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1
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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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2
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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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3
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Khatiwada R, Bowring D, Chou AS, Sonnenschein A, Wester W, Mitchell DV, Braine T, Bartram C, Cervantes R, Crisosto N, Du N, Rosenberg LJ, Rybka G, Yang J, Will D, Kimes S, Carosi G, Woollett N, Durham S, Duffy LD, Bradley R, Boutan C, Jones M, LaRoque BH, Oblath NS, Taubman MS, Tedeschi J, Clarke J, Dove A, Hashim A, Siddiqi I, Stevenson N, Eddins A, O'Kelley SR, Nawaz S, Agrawal A, Dixit AV, Gleason JR, Jois S, Sikivie P, Sullivan NS, Tanner DB, Solomon JA, Lentz E, Daw EJ, Perry MG, Buckley JH, Harrington PM, Henriksen EA, Murch KW, Hilton GC. Axion Dark Matter Experiment: Detailed design and operations. Rev Sci Instrum 2021; 92:124502. [PMID: 34972408 DOI: 10.1063/5.0037857] [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: 11/16/2020] [Accepted: 11/09/2021] [Indexed: 06/14/2023]
Abstract
Axion dark matter experiment ultra-low noise haloscope technology has enabled the successful completion of two science runs (1A and 1B) that looked for dark matter axions in the 2.66-3.1 μeV mass range with Dine-Fischler-Srednicki-Zhitnisky sensitivity [Du et al., Phys. Rev. Lett. 120, 151301 (2018) and Braine et al., Phys. Rev. Lett. 124, 101303 (2020)]. Therefore, it is the most sensitive axion search experiment to date in this mass range. We discuss the technological advances made in the last several years to achieve this sensitivity, which includes the implementation of components, such as the state-of-the-art quantum-noise-limited amplifiers and a dilution refrigerator. Furthermore, we demonstrate the use of a frequency tunable microstrip superconducting quantum interference device amplifier in run 1A, and a Josephson parametric amplifier in run 1B, along with novel analysis tools that characterize the system noise temperature.
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Affiliation(s)
- R Khatiwada
- Department of Physics, Illinois Institute of Technology, Chicago, Illinois 60616, USA and Fermilab Quantum Institute, Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - D Bowring
- Accelerator Physics Division, Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - A S Chou
- Particle Physics Division, Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - A Sonnenschein
- Particle Physics Division, Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - W Wester
- Particle Physics Division, Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - D V Mitchell
- Particle Physics Division, Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - T Braine
- Department of Physics, University of Washington, Seattle, Washington 98195, USA
| | - C Bartram
- Department of Physics, University of Washington, Seattle, Washington 98195, USA
| | - R Cervantes
- Department of Physics, University of Washington, Seattle, Washington 98195, USA
| | - N Crisosto
- Department of Physics, University of Washington, Seattle, Washington 98195, USA
| | - N Du
- Department of Physics, University of Washington, Seattle, Washington 98195, USA
| | - L J Rosenberg
- Department of Physics, University of Washington, Seattle, Washington 98195, USA
| | - G Rybka
- Department of Physics, University of Washington, Seattle, Washington 98195, USA
| | - J Yang
- Department of Physics, University of Washington, Seattle, Washington 98195, USA
| | - D Will
- Department of Physics, University of Washington, Seattle, Washington 98195, USA
| | - S Kimes
- Department of Physics, University of Washington, Seattle, Washington 98195, USA
| | - G Carosi
- Nuclear and Chemical Sciences Division, Lawrence Livermore National Laboratory, Livermore, California 94550, USA
| | - N Woollett
- Nuclear and Chemical Sciences Division, Lawrence Livermore National Laboratory, Livermore, California 94550, USA
| | - S Durham
- Nuclear and Chemical Sciences Division, Lawrence Livermore National Laboratory, Livermore, California 94550, USA
| | - L D Duffy
- Accelerators and Electrodynamics Group, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
| | - R Bradley
- NRAO Technology Center, National Radio Astronomy Observatory, Charlottesville, Virginia 22903, USA
