Statistics and sensitivity of axion wind detection with the homogeneous precession domain of superfluid helium-3

The homogeneous precession domain (HPD) of superfluid <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:mrow><a:mmultiscripts><a:mrow><a:mi>He</a:mi></a:mrow><a:mprescripts/><a:none/><a:mrow><a:mn>3</a:mn></a:mrow></a:mmultiscripts></a:mrow></a:math> has recently been identified as a detection medium which might provide sensitivity to the axion-nucleon coupling <c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"><c:msub><c:mi>g</c:mi><c:mrow><c:mi>a</c:mi><c:mi>N</c:mi><c:mi>N</c:mi></c:mrow></c:msub></c:math> competitive with, or surpassing, existing experimental proposals. In this work, we make a detailed study of the statistical and dynamical properties of the HPD system in order to make realistic projections for a full-fledged experimental program. We include the effects of clock error and measurement error in a concrete readout scheme using superconducting qubits and quantum metrology. This work also provides a more general framework to describe the statistics associated with the axion gradient coupling through the treatment of a transient resonance with a nonstationary background in a time-series analysis. Incorporating an optimal data-taking and analysis strategy, we project a sensitivity approaching <e:math xmlns:e="http://www.w3.org/1998/Math/MathML" display="inline"><e:msub><e:mi>g</e:mi><e:mrow><e:mi>a</e:mi><e:mi>N</e:mi><e:mi>N</e:mi></e:mrow></e:msub><e:mo>∼</e:mo><e:msup><e:mn>10</e:mn><e:mrow><e:mo>−</e:mo><e:mn>12</e:mn></e:mrow></e:msup><e:mtext> </e:mtext><e:mtext> </e:mtext><e:mrow><e:msup><e:mrow><e:mi>GeV</e:mi></e:mrow><e:mrow><e:mo>−</e:mo><e:mn>1</e:mn></e:mrow></e:msup></e:mrow></e:math> across a decade in axion mass. Published by the American Physical Society 2024

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Journal
Physical review. D/Physical review. D.
Published
2024-12-13
DOI
https://doi.org/10.1103/physrevd.110.115020
Citations
4
Primary Topic
Dark Matter and Cosmic Phenomena
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article
Field-Weighted Citation Impact
1.98

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article

Statistics and sensitivity of axion wind detection with the homogeneous precession domain of superfluid helium-3

Joshua W. Foster, W. P. Halperin, Christina Gao, M. D. Nguyen et al.
4 citations
Physical review. D/Physical review. D.
Dark Matter and Cosmic Phenomena
1.98
article

Statistics and sensitivity of axion wind detection with the homogeneous precession domain of superfluid helium-3

Joshua W. Foster, W. P. Halperin, Christina Gao, M. D. Nguyen, J. W. Scott, Jan Schütte-Engel, Aarav Mande, Yonatan Kahn
article en
4 citations

Abstract

The homogeneous precession domain (HPD) of superfluid <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:mrow><a:mmultiscripts><a:mrow><a:mi>He</a:mi></a:mrow><a:mprescripts/><a:none/><a:mrow><a:mn>3</a:mn></a:mrow></a:mmultiscripts></a:mrow></a:math> has recently been identified as a detection medium which might provide sensitivity to the axion-nucleon coupling <c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"><c:msub><c:mi>g</c:mi><c:mrow><c:mi>a</c:mi><c:mi>N</c:mi><c:mi>N</c:mi></c:mrow></c:msub></c:math> competitive with, or surpassing, existing experimental proposals. In this work, we make a detailed study of the statistical and dynamical properties of the HPD system in order to make realistic projections for a full-fledged experimental program. We include the effects of clock error and measurement error in a concrete readout scheme using superconducting qubits and quantum metrology. This work also provides a more general framework to describe the statistics associated with the axion gradient coupling through the treatment of a transient resonance with a nonstationary background in a time-series analysis. Incorporating an optimal data-taking and analysis strategy, we project a sensitivity approaching <e:math xmlns:e="http://www.w3.org/1998/Math/MathML" display="inline"><e:msub><e:mi>g</e:mi><e:mrow><e:mi>a</e:mi><e:mi>N</e:mi><e:mi>N</e:mi></e:mrow></e:msub><e:mo>∼</e:mo><e:msup><e:mn>10</e:mn><e:mrow><e:mo>−</e:mo><e:mn>12</e:mn></e:mrow></e:msup><e:mtext> </e:mtext><e:mtext> </e:mtext><e:mrow><e:msup><e:mrow><e:mi>GeV</e:mi></e:mrow><e:mrow><e:mo>−</e:mo><e:mn>1</e:mn></e:mrow></e:msup></e:mrow></e:math> across a decade in axion mass. Published by the American Physical Society 2024

Physical review. D/Physical review. D.Vol. 110(11)
Northwestern University (US), Fermi National Accelerator Laboratory (US), University of Illinois Urbana-Champaign (US), Southern University of Science and Technology (CN), Nippon Soken (Japan) (JP), RIKEN (JP), Massachusetts Institute of Technology (US), University of California, Berkeley (US)
National Science Foundation, U.S. Department of Energy, Office of Science, Division of Materials Research, Fermilab
Openalex Percentile: Top 8%
Dark Matter and Cosmic Phenomena
1.98
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