• Open Access

ADMX-Orpheus first search for 70μeV dark photon dark matter: Detailed design, operations, and analysis

R. Cervantes, G. Carosi, S. Kimes, C. Hanretty, B. H. LaRoque, G. Leum, P. Mohapatra, N. S. Oblath, R. Ottens, Y. Park, G. Rybka, J. Sinnis, and J. Yang
Phys. Rev. D 106, 102002 – Published 9 November 2022

Abstract

Dark matter makes up 85% of the matter in the Universe and 27% of its energy density, but we do not know what comprises dark matter. It is possible that dark matter is composed of either axions or dark photons, both of which can be detected using an ultrasensitive microwave cavity known as a haloscope. The haloscope employed by ADMX consists of a cylindrical cavity operating at the TM010 mode and is sensitive to the QCD axion with masses of few μeV. However, this haloscope design becomes challenging to implement for higher masses. This is because higher masses require smaller-diameter cavities, consequently reducing the detection volume which diminishes the detected signal power. ADMX-Orpheus mitigates this issue by operating a tunable, dielectrically loaded cavity at a higher-order mode, allowing the detection volume to remain large. This paper describes the design, operation, analysis, and results of the inaugural ADMX-Orpheus dark photon search between 65.5μeV (15.8 GHz) and 69.3μeV (16.8 GHz), as well as future directions for axion searches and for exploring more parameter space.

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  • Received 22 April 2022
  • Accepted 21 September 2022

DOI:https://doi.org/10.1103/PhysRevD.106.102002

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

  1. Research Areas
  1. Physical Systems
Gravitation, Cosmology & Astrophysics

Authors & Affiliations

R. Cervantes1,2,*,†, G. Carosi2, S. Kimes1,‡, C. Hanretty1, B. H. LaRoque3, G. Leum1, P. Mohapatra1,∥, N. S. Oblath3, R. Ottens1,§, Y. Park1,**, G. Rybka1, J. Sinnis1, and J. Yang1,††

  • 1University of Washington, Seattle, Washington 98195, USA
  • 2Lawrence Livermore National Laboratory, Livermore, California 94550, USA
  • 3Pacific Northwest National Laboratory, Richland, Washington 99354, USA

  • *Corresponding author. raphaelc@fnal.gov
  • Present address: Fermi National Accelerator Laboratory, Batavia Illinois 60510, USA.
  • Present address: Microsoft Quantum, Microsoft, Redmond, Washington 98052, USA.
  • Present address: Joby Aviation, San Carlos, California 94063, USA.
  • §Present address: NASA Goddard Space Flight Center Greenbelt, Maryland, USA.
  • **Present address: University of California, Berkeley, California 94720, USA.
  • ††Present address: Pacific Northwest National Laboratory, Richland, Washington 99354, USA.

See Also

Search for 70μeV Dark Photon Dark Matter with a Dielectrically Loaded Multiwavelength Microwave Cavity

R. Cervantes, G. Carosi, C. Hanretty, S. Kimes, B. H. LaRoque, G. Leum, P. Mohapatra, N. S. Oblath, R. Ottens, Y. Park, G. Rybka, J. Sinnis, and J. Yang
Phys. Rev. Lett. 129, 201301 (2022)

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Issue

Vol. 106, Iss. 10 — 15 November 2022

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