| | - C Boutan
- National Security Directorate, Pacific Northwest National Laboratory, Richland, Washington 99354, USA
| | - M Jones
- National Security Directorate, Pacific Northwest National Laboratory, Richland, Washington 99354, USA
| | - B H LaRoque
- National Security Directorate, Pacific Northwest National Laboratory, Richland, Washington 99354, USA
| | - N S Oblath
- National Security Directorate, Pacific Northwest National Laboratory, Richland, Washington 99354, USA
| | - M S Taubman
- National Security Directorate, Pacific Northwest National Laboratory, Richland, Washington 99354, USA
| | - J Tedeschi
- National Security Directorate, Pacific Northwest National Laboratory, Richland, Washington 99354, USA
| | - John Clarke
- Department of Physics, University of California, Berkeley, California 94720, USA
| | - A Dove
- Department of Physics, University of California, Berkeley, California 94720, USA
| | - A Hashim
- Department of Physics, University of California, Berkeley, California 94720, USA
| | - I Siddiqi
- Department of Physics, University of California, Berkeley, California 94720, USA
| | - N Stevenson
- Department of Physics, University of California, Berkeley, California 94720, USA
| | - A Eddins
- Department of Physics, University of California, Berkeley, California 94720, USA
| | - S R O'Kelley
- Department of Physics, University of California, Berkeley, California 94720, USA
| | - S Nawaz
- Department of Physics, University of California, Berkeley, California 94720, USA
| | - A Agrawal
- Department of Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - A V Dixit
- Department of Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - J R Gleason
- Department of Physics, University of Florida, Gainesville, Florida 32611, USA
| | - S Jois
- Department of Physics, University of Florida, Gainesville, Florida 32611, USA
| | - P Sikivie
- Department of Physics, University of Florida, Gainesville, Florida 32611, USA
| | - N S Sullivan
- Department of Physics, University of Florida, Gainesville, Florida 32611, USA
| | - D B Tanner
- Department of Physics, University of Florida, Gainesville, Florida 32611, USA
| | - J A Solomon
- Department of Physics, University of Florida, Gainesville, Florida 32611, USA
| | - E Lentz
- Department of Physics, University of Göttingen, 37073 Göttingen, Germany
| | - E J Daw
- Department of Physics, University of Sheffield, Sheffield S10 2TN, United Kingdom
| | - M G Perry
- Department of Physics, University of Sheffield, Sheffield S10 2TN, United Kingdom
| | - J H Buckley
- Department of Physics, Washington University, St. Louis, Missouri 63130, USA
| | - P M Harrington
- Department of Physics, Washington University, St. Louis, Missouri 63130, USA
| | - E A Henriksen
- Department of Physics, Washington University, St. Louis, Missouri 63130, USA
| | - K W Murch
- Department of Physics, Washington University, St. Louis, Missouri 63130, USA
| | - G C Hilton
- Physical Measurement Laboratory, National Institute of Standards and Technology, Gaithersburg, Maryland 20899, USA
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4
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Braine T, Cervantes R, Crisosto N, Du N, Kimes S, Rosenberg LJ, Rybka G, Yang J, Bowring D, Chou AS, Khatiwada R, Sonnenschein A, Wester W, Carosi G, Woollett N, Duffy LD, Bradley R, Boutan C, Jones M, LaRoque BH, Oblath NS, Taubman MS, Clarke J, Dove A, Eddins A, O'Kelley SR, Nawaz S, Siddiqi I, Stevenson N, Agrawal A, Dixit AV, Gleason JR, Jois S, Sikivie P, Solomon JA, Sullivan NS, Tanner DB, Lentz E, Daw EJ, Buckley JH, Harrington PM, Henriksen EA, Murch KW. Extended Search for the Invisible Axion with the Axion Dark Matter Experiment. Phys Rev Lett 2020; 124:101303. [PMID: 32216421 DOI: 10.1103/physrevlett.124.101303] [Citation(s) in RCA: 63] [Impact Index Per Article: 15.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/30/2019] [Revised: 01/23/2020] [Accepted: 02/18/2020] [Indexed: 06/10/2023]
Abstract
This Letter reports on a cavity haloscope search for dark matter axions in the Galactic halo in the mass range 2.81-3.31 μeV. This search utilizes the combination of a low-noise Josephson parametric amplifier and a large-cavity haloscope to achieve unprecedented sensitivity across this mass range. This search excludes the full range of axion-photon coupling values predicted in benchmark models of the invisible axion that solve the strong CP problem of quantum chromodynamics.
