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Ashtari Esfahani A, Böser S, Buzinsky N, Carmona-Benitez MC, Claessens C, de Viveiros L, Doe PJ, Fertl M, Formaggio JA, Gaison JK, Gladstone L, Grando M, Guigue M, Hartse J, Heeger KM, Huyan X, Johnston J, Jones AM, Kazkaz K, LaRoque BH, Li M, Lindman A, Machado E, Marsteller A, Matthé C, Mohiuddin R, Monreal B, Mueller R, Nikkel JA, Novitski E, Oblath NS, Peña JI, Pettus W, Reimann R, Robertson RGH, Rosa De Jesús D, Rybka G, Saldaña L, Schram M, Slocum PL, Stachurska J, Sun YH, Surukuchi PT, Tedeschi JR, Telles AB, Thomas F, Thomas M, Thorne LA, Thümmler T, Tvrznikova L, Van De Pontseele W, VanDevender BA, Weintroub J, Weiss TE, Wendler T, Young A, Zayas E, Ziegler A. Tritium Beta Spectrum Measurement and Neutrino Mass Limit from Cyclotron Radiation Emission Spectroscopy. Phys Rev Lett 2023; 131:102502. [PMID: 37739382 DOI: 10.1103/physrevlett.131.102502] [Citation(s) in RCA: 1] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 03/22/2023] [Revised: 06/26/2023] [Accepted: 07/17/2023] [Indexed: 09/24/2023]
Abstract
The absolute scale of the neutrino mass plays a critical role in physics at every scale, from the subatomic to the cosmological. Measurements of the tritium end-point spectrum have provided the most precise direct limit on the neutrino mass scale. In this Letter, we present advances by Project 8 to the cyclotron radiation emission spectroscopy (CRES) technique culminating in the first frequency-based neutrino mass limit. With only a cm^{3}-scale physical detection volume, a limit of m_{β}<155 eV/c^{2} (152 eV/c^{2}) is extracted from the background-free measurement of the continuous tritium beta spectrum in a Bayesian (frequentist) analysis. Using ^{83m}Kr calibration data, a resolution of 1.66±0.19 eV (FWHM) is measured, the detector response model is validated, and the efficiency is characterized over the multi-keV tritium analysis window. These measurements establish the potential of CRES for a high-sensitivity next-generation direct neutrino mass experiment featuring low background and high resolution.
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Affiliation(s)
- A Ashtari Esfahani
- Center for Experimental Nuclear Physics and Astrophysics and Department of Physics, University of Washington, Seattle, Washington 98195, USA
| | - S Böser
- Institute for Physics, Johannes Gutenberg University Mainz, 55128 Mainz, Germany
| | - N Buzinsky
- Laboratory for Nuclear Science, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M C Carmona-Benitez
- Department of Physics, Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - C Claessens
- Center for Experimental Nuclear Physics and Astrophysics and Department of Physics, University of Washington, Seattle, Washington 98195, USA
- Institute for Physics, Johannes Gutenberg University Mainz, 55128 Mainz, Germany
| | - L de Viveiros
- Department of Physics, Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - P J Doe
- Center for Experimental Nuclear Physics and Astrophysics and Department of Physics, University of Washington, Seattle, Washington 98195, USA
| | - M Fertl
- Institute for Physics, Johannes Gutenberg University Mainz, 55128 Mainz, Germany
| | - J A Formaggio
- Laboratory for Nuclear Science, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - J K Gaison
- Pacific Northwest National Laboratory, Richland, Washington 99354, USA
| | - L Gladstone
- Department of Physics, Case Western Reserve University, Cleveland, Ohio 44106, USA
| | - M Grando
- Pacific Northwest National Laboratory, Richland, Washington 99354, USA
| | - M Guigue
- Laboratoire de Physique Nucléaire et de Hautes Énergies, Sorbonne Université, Université Paris Cité, CNRS/IN2P3, 75005 Paris, France
| | - J Hartse
- Center for Experimental Nuclear Physics and Astrophysics and Department of Physics, University of Washington, Seattle, Washington 98195, USA
| | - K M Heeger
- Wright Laboratory and Department of Physics, Yale University, New Haven, Connecticut 06520, USA
| | - X Huyan
- Pacific Northwest National Laboratory, Richland, Washington 99354, USA
| | - J Johnston
- Laboratory for Nuclear Science, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A M Jones
- Pacific Northwest National Laboratory, Richland, Washington 99354, USA
| | - K Kazkaz
- Lawrence Livermore National Laboratory, Livermore, California 94550, USA
| | - B H LaRoque
