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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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Myers TL, Williams RM, Taubman MS, Gmachl C, Capasso F, Sivco DL, Baillargeon JN, Cho AY. Free-running frequency stability of mid-infrared quantum cascade lasers. Opt Lett 2002; 27:170-172. [PMID: 18007745 DOI: 10.1364/ol.27.000170] [Citation(s) in RCA: 8] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/25/2023]
Abstract
The intrinsic frequency fluctuations of two single-mode quantum cascade (QC) distributed-feedback lasers operating continuously at a wavelength of 8.5 mum are reported. A Doppler-limited rovibrational resonance of nitrous oxide is used to transform the frequency noise into measurable intensity fluctuations. The QC lasers, along with recently improved current controllers, exhibit a free-running frequency stability of 150 kHz over a 15-ms time interval.
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6
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Jones DJ, Diddams SA, Taubman MS, Cundiff ST, Ma LS, Hall JL. Frequency comb generation using femtosecond pulses and cross-phase modulation in optical fiber at arbitrary center frequencies. Opt Lett 2000; 25:308-310. [PMID: 18059863 DOI: 10.1364/ol.25.000308] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/25/2023]
Abstract
A technique is presented for generating optical frequency combs centered at arbitrary wavelengths by use of cross-phase modulation (XPM) between a femtosecond pulse train and a cw laser beam by copropagating these signals through an optical fiber. We report results from use of this method to place a 90-MHz frequency comb on an iodine-stabilized Nd:YAG laser at 1064 nm and on a frequency-doubled Nd:YVO(4) laser at 532 nm. XPM is verified to be the comb-generating process, and the width of the frequency comb is measured and compared with theory. The spacing of the frequency comb is compared with the femtosecond source, and a frequency measurement with this comb is demonstrated.
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7
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Abstract
We demonstrate the removal of the dither modulation from an iodine-stabilized He-Ne laser by using a frequency-modulated acousto-optic modulator and feed-forward techniques. This procedure reduces the linewidth of the beat between this laser and a flywheel He-Ne laser from 6 MHz to 8 kHz, the undithered beat linewidth being ~7 kHz. Dither suppression greatly reduces counter errors during beat measurements from stroboscopic effects between the counter's gate and the frequency of the dither modulation and increases the utility of the already formidable array of dithered laser frequency standards by making locking to them an easier task.
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8
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Williams RM, Kelly JF, Hartman JS, Sharpe SW, Taubman MS, Hall JL, Capasso F, Gmachl C, Sivco DL, Baillargeon JN, Cho AY. Kilohertz linewidth from frequency-stabilized mid-infrared quantum cascade lasers. Opt Lett 1999; 24:1844-1846. [PMID: 18079950 DOI: 10.1364/ol.24.001844] [Citation(s) in RCA: 22] [Impact Index Per Article: 0.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/25/2023]
Abstract
Frequency stabilization of mid-IR quantum cascade (QC) lasers to the kilohertz level has been accomplished by use of electronic servo techniques. With this active feedback, an 8.5-microm QC distributed-feedback laser is locked to the side of a rovibrational resonance of nitrous oxide (N(2) O) at 1176.61cm (-1) . A stabilized frequency-noise spectral density of 42Hz/ radicalHz has been measured at 100 kHz; the calculated laser linewidth is 12 kHz.
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9
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White AG, Taubman MS, Ralph TC, Lam PK, McClelland DE, Bachor HA. Experimental test of modular noise propagation theory for quantum optics. Phys Rev A 1996; 54:3400-3404. [PMID: 9913865 DOI: 10.1103/physreva.54.3400] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/22/2023]
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10
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Ralph TC, Taubman MS, White AG, McClelland DE, Bachor HA. Squeezed light from second-harmonic generation: experiment versus theory. Opt Lett 1995; 20:1316-1318. [PMID: 19859511 DOI: 10.1364/ol.20.001316] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/28/2023]
Abstract
We report excellent quantitative agreement between theoretical predictions and experimental observation of squeezing from a singly resonant second-harmonic-generating crystal. Limitations in the noise suppression imposed by the pump laser are explicitly modeled and confirmed by our measurements.
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11
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