ADMX Axion Dark Matter Bounds around 3.3 μeV with Dine-Fischler-Srednicki-Zhitnitsky Discovery Ability

C Goodman¹, M Guzzetti¹, C Hanretty¹, L J Rosenberg¹, G Rybka¹, J Sinnis¹, D Zhang¹, John Clarke², I Siddiqi², A S Chou³, M Hollister³, S Knirck³, A Sonnenschein³, T J Caligiure⁴, J R Gleason⁴, A T Hipp⁴, P Sikivie⁴, M E Solano⁴, N S Sullivan⁴, D B Tanner⁴, R Khatiwada⁵, G Carosi⁶, C Cisneros⁶, N Du⁶, N Robertson⁶, N Woollett⁶, L D Duffy⁷, C Boutan⁸, T Braine⁸, E Lentz⁸, N S Oblath⁸, M S Taubman⁸, E J Daw⁹, C Mostyn⁹, M G Perry⁹, C Bartram¹⁰, T A Dyson¹¹, S Ruppert¹¹, M O Withers¹¹, C L Kuo¹², B T McAllister¹³, J H Buckley¹⁴, C Gaikwad¹⁴, J Hoffman¹⁴, K Murch¹⁴, M Goryachev¹⁵, E Hartman¹⁵, A Quiskamp¹⁵, M E Tobar¹⁵; ADMX Collaboration

Affiliations

¹ University of Washington, Seattle, Washington 98195, USA.
² University of California, Berkeley, California 94720, USA.
³ Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA.
⁴ University of Florida, Gainesville, Florida 32611, USA.
⁵ Fermi National Accelerator Laboratory, Illinois Institute of Technology, Chicago, Illinois 60616, USA and , Batavia, Illinois 60510, USA.
⁶ Lawrence Livermore National Laboratory, Livermore, California 94550, USA.
⁷ Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA.
⁸ Pacific Northwest National Laboratory, Richland, Washington 99354, USA.
⁹ University of Sheffield, Sheffield S10 2TN, United Kingdom.
¹⁰ SLAC National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, California 94025, USA.
¹¹ Stanford University, Stanford, California 94305, USA.
¹² Stanford University, SLAC National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, California 94025, USA and , Stanford, California 94305, USA.
¹³ Swinburne University of Technology, John St., Hawthorn Victoria 3122, Australia.
¹⁴ Washington University, St. Louis, Missouri 63130, USA.
¹⁵ University of Western Australia, Perth, Western Australia 6009, Australia.

PMID: 40192393
DOI: 10.1103/PhysRevLett.134.111002

ADMX Axion Dark Matter Bounds around 3.3 μeV with Dine-Fischler-Srednicki-Zhitnitsky Discovery Ability

C Goodman et al. Phys Rev Lett. 2025.

. 2025 Mar 21;134(11):111002.

doi: 10.1103/PhysRevLett.134.111002.

Authors

Affiliations

¹ University of Washington, Seattle, Washington 98195, USA.
² University of California, Berkeley, California 94720, USA.
³ Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA.
⁴ University of Florida, Gainesville, Florida 32611, USA.
⁵ Fermi National Accelerator Laboratory, Illinois Institute of Technology, Chicago, Illinois 60616, USA and , Batavia, Illinois 60510, USA.
⁶ Lawrence Livermore National Laboratory, Livermore, California 94550, USA.
⁷ Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA.
⁸ Pacific Northwest National Laboratory, Richland, Washington 99354, USA.
⁹ University of Sheffield, Sheffield S10 2TN, United Kingdom.
¹⁰ SLAC National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, California 94025, USA.
¹¹ Stanford University, Stanford, California 94305, USA.
¹² Stanford University, SLAC National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, California 94025, USA and , Stanford, California 94305, USA.
¹³ Swinburne University of Technology, John St., Hawthorn Victoria 3122, Australia.
¹⁴ Washington University, St. Louis, Missouri 63130, USA.
¹⁵ University of Western Australia, Perth, Western Australia 6009, Australia.

PMID: 40192393
DOI: 10.1103/PhysRevLett.134.111002

Abstract

We report the results of a QCD axion dark matter search with discovery ability for Dine-Fischler-Srednicki-Zhitnitsky (DFSZ) axions using an axion haloscope. Sub-Kelvin noise temperatures are reached with an ultralow noise Josephson parametric amplifier cooled by a dilution refrigerator. This work excludes (with a 90% confidence level) DFSZ axions with masses between 3.27 to 3.34 μeV, assuming a standard halo model with a local energy density of 0.45 GeV/cm^{3} made up 100% of axions.

PubMed Disclaimer

Save citation to file

Email citation

Add to Collections

Add to My Bibliography

Your saved search

Create a file for external citation management software

Your RSS Feed

ADMX Axion Dark Matter Bounds around 3.3 μeV with Dine-Fischler-Srednicki-Zhitnitsky Discovery Ability

Affiliations

ADMX Axion Dark Matter Bounds around 3.3 μeV with Dine-Fischler-Srednicki-Zhitnitsky Discovery Ability

Authors

Affiliations

Abstract