- Pacific Northwest National Laboratory, Richland, Washington 99354, USA
| | - M Li
- Laboratory for Nuclear Science, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A Lindman
- Institute for Physics, Johannes Gutenberg University Mainz, 55128 Mainz, Germany
| | - E Machado
- Center for Experimental Nuclear Physics and Astrophysics and Department of Physics, University of Washington, Seattle, Washington 98195, USA
| | - A Marsteller
- Center for Experimental Nuclear Physics and Astrophysics and Department of Physics, University of Washington, Seattle, Washington 98195, USA
| | - C Matthé
- Institute for Physics, Johannes Gutenberg University Mainz, 55128 Mainz, Germany
| | - R Mohiuddin
- Department of Physics, Case Western Reserve University, Cleveland, Ohio 44106, USA
| | - B Monreal
- Department of Physics, Case Western Reserve University, Cleveland, Ohio 44106, USA
| | - R Mueller
- Department of Physics, Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - J A Nikkel
- Wright Laboratory and Department of Physics, Yale University, New Haven, Connecticut 06520, USA
| | - E Novitski
- Center for Experimental Nuclear Physics and Astrophysics and Department of Physics, University of Washington, Seattle, Washington 98195, USA
| | - N S Oblath
- Pacific Northwest National Laboratory, Richland, Washington 99354, USA
| | - J I Peña
- Laboratory for Nuclear Science, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - W Pettus
- Center for Exploration of Energy and Matter and Department of Physics, Indiana University, Bloomington, Indiana 47405, USA
| | - R Reimann
- Institute for Physics, Johannes Gutenberg University Mainz, 55128 Mainz, Germany
| | - R G H Robertson
- Center for Experimental Nuclear Physics and Astrophysics and Department of Physics, University of Washington, Seattle, Washington 98195, USA
| | - D Rosa De Jesús
- Pacific Northwest National Laboratory, Richland, Washington 99354, USA
| | - G Rybka
- Center for Experimental Nuclear Physics and Astrophysics and Department of Physics, University of Washington, Seattle, Washington 98195, USA
| | - L Saldaña
- Wright Laboratory and Department of Physics, Yale University, New Haven, Connecticut 06520, USA
| | - M Schram
- Pacific Northwest National Laboratory, Richland, Washington 99354, USA
| | - P L Slocum
- Wright Laboratory and Department of Physics, Yale University, New Haven, Connecticut 06520, USA
| | - J Stachurska
- Laboratory for Nuclear Science, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - Y-H Sun
- Department of Physics, Case Western Reserve University, Cleveland, Ohio 44106, USA
| | - P T Surukuchi
- Wright Laboratory and Department of Physics, Yale University, New Haven, Connecticut 06520, USA
| | - J R Tedeschi
- Pacific Northwest National Laboratory, Richland, Washington 99354, USA
| | - A B Telles
- Wright Laboratory and Department of Physics, Yale University, New Haven, Connecticut 06520, USA
| | - F Thomas
- Institute for Physics, Johannes Gutenberg University Mainz, 55128 Mainz, Germany
| | - M Thomas
- Pacific Northwest National Laboratory, Richland, Washington 99354, USA
| | - L A Thorne
- Institute for Physics, Johannes Gutenberg University Mainz, 55128 Mainz, Germany
| | - T Thümmler
- Institute of Astroparticle Physics, Karlsruhe Institute of Technology, 76021 Karlsruhe, Germany
| | - L Tvrznikova
- Lawrence Livermore National Laboratory, Livermore, California 94550, USA
| | - W Van De Pontseele
- Laboratory for Nuclear Science, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - B A VanDevender
- Center for Experimental Nuclear Physics and Astrophysics and Department of Physics, University of Washington, Seattle, Washington 98195, USA
- Pacific Northwest National Laboratory, Richland, Washington 99354, USA
| | - J Weintroub
- Center for Astrophysics, Harvard & Smithsonian, Cambridge, Massachusetts 02138, USA
| | - T E Weiss
- Wright Laboratory and Department of Physics, Yale University, New Haven, Connecticut 06520, USA
| | - T Wendler
- Department of Physics, Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - A Young
- Center for Astrophysics, Harvard & Smithsonian, Cambridge, Massachusetts 02138, USA
| | - E Zayas
- Laboratory for Nuclear Science, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A Ziegler
- Department of Physics, Pennsylvania State University, University Park, Pennsylvania 16802, USA
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2
