4.8 Article

Broadband Solenoidal Haloscope for Terahertz Axion Detection

Journal

PHYSICAL REVIEW LETTERS
Volume 128, Issue 13, Pages -

Publisher

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevLett.128.131801

Keywords

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Funding

  1. Department of Energy through the program for Quantum Information Science Enabled Discovery (QuantISED) for High Energy Physics
  2. U.S. Department of Energy, Office of High Energy Physics [DE-AC02-06CH1135, DE-AC02-07CH11359]
  3. Kavli Institute for Cosmological Physics at the University of Chicago [NSF PHY-1125897]
  4. Kavli Foundation
  5. Lawrence Livermore National Laboratory [DE-AC52-07NA27344, LLNL-JRNL-828670]
  6. Fermi Research Alliance, LLC (FRA)
  7. US Department of Energy (DOE) [DE-AC02-07CH11359]
  8. National Science Foundation [PHY-1607611]
  9. Heising-Simons Foundation
  10. Grainger Foundation
  11. Junior Research Fellowship at Trinity College, University of Cambridge

Ask authors/readers for more resources

We introduce the Broadband Reflector Experiment for Axion Detection (BREAD) conceptual design and science program, which plans to search for bosonic dark matter. BREAD proposes a cylindrical metal barrel to convert dark matter into photons and focuses them onto a photosensor using a novel parabolic reflector design. By conducting a pilot 0.7 m(2) barrel experiment, BREAD is expected to surpass existing dark photon coupling constraints and improve sensitivity.
We introduce the Broadband Reflector Experiment for Axion Detection (BREAD) conceptual design and science program. This haloscope plans to search for bosonic dark matter across the [10(-3), 1] eV ([0.24, 240] THz) mass range. BREAD proposes a cylindrical metal barrel to convert dark matter into photons, which a novel parabolic reflector design focuses onto a photosensor. This unique geometry enables enclosure in standard cryostats and high-field solenoids, overcoming limitations of current dish antennas. A pilot 0.7 m(2) barrel experiment planned at Fermilab is projected to surpass existing dark photon coupling constraints by over a decade with one-day runtime. Axion sensitivity requires < 10(-20) W/root Hz sensor noise equivalent power with a 10 T solenoid and 10 m(2) barrel. We project BREAD sensitivity for various sensor technologies and discuss future prospects.

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