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Search for Dark Matter Axions with CAST-CAPP.

C M Adair1, K Altenmüller2, V Anastassopoulos3

  • 1Department of Physics and Astronomy, University of British Columbia, Vancouver, V6T 1Z1, BC, Canada.

Nature Communications
|October 19, 2022
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Summary
This summary is machine-generated.

The CAST-CAPP experiment searched for axions, a type of dark matter, using a haloscope. This study excluded specific axion-photon couplings, advancing dark matter detection capabilities.

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Area of Science:

  • Particle Physics
  • Cosmology
  • Astrophysics

Background:

  • Axions are hypothetical particles proposed as a dark matter candidate.
  • The CAST experiment at CERN utilizes a dipole magnet to search for axions.
  • The haloscope detection principle relies on axion-to-photon conversion in a magnetic field.

Purpose of the Study:

  • To search for axions within the 19.74–22.47 μeV mass range.
  • To constrain the axion-photon coupling constant (gaγγ).
  • To test the efficacy of phase-matching techniques for future axion haloscope upgrades.

Main Methods:

  • Utilized the CAST-CAPP axion haloscope, an array of four phase-matched rectangular cavities.
  • Operated within the CERN CAST dipole magnet from 2019 to 2021, accumulating 4124 hours of data.
  • Employed fast frequency tuning mechanisms (10 MHz/min) across the 4.774–5.434 GHz range.

Main Results:

  • Excluded axion-photon couplings down to gaγγ = 8 × 10-14 GeV-1 at the 90% confidence level for virialized galactic axions.
  • The data covers the axion mass range of 19.74–22.47 μeV.
  • Demonstrated the feasibility of the phase-matching technique for enhanced sensitivity.

Conclusions:

  • The CAST-CAPP experiment has set new limits on axion properties.
  • The implemented phase-matching technique shows promise for future, more sensitive dark matter searches.
  • Further upgrades incorporating this technique could significantly improve dark matter detection.