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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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To C, Krause E, Rozo E, Wu H, Gruen D, Wechsler RH, Eifler TF, Rykoff ES, Costanzi M, Becker MR, Bernstein GM, Blazek J, Bocquet S, Bridle SL, Cawthon R, Choi A, Crocce M, Davis C, DeRose J, Drlica-Wagner A, Elvin-Poole J, Fang X, Farahi A, Friedrich O, Gatti M, Gaztanaga E, Giannantonio T, Hartley WG, Hoyle B, Jarvis M, MacCrann N, McClintock T, Miranda V, Pereira MES, Park Y, Porredon A, Prat J, Rau MM, Ross AJ, Samuroff S, Sánchez C, Sevilla-Noarbe I, Sheldon E, Troxel MA, Varga TN, Vielzeuf P, Zhang Y, Zuntz J, Abbott TMC, Aguena M, Amon A, Annis J, Avila S, Bertin E, Bhargava S, Brooks D, Burke DL, Carnero Rosell A, Carrasco Kind M, Carretero J, Chang C, Conselice C, da Costa LN, Davis TM, Desai S, Diehl HT, Dietrich JP, Everett S, Evrard AE, Ferrero I, Flaugher B, Fosalba P, Frieman J, García-Bellido J, Gruendl RA, Gutierrez G, Hinton SR, Hollowood DL, Honscheid K, Huterer D, James DJ, Jeltema T, Kron R, Kuehn K, Kuropatkin N, Lima M, Maia MAG, Marshall JL, Menanteau F, Miquel R, Morgan R, Muir J, Myles J, Palmese A, Paz-Chinchón F, Plazas AA, Romer AK, Roodman A, Sanchez E, Santiago B, Scarpine V, Serrano S, Smith M, Suchyta E, Swanson MEC, Tarle G, Thomas D, Tucker DL, Weller J, Wester W, Wilkinson RD. Dark Energy Survey Year 1 Results: Cosmological Constraints from Cluster Abundances, Weak Lensing, and Galaxy Correlations. Phys Rev Lett 2021; 126:141301. [PMID: 33891448 DOI: 10.1103/physrevlett.126.141301] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/06/2020] [Revised: 01/07/2021] [Accepted: 02/23/2021] [Indexed: 06/12/2023]
Abstract
We present the first joint analysis of cluster abundances and auto or cross-correlations of three cosmic tracer fields: galaxy density, weak gravitational lensing shear, and cluster density split by optical richness. From a joint analysis (4×2pt+N) of cluster abundances, three cluster cross-correlations, and the auto correlations of the galaxy density measured from the first year data of the Dark Energy Survey, we obtain Ω_{m}=0.305_{-0.038}^{+0.055} and σ_{8}=0.783_{-0.054}^{+0.064}. This result is consistent with constraints from the DES-Y1 galaxy clustering and weak lensing two-point correlation functions for the flat νΛCDM model. Consequently, we combine cluster abundances and all two-point correlations from across all three cosmic tracer fields (6×2pt+N) and find improved constraints on cosmological parameters as well as on the cluster observable-mass scaling relation. This analysis is an important advance in both optical cluster cosmology and multiprobe analyses of upcoming wide imaging surveys.
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Affiliation(s)
- C To
- Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, California 94305, USA
- Kavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USA
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - E Krause
- Department of Astronomy/Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, Arizona 85721-0065, USA
- Department of Physics, University of Arizona, Tucson, Arizona 85721, USA
| | - E Rozo
- Department of Physics, University of Arizona, Tucson, Arizona 85721, USA
| | - H Wu
- Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USA
- Department of Physics, Boise State University, Boise, Idaho 83725, USA
| | - D Gruen
- Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, California 94305, USA
- Kavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USA
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - R H Wechsler
- Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, California 94305, USA
- Kavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USA
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - T F Eifler
- Department of Astronomy/Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, Arizona 85721-0065, USA
| | - E S Rykoff
- Kavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USA
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - M Costanzi
- INAF-Osservatorio Astronomico di Trieste, via G. B. Tiepolo 11, I-34143 Trieste, Italy
- Institute for Fundamental Physics of the Universe, Via Beirut 2, 34014 Trieste, Italy
| | - M R Becker
- Argonne National Laboratory, 9700 South Cass Avenue, Lemont, Illinois 60439, USA
| | - G M Bernstein
- Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA
| | - J Blazek
- Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USA
- Institute of Physics, Laboratory of Astrophysics, École Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, 1290 Versoix, Switzerland
| | - S Bocquet
- Faculty of Physics, Ludwig-Maximilians-Universität, Scheinerstr. 1, 81679 Munich, Germany
| | - S L Bridle
- Jodrell Bank Center for Astrophysics, School of Physics and Astronomy, University of Manchester, Oxford Road, Manchester, M13 9PL, United Kingdom
| | - R Cawthon
- Physics Department, 2320 Chamberlin Hall, University of Wisconsin-Madison, 1150 University Avenue Madison, Wisconsin 53706-1390
| | - A Choi
- Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USA
| | - M Crocce
- Institut d'Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, Spain
- Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, 08193 Barcelona, Spain
