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Nitta T, Braine T, Du N, Guzzetti M, Hanretty C, Leum G, Rosenberg LJ, Rybka G, Sinnis J, Clarke J, Siddiqi I, Awida MH, Chou AS, Hollister M, Knirck S, Sonnenschein A, Wester W, Gleason JR, Hipp AT, Sikivie P, Sullivan NS, Tanner DB, Khatiwada R, Carosi G, Robertson N, Duffy LD, Boutan C, Lentz E, Oblath NS, Taubman MS, Yang J, Daw EJ, Perry MG, Bartram C, Buckley JH, Gaikwad C, Hoffman J, Murch KW, Goryachev M, Hartman E, McAllister BT, Quiskamp A, Thomson C, Tobar ME, Dror JA, Murayama H, Rodd NL. Search for a Dark-Matter-Induced Cosmic Axion Background with ADMX. Phys Rev Lett 2023; 131:101002. [PMID: 37739367 DOI: 10.1103/physrevlett.131.101002] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 03/19/2023] [Revised: 06/05/2023] [Accepted: 08/16/2023] [Indexed: 09/24/2023]
Abstract
We report the first result of a direct search for a cosmic axion background (CaB)-a relativistic background of axions that is not dark matter-performed with the axion haloscope, the Axion Dark Matter eXperiment (ADMX). Conventional haloscope analyses search for a signal with a narrow bandwidth, as predicted for dark matter, whereas the CaB will be broad. We introduce a novel analysis strategy, which searches for a CaB induced daily modulation in the power measured by the haloscope. Using this, we repurpose data collected to search for dark matter to set a limit on the axion photon coupling of a CaB originating from dark matter cascade decay via a mediator in the 800-995 MHz frequency range. We find that the present sensitivity is limited by fluctuations in the cavity readout as the instrument scans across dark matter masses. Nevertheless, we suggest that these challenges can be surmounted using superconducting qubits as single photon counters, and allow ADMX to operate as a telescope searching for axions emerging from the decay of dark matter. The daily modulation analysis technique we introduce can be deployed for various broadband rf signals, such as other forms of a CaB or even high-frequency gravitational waves.
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Affiliation(s)
| | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | - J A Dror
- Santa Cruz Institute for Particle Physics and Department of Physics, University of California, 1156 High St, Santa Cruz, California 95060, USA
| | - H Murayama
- University of California, Berkeley, California 94720, USA
- Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo, Kashiwa 277-8583, Japan
| | - N L Rodd
- Theoretical Physics Department, CERN, 1 Esplanade des Particules, CH-1211 Geneva 23, Switzerland
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Bartram C, Braine T, Burns E, Cervantes R, Crisosto N, Du N, Korandla H, Leum G, Mohapatra P, Nitta T, Rosenberg LJ, Rybka G, Yang J, Clarke J, Siddiqi I, Agrawal A, Dixit AV, Awida MH, Chou AS, Hollister M, Knirck S, Sonnenschein A, Wester W, Gleason JR, Hipp AT, Jois S, Sikivie P, Sullivan NS, Tanner DB, Lentz E, Khatiwada R, Carosi G, Robertson N, Woollett N, Duffy LD, Boutan C, Jones M, LaRoque BH, Oblath NS, Taubman MS, Daw EJ, Perry MG, Buckley JH, Gaikwad C, Hoffman J, Murch KW, Goryachev M, McAllister BT, Quiskamp A, Thomson C, Tobar ME. Search for Invisible Axion Dark Matter in the 3.3-4.2 μeV Mass Range. Phys Rev Lett 2021; 127:261803. [PMID: 35029490 DOI: 10.1103/physrevlett.127.261803] [Citation(s) in RCA: 7] [Impact Index Per Article: 2.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/11/2021] [Accepted: 11/16/2021] [Indexed: 06/14/2023]
Abstract
We report the results from a haloscope search for axion dark matter in the 3.3-4.2 μeV mass range. This search excludes the axion-photon coupling predicted by one of the benchmark models of "invisible" axion dark matter, the Kim-Shifman-Vainshtein-Zakharov model. This sensitivity is achieved using a large-volume cavity, a superconducting magnet, an ultra low noise Josephson parametric amplifier, and sub-Kelvin temperatures. The validity of our detection procedure is ensured by injecting and detecting blind synthetic axion signals.
