical Physics at Caltech, by DOE grant DE-SC0011632, by the Foundational Questions Institute, by the Gordon and Betty Moore Foundation through Grant 776 to the Caltech Moore Center for Theoretical Cosmology and Physics, and by the John Simon Guggenheim Memorial Foundation.
Group:Walter Burke Institute for Theoretical Physics, Moore Center for Theoretical Cosmology and Physics
Funders:
Funding AgencyGrant Number
Natural Sciences and Engineering Research Council of Canada (NSERC)UNSPECIFIED
Walter Burke Institute for Theoretical Physics, CaltechUNSPECIFIED
Department of Energy (DOE)DE-SC0011632
Foundational Questions Institute (FQXI)UNSPECIFIED
Gordon and Betty Moore Foundation776
John Simon Guggenheim Memorial FoundationUNSPECIFIED
Other Numbering System:
Other Numbering System NameOther Numbering System ID
CALT-TH2017-007
Issue or Number:1
Record Number:CaltechAUTHORS:20170209-150222935
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20170209-150222935
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:74199
Collection:CaltechAUTHORS
Deposited By: Joy Painter
Deposited On:09 Feb 2017 23:44
Last Modified:03 Oct 2019 16:35

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