| | - C Davis
- Kavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USA
| | - J DeRose
- Department of Astronomy, University of California, Berkeley, 501 Campbell Hall, Berkeley, California 94720, USA
- Santa Cruz Institute for Particle Physics, Santa Cruz, California 95064, USA
| | - A Drlica-Wagner
- Department of Astronomy and Astrophysics, University of Chicago, Chicago, Illinois 60637, USA
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - J Elvin-Poole
- Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USA
- Department of Physics, The Ohio State University, Columbus, Ohio 43210, USA
| | - X Fang
- Department of Astronomy/Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, Arizona 85721-0065, USA
| | - A Farahi
- Department of Physics, University of Michigan, Ann Arbor, Michigan 48109, USA
| | - O Friedrich
- Kavli Institute for Cosmology, University of Cambridge, Madingley Road, Cambridge CB3 0HA, United Kingdom
| | - M Gatti
- Institut de Física d'Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, 08193 Bellaterra (Barcelona) Spain
| | - E Gaztanaga
- Institut d'Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, Spain
- Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, 08193 Barcelona, Spain
| | - T Giannantonio
- Kavli Institute for Cosmology, University of Cambridge, Madingley Road, Cambridge CB3 0HA, United Kingdom
- Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, United Kingdom
| | - W G Hartley
- Département de Physique Théorique and Center for Astroparticle Physics, Université de Genève, 24 quai Ernest Ansermet, CH-1211 Geneva, Switzerland
- Department of Physics & Astronomy, University College London, Gower Street, London, WC1E 6BT, United Kingdom
- Department of Physics, ETH Zurich, Wolfgang-Pauli-Strasse 16, CH-8093 Zurich, Switzerland
| | - B Hoyle
- Faculty of Physics, Ludwig-Maximilians-Universität, Scheinerstr. 1, 81679 Munich, Germany
- Max Planck Institute for Extraterrestrial Physics, Giessenbachstrasse, 85748 Garching, Germany
- Universitäts-Sternwarte, Fakultät für Physik, Ludwig-Maximilians Universität München, Scheinerstr. 1, 81679 München, Germany
| | - M Jarvis
- Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA
| | - N MacCrann
- Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USA
- Department of Physics, The Ohio State University, Columbus, Ohio 43210, USA
| | - T McClintock
- Department of Physics, University of Arizona, Tucson, Arizona 85721, USA
| | - V Miranda
- Department of Astronomy/Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, Arizona 85721-0065, USA
| | - M E S Pereira
- Department of Physics, University of Michigan, Ann Arbor, Michigan 48109, USA
| | - Y Park
- Department of Physics, University of Arizona, Tucson, Arizona 85721, USA
| | - A Porredon
- Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USA
- Institut d'Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, Spain
- Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, 08193 Barcelona, Spain
| | - J Prat
- Department of Astronomy and Astrophysics, University of Chicago, Chicago, Illinois 60637, USA
| | - M M Rau
- Department of Physics, Carnegie Mellon University, Pittsburgh, Pennsylvania 15312, USA
| | - A J Ross
- Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USA
| | - S Samuroff
- Department of Physics, Carnegie Mellon University, Pittsburgh, Pennsylvania 15312, USA
| | - C Sánchez
- Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA
| | - I Sevilla-Noarbe
- Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain
| | - E Sheldon
- Brookhaven National Laboratory, Bldg 510, Upton, New York 11973, USA
| | - M A Troxel
- Department of Physics, Duke University Durham, North Carolina 27708, USA
| | - T N Varga
- Max Planck Institute for Extraterrestrial Physics, Giessenbachstrasse, 85748 Garching, Germany
- Universitäts-Sternwarte, Fakultät für Physik, Ludwig-Maximilians Universität München, Scheinerstr. 1, 81679 München, Germany
| | - P Vielzeuf
- Institut de Física d'Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, 08193 Bellaterra (Barcelona) Spain
| | - Y Zhang
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - J Zuntz
- Institute for Astronomy, University of Edinburgh, Edinburgh EH9 3HJ, United Kingdom
| | - T M C Abbott
- Cerro Tololo Inter-American Observatory, NSF's National Optical-Infrared Astronomy Research Laboratory, Casilla 603, La Serena, Chile
| | - M Aguena
- Departamento de Física Matemática, Instituto de Física, Universidade de São Paulo, CP 66318, São Paulo, SP, 05314-970, Brazil
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
| | - A Amon
- Kavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USA
| | - J Annis
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - S Avila
- Instituto de Fisica Teorica UAM/CSIC, Universidad Autonoma de Madrid, 28049 Madrid, Spain
| | - E Bertin
- CNRS, UMR 7095, Institut d'Astrophysique de Paris, F-75014, Paris, France
- Sorbonne Universités, UPMC Univ Paris 06, UMR 7095, Institut d'Astrophysique de Paris, F-75014, Paris, France
| | - S Bhargava
- Department of Physics and Astronomy, Pevensey Building, University of Sussex, Brighton, BN1 9QH, United Kingdom
| | - D Brooks
- Department of Physics & Astronomy, University College London, Gower Street, London, WC1E 6BT, United Kingdom
| | - D L Burke
- Kavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USA
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - A Carnero Rosell
- Instituto de Astrofisica de Canarias, E-38205 La Laguna, Tenerife, Spain
- Universidad de La Laguna, Dpto. Astrofsica, E-38206 La Laguna, Tenerife, Spain
| | - M Carrasco Kind
- Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 W. Green Street, Urbana, Illinois 61801, USA
- National Center for Supercomputing Applications, 1205 West Clark St., Urbana, Illinois 61801, USA
| | - J Carretero
- Institut de Física d'Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, 08193 Bellaterra (Barcelona) Spain
| | - C Chang
- Department of Astronomy and Astrophysics, University of Chicago, Chicago, Illinois 60637, USA
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - C Conselice
- Jodrell Bank Center for Astrophysics, School of Physics and Astronomy, University of Manchester, Oxford Road, Manchester, M13 9PL, United Kingdom
- University of Nottingham, School of Physics and Astronomy, Nottingham NG7 2RD, United Kingdom
| | - L N da Costa
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
- Observatório Nacional, Rua Gal. José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
| | - T M Davis
- School of Mathematics and Physics, University of Queensland, Brisbane, QLD 4072, Australia
| | - S Desai
- Department of Physics, IIT Hyderabad, Kandi, Telangana 502285, India
| | - H T Diehl
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - J P Dietrich
- Faculty of Physics, Ludwig-Maximilians-Universität, Scheinerstr. 1, 81679 Munich, Germany
| | - S Everett
- Santa Cruz Institute for Particle Physics, Santa Cruz, California 95064, USA
| | - A E Evrard
- Department of Physics, University of Michigan, Ann Arbor, Michigan 48109, USA
- Department of Astronomy, University of Michigan, Ann Arbor, Michigan 48109, USA
| | - I Ferrero
- Institute of Theoretical Astrophysics, University of Oslo. P.O. Box 1029 Blindern, NO-0315 Oslo, Norway
| | - B Flaugher
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - P Fosalba
- Institut d'Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, Spain
- Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, 08193 Barcelona, Spain
| | - J Frieman
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - J García-Bellido
- Instituto de Fisica Teorica UAM/CSIC, Universidad Autonoma de Madrid, 28049 Madrid, Spain
| | - R A Gruendl
- Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 W. Green Street, Urbana, Illinois 61801, USA
- National Center for Supercomputing Applications, 1205 West Clark St., Urbana, Illinois 61801, USA
| | - G Gutierrez
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - S R Hinton
- School of Mathematics and Physics, University of Queensland, Brisbane, QLD 4072, Australia
| | - D L Hollowood
- Santa Cruz Institute for Particle Physics, Santa Cruz, California 95064, USA
| | - K Honscheid
- Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USA
- Department of Physics, The Ohio State University, Columbus, Ohio 43210, USA
| | - D Huterer
- Department of Physics, University of Michigan, Ann Arbor, Michigan 48109, USA
| | - D J James
- Center for Astrophysics | Harvard & Smithsonian, 60 Garden Street, Cambridge, Massachusetts 02138, USA
| | - T Jeltema
- Santa Cruz Institute for Particle Physics, Santa Cruz, California 95064, USA
| | - R Kron
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - K Kuehn
- Australian Astronomical Optics, Macquarie University, North Ryde, New South Wales 2113, Australia
- Lowell Observatory, 1400 Mars Hill Rd, Flagstaff, Arizona 86001, USA
| | - N Kuropatkin
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - M Lima
- Departamento de Física Matemática, Instituto de Física, Universidade de São Paulo, CP 66318, São Paulo, SP, 05314-970, Brazil
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
| | - M A G Maia
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
- Observatório Nacional, Rua Gal. José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
| | - J L Marshall
- George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, and Department of Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - F Menanteau
- Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 W. Green Street, Urbana, Illinois 61801, USA
- National Center for Supercomputing Applications, 1205 West Clark St., Urbana, Illinois 61801, USA
| | - R Miquel
- Institut de Física d'Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, 08193 Bellaterra (Barcelona) Spain
- Institució Catalana de Recerca i Estudis Avanćats, E-08010 Barcelona, Spain
| | - R Morgan
- Physics Department, 2320 Chamberlin Hall, University of Wisconsin-Madison, 1150 University Avenue Madison, Wisconsin 53706-1390
| | - J Muir
- Kavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USA
| | - J Myles
- Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, California 94305, USA
| | - A Palmese
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - F Paz-Chinchón
- Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, United Kingdom
- National Center for Supercomputing Applications, 1205 West Clark St., Urbana, Illinois 61801, USA
| | - A A Plazas
- Department of Astrophysical Sciences, Princeton University, Peyton Hall, Princeton, New Jersey 08544, USA
| | - A K Romer