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Affiliation(s)
- T Braine
- 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
| | - S Kimes
- 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
| | - D Bowring
- Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - A S Chou
- Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - R Khatiwada
- 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
| | - G Carosi
- 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, California 87545, USA
| | - R Bradley
- National Radio Astronomy Observatory, Charlottesville, Virginia 22903, 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
| | - J Clarke
- University of California, Berkeley, California 94720, USA
| | - A Dove
- University of California, Berkeley, California 94720, USA
| | - A Eddins
- University of California, Berkeley, California 94720, USA
| | - S R O'Kelley
- University of California, Berkeley, California 94720, USA
| | - S Nawaz
- University of California, Berkeley, California 94720, USA
| | - I Siddiqi
- University of California, Berkeley, California 94720, USA
| | - N Stevenson
- University of California, Berkeley, California 94720, USA
| | - A Agrawal
- University of Chicago, Chicago, Illinois 60637, USA
| | - A V Dixit
- University of Chicago, Chicago, Illinois 60637, USA
| | - J R Gleason
- 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
| | - J A Solomon
- 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
| | - E J Daw
- University of Sheffield, Sheffield S3 7RH, United Kingdom
| | - J H Buckley
- Washington University, St. Louis, Missouri 63130, USA
| | | | - E A Henriksen
- Washington University, St. Louis, Missouri 63130, USA
| | - K W Murch
- Washington University, St. Louis, Missouri 63130, USA
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5
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Boutan C, Jones M, LaRoque BH, Oblath NS, Cervantes R, Du N, Force N, Kimes S, Ottens R, Rosenberg LJ, Rybka G, Yang J, Carosi G, Woollett N, Bowring D, Chou AS, Khatiwada R, Sonnenschein A, Wester W, Bradley R, Daw EJ, Agrawal A, Dixit AV, Clarke J, O'Kelley SR, Crisosto N, Gleason JR, Jois S, Sikivie P, Stern I, Sullivan NS, Tanner DB, Harrington PM, Lentz E. Piezoelectrically Tuned Multimode Cavity Search for Axion Dark Matter. Phys Rev Lett 2018; 121:261302. [PMID: 30636160 DOI: 10.1103/physrevlett.121.261302] [Citation(s) in RCA: 5] [Impact Index Per Article: 0.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 08/22/2018] [Indexed: 06/09/2023]
Abstract
The μeV axion is a well-motivated extension to the standard model. The Axion Dark Matter eXperiment (ADMX) collaboration seeks to discover this particle by looking for the resonant conversion of dark-matter axions to microwave photons in a strong magnetic field. In this Letter, we report results from a pathfinder experiment, the ADMX "Sidecar," which is designed to pave the way for future, higher mass, searches. This testbed experiment lives inside of and operates in tandem with the main ADMX experiment. The Sidecar experiment excludes masses in three widely spaced frequency ranges (4202-4249, 5086-5799, and 7173-7203 MHz). In addition, Sidecar demonstrates the successful use of a piezoelectric actuator for cavity tuning. Finally, this publication is the first to report data measured using both the TM_{010} and TM_{020} modes.
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Affiliation(s)
- 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
| | - R Cervantes
- University of Washington, Seattle, Washington 98195, USA
| | - N Du
- University of Washington, Seattle, Washington 98195, USA
| | - N Force
- University of Washington, Seattle, Washington 98195, USA
| | - S Kimes
- University of Washington, Seattle, Washington 98195, USA
| | - R Ottens
- 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
| | - G Carosi
- Lawrence Livermore National Laboratory, Livermore, California 94550, USA
| | - N Woollett
- Lawrence Livermore National Laboratory, Livermore, California 94550, USA
| | - D Bowring
- Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - A S Chou
- Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - R Khatiwada
- 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
| | - R Bradley
- National Radio Astronomy Observatory, Charlottesville, Virginia 22903, USA
| | - E J Daw
- University of Sheffield, Sheffield S3 7RH, United Kingdom
| | - A Agrawal
- University of Chicago, Illinois 60637, USA
| | - A V Dixit
- University of Chicago, Illinois 60637, USA
| | - J Clarke
- University of California, Berkeley, California 94720, USA
| | - S R O'Kelley
- University of California, Berkeley, California 94720, USA
| | - N Crisosto
- University of Florida, Gainesville, Florida 32611, USA
| | - J R Gleason
- 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
| | - I Stern
- 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
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6
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Du N, Force N, Khatiwada R, Lentz E, Ottens R, Rosenberg LJ, Rybka G, Carosi G, Woollett N, Bowring D, Chou AS, Sonnenschein A, Wester W, Boutan C, Oblath NS, Bradley R, Daw EJ, Dixit AV, Clarke J, O'Kelley SR, Crisosto N, Gleason JR, Jois S, Sikivie P, Stern I, Sullivan NS, Tanner DB, Hilton GC. Search for Invisible Axion Dark Matter with the Axion Dark Matter Experiment. Phys Rev Lett 2018; 120:151301. [PMID: 29756850 DOI: 10.1103/physrevlett.120.151301] [Citation(s) in RCA: 24] [Impact Index Per Article: 4.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 01/04/2018] [Indexed: 05/27/2023]
Abstract
This Letter reports the results from a haloscope search for dark matter axions with masses between 2.66 and 2.81 μeV. The search excludes the range of axion-photon couplings predicted by plausible models of the invisible axion. This unprecedented sensitivity is achieved by operating a large-volume haloscope at subkelvin temperatures, thereby reducing thermal noise as well as the excess noise from the ultralow-noise superconducting quantum interference device amplifier used for the signal power readout. Ongoing searches will provide nearly definitive tests of the invisible axion model over a wide range of axion masses.