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Affiliation(s)
- C Bartram
- University of Washington, Seattle, Washington 98195, USA
| | - T Braine
- University of Washington, Seattle, Washington 98195, USA
| | - E Burns
- University of Washington, Seattle, Washington 98195, USA
| | - R Cervantes
- University of Washington, Seattle, Washington 98195, USA
| | - N Crisosto
- University of Washington, Seattle, Washington 98195, USA
| | - N Du
- University of Washington, Seattle, Washington 98195, USA
| | - H Korandla
- University of Washington, Seattle, Washington 98195, USA
| | - G Leum
- University of Washington, Seattle, Washington 98195, USA
| | - P Mohapatra
- University of Washington, Seattle, Washington 98195, USA
| | - T Nitta
- University of Washington, Seattle, Washington 98195, USA
| | - L J Rosenberg
- University of Washington, Seattle, Washington 98195, USA
| | - G Rybka
- University of Washington, Seattle, Washington 98195, USA
| | - J Yang
- University of Washington, Seattle, Washington 98195, USA
| | - John Clarke
- University of California, Berkeley, California 94720, USA
| | - I Siddiqi
- University of California, Berkeley, California 94720, USA
| | - A Agrawal
- University of Chicago, Illinois 60637, USA
| | - A V Dixit
- University of Chicago, Illinois 60637, USA
| | - M H Awida
- Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - A S Chou
- Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - M Hollister
- Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - S Knirck
- Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - A Sonnenschein
- Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - W Wester
- Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - J R Gleason
- University of Florida, Gainesville, Florida 32611, USA
| | - A T Hipp
- University of Florida, Gainesville, Florida 32611, USA
| | - S Jois
- University of Florida, Gainesville, Florida 32611, USA
| | - P Sikivie
- University of Florida, Gainesville, Florida 32611, USA
| | - N S Sullivan
- University of Florida, Gainesville, Florida 32611, USA
| | - D B Tanner
- University of Florida, Gainesville, Florida 32611, USA
| | - E Lentz
- University of Göttingen, Göttingen 37077, Germany
| | - R Khatiwada
- Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
- Illinois Institute of Technology, Chicago, Illinois 60616, USA
| | - G Carosi
- Lawrence Livermore National Laboratory, Livermore, California 94550, USA
| | - N Robertson
- Lawrence Livermore National Laboratory, Livermore, California 94550, USA
| | - N Woollett
- Lawrence Livermore National Laboratory, Livermore, California 94550, USA
| | - L D Duffy
- Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
| | - C Boutan
- Pacific Northwest National Laboratory, Richland, Washington 99354, USA
| | - M Jones
- Pacific Northwest National Laboratory, Richland, Washington 99354, USA
| | - B H LaRoque
- Pacific Northwest National Laboratory, Richland, Washington 99354, USA
| | - N S Oblath
- Pacific Northwest National Laboratory, Richland, Washington 99354, USA
| | - M S Taubman
- Pacific Northwest National Laboratory, Richland, Washington 99354, USA
| | - E J Daw
- University of Sheffield, Sheffield S3 7RH, United Kingdom
| | - M G Perry
- University of Sheffield, Sheffield S3 7RH, United Kingdom
| | - J H Buckley
- Washington University, St. Louis, Missouri 63130, USA
| | - C Gaikwad
- Washington University, St. Louis, Missouri 63130, USA
| | - J Hoffman
- Washington University, St. Louis, Missouri 63130, USA
| | - K W Murch
- Washington University, St. Louis, Missouri 63130, USA
| | - M Goryachev
- University of Western Australia, Perth, Western Australia 6009, Australia
| | - B T McAllister
- University of Western Australia, Perth, Western Australia 6009, Australia
| | - A Quiskamp
- University of Western Australia, Perth, Western Australia 6009, Australia
| | - C Thomson
- University of Western Australia, Perth, Western Australia 6009, Australia
| | - M E Tobar
- University of Western Australia, Perth, Western Australia 6009, Australia
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