- Department of Physics and Astronomy, Pevensey Building, University of Sussex, Brighton, BN1 9QH, United Kingdom
| | - A Roodman
- Kavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USA
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - E Sanchez
- Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain
| | - B Santiago
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
- Instituto de Física, UFRGS, Caixa Postal 15051, Porto Alegre, RS-91501-970, Brazil
| | - V Scarpine
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - S Serrano
- Institut d'Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, Spain
- Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, 08193 Barcelona, Spain
| | - M Smith
- School of Physics and Astronomy, University of Southampton, Southampton, SO17 1BJ, United Kingdom
| | - E Suchyta
- Computer Science and Mathematics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831
| | - M E C Swanson
- National Center for Supercomputing Applications, 1205 West Clark St., Urbana, Illinois 61801, USA
| | - G Tarle
- Department of Physics, University of Michigan, Ann Arbor, Michigan 48109, USA
| | - D Thomas
- Institute of Cosmology and Gravitation, University of Portsmouth, Portsmouth, PO1 3FX, United Kingdom
| | - D L Tucker
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - J Weller
- Max Planck Institute for Extraterrestrial Physics, Giessenbachstrasse, 85748 Garching, Germany
- Universitäts-Sternwarte, Fakultät für Physik, Ludwig-Maximilians Universität München, Scheinerstr. 1, 81679 München, Germany
| | - W Wester
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - R D Wilkinson
- Department of Physics and Astronomy, Pevensey Building, University of Sussex, Brighton, BN1 9QH, United Kingdom
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5
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Nadler EO, Drlica-Wagner A, Bechtol K, Mau S, Wechsler RH, Gluscevic V, Boddy K, Pace AB, Li TS, McNanna M, Riley AH, García-Bellido J, Mao YY, Green G, Burke DL, Peter A, Jain B, Abbott TMC, Aguena M, Allam S, Annis J, Avila S, Brooks D, Carrasco Kind M, Carretero J, Costanzi M, da Costa LN, De Vicente J, Desai S, Diehl HT, Doel P, Everett S, Evrard AE, Flaugher B, Frieman J, Gerdes DW, Gruen D, Gruendl RA, Gschwend J, Gutierrez G, Hinton SR, Honscheid K, Huterer D, James DJ, Krause E, Kuehn K, Kuropatkin N, Lahav O, Maia MAG, Marshall JL, Menanteau F, Miquel R, Palmese A, Paz-Chinchón F, Plazas AA, Romer AK, Sanchez E, Scarpine V, Serrano S, Sevilla-Noarbe I, Smith M, Soares-Santos M, Suchyta E, Swanson MEC, Tarle G, Tucker DL, Walker AR, Wester W. Constraints on Dark Matter Properties from Observations of Milky Way Satellite Galaxies. Phys Rev Lett 2021; 126:091101. [PMID: 33750144 DOI: 10.1103/physrevlett.126.091101] [Citation(s) in RCA: 6] [Impact Index Per Article: 2.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 07/30/2020] [Revised: 12/12/2020] [Accepted: 01/27/2021] [Indexed: 06/12/2023]
Abstract
We perform a comprehensive study of Milky Way (MW) satellite galaxies to constrain the fundamental properties of dark matter (DM). This analysis fully incorporates inhomogeneities in the spatial distribution and detectability of MW satellites and marginalizes over uncertainties in the mapping between galaxies and DM halos, the properties of the MW system, and the disruption of subhalos by the MW disk. Our results are consistent with the cold, collisionless DM paradigm and yield the strongest cosmological constraints to date on particle models of warm, interacting, and fuzzy dark matter. At 95% confidence, we report limits on (i) the mass of thermal relic warm DM, m_{WDM}>6.5 keV (free-streaming length, λ_{fs}≲10h^{-1} kpc), (ii) the velocity-independent DM-proton scattering cross section, σ_{0}<8.8×10^{-29} cm^{2} for a 100 MeV DM particle mass [DM-proton coupling, c_{p}≲(0.3 GeV)^{-2}], and (iii) the mass of fuzzy DM, m_{ϕ}>2.9×10^{-21} eV (de Broglie wavelength, λ_{dB}≲0.5 kpc). These constraints are complementary to other observational and laboratory constraints on DM properties.
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Affiliation(s)
- E O Nadler
- Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, California 94305, USA
- Kavli Institute for Particle Astrophysics and Cosmology, P.O. Box 2450, Stanford University, Stanford, California 94305, USA
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - A Drlica-Wagner
- Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510, USA
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
- Department of Astronomy and Astrophysics, University of Chicago, Chicago, Illinois 60637, USA
| | - K Bechtol
- Physics Department, 2320 Chamberlin Hall, University of Wisconsin-Madison, 1150 University Avenue, Madison, Wisconsin 53706-1390, USA
| | - S Mau
- Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, California 94305, USA
- Kavli Institute for Particle Astrophysics and Cosmology, P.O. Box 2450, Stanford University, Stanford, California 94305, USA
| | - R H Wechsler
- Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, California 94305, USA
- Kavli Institute for Particle Astrophysics and Cosmology, P.O. Box 2450, Stanford University, Stanford, California 94305, USA
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - V Gluscevic