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Affiliation(s)
- N Du
- University of Washington, Seattle, Washington 98195, USA
| | - N Force
- University of Washington, Seattle, Washington 98195, USA
| | - R Khatiwada
- University of Washington, Seattle, Washington 98195, USA
| | - E Lentz
- University of Washington, Seattle, Washington 98195, USA
| | - R Ottens
- 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
| | - G Carosi
- Lawrence Livermore National Laboratory, Livermore, California 94550, USA
| | - N Woollett
- Lawrence Livermore National Laboratory, Livermore, California 94550, USA
| | - D Bowring
- Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - A S Chou
- 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
| | - C Boutan
- Pacific Northwest National Laboratory, Richland, Washington 99354, USA
| | - N S Oblath
- Pacific Northwest National Laboratory, Richland, Washington 99354, USA
| | - R Bradley
- National Radio Astronomy Observatory, Charlottesville, Virginia 22903, USA
| | - E J Daw
- University of Sheffield, Sheffield S3 7RH, United Kingdom
| | - A V Dixit
- University of Chicago, Illinois 60637, USA
| | - J Clarke
- University of California, Berkeley, California 94720, USA
| | - S R O'Kelley
- University of California, Berkeley, California 94720, USA
| | - N Crisosto
- University of Florida, Gainesville, Florida 32611, USA
| | - J R Gleason
- 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
| | - I Stern
- 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
| | - G C Hilton
- National Institute of Standards and Technology, Boulder, Colorado 80305, USA
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Steffen JH, Upadhye A, Baumbaugh A, Chou AS, Mazur PO, Tomlin R, Weltman A, Wester W. Laboratory constraints on chameleon dark energy and power-law fields. Phys Rev Lett 2010; 105:261803. [PMID: 21231645 DOI: 10.1103/physrevlett.105.261803] [Citation(s) in RCA: 5] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/11/2010] [Indexed: 05/30/2023]
Abstract
We report results from a search for chameleon particles created via photon-chameleon oscillations within a magnetic field. This experiment is sensitive to a wide class of unexplored chameleon power-law and dark energy models. These results exclude 5 orders of magnitude in the coupling of chameleons to photons covering a range of 4 orders of magnitude in chameleon effective mass and, for individual models, exclude between 4 and 12 orders of magnitude in chameleon couplings to matter.
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Affiliation(s)
- J H Steffen
- Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
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8
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Sywak MS, Suliburk JW, Chou AS, Sidhu SB, Gill AJ. ES25P�TUMOUR HISTOLOGY DOES NOT PREDICT RESPONSE TO LAPAROSCOPIC ADRENALECTOMY IN CONN'S SYNDROME. ANZ J Surg 2009. [DOI: 10.1111/j.1445-2197.2009.04916_25.x] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/30/2022]
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9
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Chou AS, Wester W, Baumbaugh A, Gustafson HR, Irizarry-Valle Y, Mazur PO, Steffen JH, Tomlin R, Upadhye A, Weltman A, Yang X, Yoo J. Search for chameleon particles using a photon-regeneration technique. Phys Rev Lett 2009; 102:030402. [PMID: 19257328 DOI: 10.1103/physrevlett.102.030402] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 08/01/2008] [Indexed: 05/27/2023]
Abstract
We report the first results from the GammeV search for chameleon particles, which may be created via photon-photon interactions within a strong magnetic field. Chameleons are hypothesized scalar fields that could explain the dark energy problem. We implement a novel technique to create and trap the reflective particles within a jar and to detect them later via their afterglow as they slowly convert back into photons. These measurements provide the first experimental constraints on the couplings of chameleons to photons.
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Affiliation(s)
- A S Chou
- Center for Cosmology and Particle Physics, New York University, 4 Washington Place, New York, New York 10003, USA
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10
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Chou AS, Wester W, Baumbaugh A, Gustafson HR, Irizarry-Valle Y, Mazur PO, Steffen JH, Tomlin R, Yang X, Yoo J. Search for axionlike particles using a variable-baseline photon-regeneration technique. Phys Rev Lett 2008; 100:080402. [PMID: 18352604 DOI: 10.1103/physrevlett.100.080402] [Citation(s) in RCA: 5] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 12/24/2007] [Indexed: 05/26/2023]
Abstract
We report the first results of the GammeV experiment, a search for milli-eV mass particles with axionlike couplings to two photons. The search is performed using a "light shining through a wall" technique where incident photons oscillate into new weakly interacting particles that are able to pass through the wall and subsequently regenerate back into detectable photons. The oscillation baseline of the apparatus is variable, thus allowing probes of different values of particle mass. We find no excess of events above background and are able to constrain the two-photon couplings of possible new scalar (pseudoscalar) particles to be less than 3.1x10;(-7) GeV-1 (3.5x10;(-7) GeV-1) in the limit of massless particles.
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Affiliation(s)
- A S Chou
- Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510, USA
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