4.8 Article

Search for axion-like dark matter with spin-based amplifiers

Journal

NATURE PHYSICS
Volume 17, Issue 12, Pages 1402-+

Publisher

NATURE PORTFOLIO
DOI: 10.1038/s41567-021-01392-z

Keywords

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Funding

  1. National Key Research and Development Program of China [2018YFA0306600]
  2. National Natural Science Foundation of China [11661161018, 11927811, 12004371]
  3. Anhui Initiative in Quantum Information Technologies [AHY050000]
  4. USTC Research Funds of the Double First-Class Initiative [YD3540002002]
  5. Cluster of Excellence PRISMA+ - German Research Foundation (DFG) within the German Excellence Strategy [39083149]
  6. European Research Council (ERC) under the European Union Horizon 2020 research and innovation programme (Dark-OsT project) [695405]
  7. DFG Reinhart Koselleck project
  8. Emergent AI Center - Carl-Zeiss-Stiftung

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This study reports on the search for axion-like dark matter using a quantum sensor with enhanced potential signals. By utilizing hyperpolarized long-lived nuclear spins as pre-amplifiers, the study achieved ultrahigh magnetic sensitivity and constrained the parameter space of interactions between nucleons and axion-like particles. The experiment significantly improved on previous laboratory constraints and exceeded bounds from astrophysical observations.
A search for axion-like dark matter with a quantum sensor that enhances potential signals is reported. This work constrains the parameter space of different interactions between nucleons and axion-like particles and between nucleons and dark photons. Ultralight axion-like particles are well-motivated dark matter candidates introduced by theories beyond the standard model of particle physics. However, directly constraining their parameter space with laboratory experiments usually yields weaker limits than indirect approaches relying on astrophysical observations. Here we report the search for axion-like particles with a quantum sensor in the mass range of 8.3-744.0 feV. The sensor makes use of hyperpolarized long-lived nuclear spins as a pre-amplifier that effectively enhances a coherently oscillating axion-like dark matter field by a factor of more than 100. Using these spin-based amplifiers, we achieve an ultrahigh magnetic sensitivity of 18 fT Hz(-(1/2)), which exceeds the performance of state-of-the-art nuclear spin magnetometers. Our experiment constrains the parameter space describing the coupling of axion-like particles to nucleons over the aforementioned mass range, namely, at 67.5 feV reaching 2.9 x 10(-9) GeV-1, improving on previous laboratory constraints by at least five orders of magnitude. Our measurements also constrain the quadratic interaction between axion-like particles and nucleons as well as interactions between dark photons and nucleons, exceeding bounds from astrophysical observations.

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