- University of Southern California, Department of Physics and Astronomy, 825 Bloom Walk ACB 439, Los Angeles, California 90089-0484, USA
| | - K Boddy
- Theory Group, Department of Physics, The University of Texas at Austin, Austin, Texas 78712, USA
| | - A B Pace
- Department of Physics, Carnegie Mellon University, Pittsburgh, Pennsylvania 15312, USA
| | - T S Li
- Department of Astrophysical Sciences, Princeton University, Peyton Hall, Princeton, New Jersey 08544, USA
- Observatories of the Carnegie Institution for Science, 813 Santa Barbara Street, Pasadena, California 91101, USA
| | - M McNanna
- Physics Department, 2320 Chamberlin Hall, University of Wisconsin-Madison, 1150 University Avenue, Madison, Wisconsin 53706-1390, USA
| | - A H Riley
- George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, and Department of Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - J García-Bellido
- Instituto de Fisica Teorica UAM/CSIC, Universidad Autonoma de Madrid, 28049 Madrid, Spain
| | - Y-Y Mao
- Department of Physics and Astronomy, Rutgers, The State University of New Jersey, Piscataway, New Jersey 08854, USA
| | - G Green
- Max Planck Institute for Astronomy, Königstuhl 17 D-69117, Heidelberg, Germany
| | - D L Burke
- Kavli Institute for Particle Astrophysics and Cosmology, P.O. Box 2450, Stanford University, Stanford, California 94305, USA
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - A Peter
- Department of Physics, The Ohio State University, Columbus, Ohio 43210, USA
- Department of Astronomy, The Ohio State University, Columbus, Ohio 43210, USA
- Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USA
| | - B Jain
- Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA
| | - T M C Abbott
- Cerro Tololo Inter-American Observatory, NSF's National Optical-Infrared Astronomy Research Laboratory, Casilla 603, La Serena, Chile
| | - M Aguena
- Departamento de Física Matemática, Instituto de Física, Universidade de São Paulo, CP 66318, São Paulo, SP, 05314-970, Brazil
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
| | - S Allam
- Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510, USA
| | - J Annis
- Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510, USA
| | - S Avila
- Instituto de Fisica Teorica UAM/CSIC, Universidad Autonoma de Madrid, 28049 Madrid, Spain
| | - D Brooks
- Department of Physics and Astronomy, University College London, Gower Street, London, WC1E 6BT, United Kingdom
| | - M Carrasco Kind
- Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 West Green Street, Urbana, Illinois 61801, USA
- National Center for Supercomputing Applications, 1205 West Clark Street, Urbana, Illinois 61801, USA
| | - J Carretero
- Institut de Física d'Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, 08193 Bellaterra (Barcelona), Spain
| | - M Costanzi
- INAF-Osservatorio Astronomico di Trieste, via G.B. Tiepolo 11, I-34143 Trieste, Italy
- Institute for Fundamental Physics of the Universe, Via Beirut 2, 34014 Trieste, Italy
| | - L N da Costa
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
- Observatório Nacional, Rua Gal. José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
| | - J De Vicente
- Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain
| | - S Desai
- Department of Physics, IIT Hyderabad, Kandi, Telangana 502285, India
| | - H T Diehl
- Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510, USA
| | - P Doel
- Department of Physics and Astronomy, University College London, Gower Street, London, WC1E 6BT, United Kingdom
| | - S Everett
- Santa Cruz Institute for Particle Physics, Santa Cruz, California 95064, USA
| | - A E Evrard
- Department of Astronomy, University of Michigan, Ann Arbor, Michigan 48109, USA
- Department of Physics, University of Michigan, Ann Arbor, Michigan 48109, USA
| | - B Flaugher
- Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510, USA
| | - J Frieman
- Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510, USA
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - D W Gerdes
- Department of Astronomy, University of Michigan, Ann Arbor, Michigan 48109, USA
- Department of Physics, University of Michigan, Ann Arbor, Michigan 48109, USA
| | - D Gruen
- Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, California 94305, USA
- Kavli Institute for Particle Astrophysics and Cosmology, P.O. Box 2450, Stanford University, Stanford, California 94305, USA
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - R A Gruendl
- Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 West Green Street, Urbana, Illinois 61801, USA
- National Center for Supercomputing Applications, 1205 West Clark Street, Urbana, Illinois 61801, USA
| | - J Gschwend
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
- Observatório Nacional, Rua Gal. José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
| | - G Gutierrez
- Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510, USA
| | - S R Hinton
- School of Mathematics and Physics, University of Queensland, Brisbane, Queensland 4072, Australia
| | - K Honscheid
- Department of Physics, The Ohio State University, Columbus, Ohio 43210, USA
- Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USA
| | - D Huterer
- Department of Physics, University of Michigan, Ann Arbor, Michigan 48109, USA
| | - D J James
- Center for Astrophysics, Harvard and Smithsonian, 60 Garden Street, Cambridge, Massachusetts 02138, USA