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Cervantes R, Carosi G, Hanretty C, Kimes S, LaRoque BH, Leum G, Mohapatra P, Oblath NS, Ottens R, Park Y, Rybka G, Sinnis J, Yang J. Search for 70 μeV Dark Photon Dark Matter with a Dielectrically Loaded Multiwavelength Microwave Cavity. Phys Rev Lett 2022; 129:201301. [PMID: 36462025 DOI: 10.1103/physrevlett.129.201301] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 04/22/2022] [Revised: 08/29/2022] [Accepted: 09/21/2022] [Indexed: 06/17/2023]
Abstract
Microwave cavities have been deployed to search for bosonic dark matter candidates with masses of a few μeV. However, the sensitivity of these cavity detectors is limited by their volume, and the traditionally employed half-wavelength cavities suffer from a significant volume reduction at higher masses. Axion dark matter experiment (ADMX)-Orpheus mitigates this issue by operating a tunable, dielectrically loaded cavity at a higher-order mode, which allows the detection volume to remain large. The ADMX-Orpheus inaugural run excludes dark photon dark matter with kinetic mixing angle χ>10^{-13} between 65.5 μeV (15.8 GHz) and 69.3 μeV (16.8 GHz), marking the highest-frequency tunable microwave cavity dark matter search to date.
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Affiliation(s)
- R Cervantes
- University of Washington, Seattle, Washington 98195, USA
| | - G Carosi
- Lawrence Livermore National Laboratory, Livermore, California 94550, USA
| | - C Hanretty
- University of Washington, Seattle, Washington 98195, USA
| | - S Kimes
- University of Washington, Seattle, Washington 98195, USA
| | - B H LaRoque
- Pacific Northwest National Laboratory, Richland, Washington 99354, USA
| | - G Leum
- University of Washington, Seattle, Washington 98195, USA
| | - P Mohapatra
- University of Washington, Seattle, Washington 98195, USA
| | - N S Oblath
- Pacific Northwest National Laboratory, Richland, Washington 99354, USA
| | - R Ottens
- University of Washington, Seattle, Washington 98195, USA
| | - Y Park
- University of Washington, Seattle, Washington 98195, USA
| | - G Rybka
- University of Washington, Seattle, Washington 98195, USA
| | - J Sinnis
- University of Washington, Seattle, Washington 98195, USA
| | - J Yang
- University of Washington, Seattle, Washington 98195, USA
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3
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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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4
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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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5
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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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6
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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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7
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Asner DM, Bradley RF, de Viveiros L, Doe PJ, Fernandes JL, Fertl M, Finn EC, Formaggio JA, Furse D, Jones AM, Kofron JN, LaRoque BH, Leber M, McBride EL, Miller ML, Mohanmurthy P, Monreal B, Oblath NS, Robertson RGH, Rosenberg LJ, Rybka G, Rysewyk D, Sternberg MG, Tedeschi JR, Thümmler T, VanDevender BA, Woods NL. Single-Electron Detection and Spectroscopy via Relativistic Cyclotron Radiation. Phys Rev Lett 2015; 114:162501. [PMID: 25955048 DOI: 10.1103/physrevlett.114.162501] [Citation(s) in RCA: 2] [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: 12/24/2014] [Indexed: 06/04/2023]
Abstract
It has been understood since 1897 that accelerating charges must emit electromagnetic radiation. Although first derived in 1904, cyclotron radiation from a single electron orbiting in a magnetic field has never been observed directly. We demonstrate single-electron detection in a novel radio-frequency spectrometer. The relativistic shift in the cyclotron frequency permits a precise electron energy measurement. Precise beta electron spectroscopy from gaseous radiation sources is a key technique in modern efforts to measure the neutrino mass via the tritium decay end point, and this work demonstrates a fundamentally new approach to precision beta spectroscopy for future neutrino mass experiments.