| | - E Krause
- Department of Astronomy/Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, Arizona 85721-0065, USA
| | - K Kuehn
- Australian Astronomical Optics, Macquarie University, North Ryde, New South Wales 2113, Australia
- Lowell Observatory, 1400 Mars Hill Road, Flagstaff, Arizona 86001, USA
| | - N Kuropatkin
- Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510, USA
| | - O Lahav
- Department of Physics and Astronomy, University College London, Gower Street, London, WC1E 6BT, United Kingdom
| | - M A G Maia
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
- Observatório Nacional, Rua Gal. José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
| | - J L Marshall
- George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, and Department of Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - F Menanteau
- Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 West Green Street, Urbana, Illinois 61801, USA
- National Center for Supercomputing Applications, 1205 West Clark Street, Urbana, Illinois 61801, USA
| | - R Miquel
- Institut de Física d'Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, 08193 Bellaterra (Barcelona), Spain
- Institució Catalana de Recerca i Estudis Avançats, E-08010 Barcelona, Spain
| | - A Palmese
- Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510, USA
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - F Paz-Chinchón
- National Center for Supercomputing Applications, 1205 West Clark Street, Urbana, Illinois 61801, USA
- Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, United Kingdom
| | - A A Plazas
- Department of Astrophysical Sciences, Princeton University, Peyton Hall, Princeton, New Jersey 08544, USA
| | - A K Romer
- Department of Physics and Astronomy, Pevensey Building, University of Sussex, Brighton, BN1 9QH, United Kingdom
| | - E Sanchez
- Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain
| | - V Scarpine
- Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510, USA
| | - S Serrano
- Institut d'Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, Spain
- Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, 08193 Barcelona, Spain
| | - I Sevilla-Noarbe
- Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain
| | - M Smith
- School of Physics and Astronomy, University of Southampton, Southampton, SO17 1BJ, United Kingdom
| | - M Soares-Santos
- Brandeis University, Physics Department, 415 South Street, Waltham, Massachusetts 02453, USA
| | - E Suchyta
- Computer Science and Mathematics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA
| | - M E C Swanson
- National Center for Supercomputing Applications, 1205 West Clark Street, Urbana, Illinois 61801, USA
| | - G Tarle
- Department of Physics, University of Michigan, Ann Arbor, Michigan 48109, USA
| | - D L Tucker
- Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510, USA
| | - A R Walker
- Cerro Tololo Inter-American Observatory, NSF's National Optical-Infrared Astronomy Research Laboratory, Casilla 603, La Serena, Chile
| | - W Wester
- Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510, USA
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6
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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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7
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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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8
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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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9
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Kessler R, Marriner J, Childress M, Covarrubias R, D’Andrea CB, Finley DA, Fischer J, Foley RJ, Goldstein D, Gupta RR, Kuehn K, Marcha M, Nichol RC, Papadopoulos A, Sako M, Scolnic D, Smith M, Sullivan M, Wester W, Yuan F, Abbott T, Abdalla FB, Allam S, Benoit-Lévy A, Bernstein GM, Bertin E, Brooks D, Rosell AC, Kind MC, Castander FJ, Crocce M, Costa LND, Desai S, Diehl HT, Eifler TF, Neto AF, Flaugher B, Frieman J, Gerdes DW, Gruen D, Gruendl RA, Honscheid K, James DJ, Kuropatkin N, Li TS, Maia MAG, Marshall JL, Martini P, Miller CJ, Miquel R, Nord B, Ogando R, Plazas AA, Reil K, Romer AK, Roodman A, Sanchez E, Sevilla-Noarbe I, Smith RC, Soares-Santos M, Sobreira F, Tarle G, Thaler J, Thomas RC, Tucker D, Walker AR. THE DIFFERENCE IMAGING PIPELINE FOR THE TRANSIENT SEARCH IN THE DARK ENERGY SURVEY. ACTA ACUST UNITED AC 2015. [DOI: 10.1088/0004-6256/150/6/172] [Citation(s) in RCA: 106] [Impact Index Per Article: 11.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/11/2022]
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10
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Flaugher B, Diehl HT, Honscheid K, Abbott TMC, Alvarez O, Angstadt R, Annis JT, Antonik M, Ballester O, Beaufore L, Bernstein GM, Bernstein RA, Bigelow B, Bonati M, Boprie D, Brooks D, Buckley-Geer EJ, Campa J, Cardiel-Sas L, Castander FJ, Castilla J, Cease H, Cela-Ruiz JM, Chappa S, Chi E, Cooper C, da Costa LN, Dede E, Derylo G, DePoy DL, de Vicente J, Doel P, Drlica-Wagner A, Eiting J, Elliott AE, Emes J, Estrada J, Fausti Neto A, Finley DA, Flores R, Frieman J, Gerdes D, Gladders MD, Gregory B, Gutierrez GR, Hao J, Holland SE, Holm S, Huffman D, Jackson C, James DJ, Jonas M, Karcher A, Karliner I, Kent S, Kessler R, Kozlovsky M, Kron RG, Kubik D, Kuehn K, Kuhlmann S, Kuk K, Lahav O, Lathrop A, Lee J, Levi ME, Lewis P, Li TS, Mandrichenko I, Marshall JL, Martinez G, Merritt KW, Miquel R, Muñoz F, Neilsen EH, Nichol RC, Nord B, Ogando R, Olsen J, Palaio N, Patton K, Peoples J, Plazas AA, Rauch J, Reil K, Rheault JP, Roe NA, Rogers H, Roodman A, Sanchez E, Scarpine V, Schindler RH, Schmidt R, Schmitt R, Schubnell M, Schultz K, Schurter P, Scott L, Serrano S, Shaw TM, Smith RC, Soares-Santos M, Stefanik A, Stuermer W, Suchyta E, Sypniewski A, Tarle G, Thaler J, Tighe R, Tran C, Tucker D, Walker AR, Wang G, Watson M, Weaverdyck C, Wester W, Woods R, Yanny B. THE DARK ENERGY CAMERA. ACTA ACUST UNITED AC 2015. [DOI: 10.1088/0004-6256/150/5/150] [Citation(s) in RCA: 580] [Impact Index Per Article: 64.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/11/2022]
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11
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Goldstein DA, D’Andrea CB, Fischer JA, Foley RJ, Gupta RR, Kessler R, Kim AG, Nichol RC, Nugent PE, Papadopoulos A, Sako M, Smith M, Sullivan M, Thomas RC, Wester W, Wolf RC, Abdalla FB, Banerji M, Benoit-Lévy A, Bertin E, Brooks D, Rosell AC, Castander FJ, Costa LND, Covarrubias R, DePoy DL, Desai S, Diehl HT, Doel P, Eifler TF, Neto AF, Finley DA, Flaugher B, Fosalba P, Frieman J, Gerdes D, Gruen D, Gruendl RA, James D, Kuehn K, Kuropatkin N, Lahav O, Li TS, Maia MAG, Makler M, March M, Marshall JL, Martini P, Merritt KW, Miquel R, Nord B, Ogando R, Plazas AA, Romer AK, Roodman A, Sanchez E, Scarpine V, Schubnell M, Sevilla-Noarbe I, Smith RC, Soares-Santos M, Sobreira F, Suchyta E, Swanson MEC, Tarle G, Thaler J, Walker AR. AUTOMATED TRANSIENT IDENTIFICATION IN THE DARK ENERGY SURVEY. ACTA ACUST UNITED AC 2015. [DOI: 10.1088/0004-6256/150/3/82] [Citation(s) in RCA: 94] [Impact Index Per Article: 10.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/11/2022]
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12
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Drlica-Wagner A, Albert A, Bechtol K, Wood M, Strigari L, Sánchez-Conde M, Baldini L, Essig R, Cohen-Tanugi J, Anderson B, Bellazzini R, Bloom ED, Caputo R, Cecchi C, Charles E, Chiang J, Angelis AD, Funk S, Fusco P, Gargano F, Giglietto N, Giordano F, Guiriec S, Gustafsson M, Kuss M, Loparco F, Lubrano P, Mirabal N, Mizuno T, Morselli A, Ohsugi T, Orlando E, Persic M, Rainò S, Sehgal N, Spada F, Suson DJ, Zaharijas G, Zimmer S, Abbott T, Allam S, Balbinot E, Bauer AH, Benoit-Lévy A, Bernstein RA, Bernstein GM, Bertin E, Brooks D, Buckley-Geer E, Burke DL, Rosell AC, Castander FJ, Covarrubias R, D’Andrea CB, Costa LND, DePoy DL, Desai S, Diehl HT, Cunha CE, Eifler TF, Estrada J, Evrard AE, Neto AF, Fernandez E, Finley DA, Flaugher B, Frieman J, Gaztanaga E, Gerdes D, Gruen D, Gruendl RA, Gutierrez G, Honscheid K, Jain B, James D, Jeltema T, Kent S, Kron R, Kuehn K, Kuropatkin N, Lahav O, Li TS, Luque E, Maia MAG, Makler M, March M, Marshall J, Martini P, Merritt KW, Miller C, Miquel R, Mohr J, Neilsen E, Nord B, Ogando R, Peoples J, Petravick D, Pieres A, Plazas AA, Queiroz A, Romer AK, Roodman A, Rykoff ES, Sako M, Sanchez E, Santiago B, Scarpine V, Schubnell M, Sevilla I, Smith RC, Soares-Santos M, Sobreira F, Suchyta E, Swanson MEC, Tarle G, Thaler J, Thomas D, Tucker D, Walker AR, Wechsler RH, Wester W, Williams P, Yanny B, Zuntz J. SEARCH FOR GAMMA-RAY EMISSION FROM DES DWARF SPHEROIDAL GALAXY CANDIDATES WITH
FERMI
-LAT DATA. ACTA ACUST UNITED AC 2015. [DOI: 10.1088/2041-8205/809/1/l4] [Citation(s) in RCA: 119] [Impact Index Per Article: 13.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/11/2022]
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13
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Simon JD, Drlica-Wagner A, Li TS, Nord B, Geha M, Bechtol K, Balbinot E, Buckley-Geer E, Lin H, Marshall J, Santiago B, Strigari L, Wang M, Wechsler RH, Yanny B, Abbott T, Bauer AH, Bernstein GM, Bertin E, Brooks D, Burke DL, Capozzi D, Rosell AC, Kind MC, D’Andrea CB, Costa LND, DePoy DL, Desai S, Diehl HT, Dodelson S, Cunha CE, Estrada J, Evrard AE, Neto AF, Fernandez E, Finley DA, Flaugher B, Frieman J, Gaztanaga E, Gerdes D, Gruen D, Gruendl RA, Honscheid K, James D, Kent S, Kuehn K, Kuropatkin N, Lahav O, Maia MAG, March M, Martini P, Miller CJ, Miquel R, Ogando R, Romer AK, Roodman A, Rykoff ES, Sako M, Sanchez E, Schubnell M, Sevilla I, Smith RC, Soares-Santos M, Sobreira F, Suchyta E, Swanson MEC, Tarle G, Thaler J, Tucker D, Vikram V, Walker AR, Wester W. STELLAR KINEMATICS AND METALLICITIES IN THE ULTRA-FAINT DWARF GALAXY RETICULUM II. ACTA ACUST UNITED AC 2015. [DOI: 10.1088/0004-637x/808/1/95] [Citation(s) in RCA: 109] [Impact Index Per Article: 12.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/11/2022]
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14