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Affiliation(s)
- D M Asner
- Pacific Northwest National Laboratory, Richland, Washington 99352, USA
| | - R F Bradley
- National Radio Astronomy Observatory, Charlottesville, Virginia 22903, USA
| | - L de Viveiros
- Department of Physics, University of California, Santa Barbara, California 93106, USA
| | - P J Doe
- Center for Experimental Nuclear Physics and Astrophysics, and Department of Physics, University of Washington, Seattle, Washington 98195, USA
| | - J L Fernandes
- Pacific Northwest National Laboratory, Richland, Washington 99352, USA
| | - M Fertl
- Center for Experimental Nuclear Physics and Astrophysics, and Department of Physics, University of Washington, Seattle, Washington 98195, USA
| | - E C Finn
- Pacific Northwest National Laboratory, Richland, Washington 99352, USA
| | - J A Formaggio
- Laboratory for Nuclear Science, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - D Furse
- Laboratory for Nuclear Science, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A M Jones
- Pacific Northwest National Laboratory, Richland, Washington 99352, USA
| | - J N Kofron
- Center for Experimental Nuclear Physics and Astrophysics, and Department of Physics, University of Washington, Seattle, Washington 98195, USA
| | - B H LaRoque
- Department of Physics, University of California, Santa Barbara, California 93106, USA
| | - M Leber
- Department of Physics, University of California, Santa Barbara, California 93106, USA
| | - E L McBride
- Center for Experimental Nuclear Physics and Astrophysics, and Department of Physics, University of Washington, Seattle, Washington 98195, USA
| | - M L Miller
- Center for Experimental Nuclear Physics and Astrophysics, and Department of Physics, University of Washington, Seattle, Washington 98195, USA
| | - P Mohanmurthy
- Laboratory for Nuclear Science, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - B Monreal
- Department of Physics, University of California, Santa Barbara, California 93106, USA
| | - N S Oblath
- Laboratory for Nuclear Science, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - R G H Robertson
- Center for Experimental Nuclear Physics and Astrophysics, and Department of Physics, University of Washington, Seattle, Washington 98195, USA
| | - L J Rosenberg
- Center for Experimental Nuclear Physics and Astrophysics, and Department of Physics, University of Washington, Seattle, Washington 98195, USA
| | - G Rybka
- Center for Experimental Nuclear Physics and Astrophysics, and Department of Physics, University of Washington, Seattle, Washington 98195, USA
| | - D Rysewyk
- Laboratory for Nuclear Science, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M G Sternberg
- Center for Experimental Nuclear Physics and Astrophysics, and Department of Physics, University of Washington, Seattle, Washington 98195, USA
| | - J R Tedeschi
- Pacific Northwest National Laboratory, Richland, Washington 99352, USA
| | - T Thümmler
- Institut für Kernphysik, Karlsruher Institut für Technologie, 76021 Karlsruhe, Germany
| | - B A VanDevender
- Pacific Northwest National Laboratory, Richland, Washington 99352, USA
| | - N L Woods
- Center for Experimental Nuclear Physics and Astrophysics, and Department of Physics, University of Washington, Seattle, Washington 98195, USA
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