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Bechtol K, Drlica-Wagner A, Balbinot E, Pieres A, Simon JD, Yanny B, Santiago B, Wechsler RH, Frieman J, Walker AR, Williams P, Rozo E, Rykoff ES, Queiroz A, Luque E, Benoit-Lévy A, Tucker D, Sevilla I, Gruendl RA, Costa LND, Neto AF, Maia MAG, Abbott T, Allam S, Armstrong R, Bauer AH, Bernstein GM, Bernstein RA, Bertin E, Brooks D, Buckley-Geer E, Burke DL, Rosell AC, Castander FJ, Covarrubias R, D’Andrea CB, DePoy DL, Desai S, Diehl HT, Eifler TF, Estrada J, Evrard AE, Fernandez E, Finley DA, Flaugher B, Gaztanaga E, Gerdes D, Girardi L, Gladders M, Gruen D, Gutierrez G, Hao J, Honscheid K, Jain B, James D, Kent S, Kron R, Kuehn K, Kuropatkin N, Lahav O, Li TS, Lin H, Makler M, March M, Marshall J, Martini P, Merritt KW, Miller C, Miquel R, Mohr J, Neilsen E, Nichol R, Nord B, Ogando R, Peoples J, Petravick D, Plazas AA, Romer AK, Roodman A, Sako M, Sanchez E, Scarpine V, Schubnell M, Smith RC, Soares-Santos M, Sobreira F, Suchyta E, Swanson MEC, Tarle G, Thaler J, Thomas D, Wester W, Zuntz J. EIGHT NEW MILKY WAY COMPANIONS DISCOVERED IN FIRST-YEAR DARK ENERGY SURVEY DATA. ACTA ACUST UNITED AC 2015. [DOI: 10.1088/0004-637x/807/1/50] [Citation(s) in RCA: 401] [Impact Index Per Article: 44.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/12/2022]
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15
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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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16
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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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17
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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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18
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Acosta D, Affolder T, Ahn MH, Akimoto T, Albrow MG, Ambrose D, Amerio S, Amidei D, Anastassov A, Anikeev K, Annovi A, Antos J, Aoki M, Apollinari G, Arguin JF, Arisawa T, Artikov A, Asakawa T, Ashmanskas W, Attal A, Azfar F, Azzi-Bacchetta P, Bacchetta N, Bachacou H, Badgett W, Bailey S, Barbaro-Galtieri A, Barker G, Barnes VE, Barnett BA, Baroiant S, Barone M, Bauer G, Bedeschi F, Behari S, Belforte S, Bell WH, Bellettini G, Bellinger J, Benjamin D, Beretvas A, Bhatti A, Binkley M, Bisello D, Bishai M, Blair RE, Blocker C, Bloom K, Blumenfeld B, Bocci A, Bodek A, Bolla G, Bolshov A, Booth PSL, Bortoletto D, Boudreau J, Bourov S, Bromberg C, Brubaker E, Budagov J, Budd HS, Burkett K, Busetto G, Bussey P, Byrum KL, Cabrera S, Calafiura P, Campanelli M, Campbell M, Canepa A, Carlsmith D, Carron S, Carosi R, Casarsa M, Castro A, Catastini P, Cauz D, Cerri A, Cerri C, Cerrito L, Chapman J, Chen C, Chen YC, Chertok M, Chiarelli G, Chlachidze G, Chlebana F, Cho K, Chokheli D, Chu ML, Chung JY, Chung WH, Chung YS, Ciobanu CI, Ciocci MA, Clark AG, Clark D, Coca MN, Connolly A, Convery ME, Conway J, Cordelli M, Cortiana G, Cranshaw J, Culbertson R, Currat C, Cyr D, Dagenhart D, DaRonco S, D'Auria S, de Barbaro P, De Cecco S, De Lentdecker G, Dell'Agnello S, Dell'Orso M, Demers S, Demortier L, Deninno M, De Pedis D, Derwent PF, Dionisi C, Dittmann JR, Doksus P, Dominguez A, Donati S, D'Onofrio M, Dorigo T, Drollinger V, Ebina K, Eddy N, Ely R, Erbacher R, Erdmann M, Errede D, Errede S, Eusebi R, Fang HC, Farrington S, Fedorko I, Feild RG, Feindt M, Fernandez JP, Ferretti C, Field RD, Fiori I, Flanagan G, Flaugher B, Flores-Castillo LR, Foland A, Forrester S, Foster GW, Franklin M, Frisch H, Fujii Y, Furic I, Gaijar A, Gallas A, Gallinaro M, Galyardt J, Garcia-Sciveres M, Garfinkel AF, Gay C, Gerberich H, Gerchtein E, Gerdes DW, Giagu S, Giannetti P, Gibson A, Gibson K, Ginsburg C, Giolo K, Giordani M, Giurgiu G, Glagolev V, Glenzinski D, Gold M, Goldschmidt N, Goldstein D, Goldstein J, Gomez G, Gomez-Ceballos G, Goncharov M, Gorelov I, Goshaw AT, Gotra Y, Goulianos K, Gresele A, Grosso-Pilcher C, Guenther M, Guimaraes da Costa J, Haber C, Hahn K, Hahn SR, Halkiadakis E, Hall C, Handler R, Happacher F, Hara K, Hare M, Harr RF, Harris RM, Hartmann F, Hatakeyama K, Hauser J, Hays C, Hayward H, Heider E, Heinemann B, Heinrich J, Hennecke M, Herndon M, Hill C, Hirschbuehl D, Hocker A, Hoffman KD, Holloway A, Hou S, Houlden MA, Huang Y, Huffman BT, Hughes RE, Huston J, Ikado K, Incandela J, Introzzi G, Iori M, Ishizawa Y, Issever C, Ivanov A, Iwata Y, Iyutin B, James E, Jang D, Jarrell J, Jeans D, Jensen H, Jones M, Jun SY, Junk T, Kamon T, Kang J, Karagoz Unel M, Karchin PE, Kartal S, Kato Y, Kemp Y, Kephart R, Kerzel U, Khotilovich V, Kilminster B, Kim BJ, Kim DH, Kim HS, Kim JE, Kim MJ, Kim MS, Kim SB, Kim SH, Kim TH, Kim YK, King BT, Kirby M, Kirsch L, Klimenko S, Knuteson B, Ko BR, Kobayashi H, Koehn P, Kondo K, Konigsberg J, Kordas K, Korn A, Korytov A, Kotelnikov K, Kotwal AV, Kovalev A, Kraus J, Kravchenko I, Kreymer A, Kroll J, Kruse M, Krutelyov V, Kuhlmann SE, Kuznetsova N, Laasanen AT, Lai S, Lami S, Lammel S, Lancaster J, Lancaster M, Lander R, Lannon K, Lath A, Latino G, Lauhakangas R, Lazzizzera I, Le Y, Lecci C, LeCompte T, Lee J, Lee J, Lee SW, Leonardo N, Leone S, Lewis JD, Li K, Lin CS, Lindgren M, Liss TM, Litvintsev DO, Liu T, Liu Y, Lockyer NS, Loginov A, Loken J, Loreti M, Loverre P, Lucchesi D, Lukens P, Lyons L, Lys J, MacQueen D, Madrak R, Maeshima K, Maksimovic P, Malferrari L, Manca G, Marginean R, Martin A, Martin M, Martin V, Martinez M, Maruyama T, Matsunaga H, Mattson M, Mazzanti P, McFarland KS, McGivern D, McIntyre PM, McNamara P, McNulty R, Menzemer S, Menzione A, Merkel P, Mesropian C, Messina A, Meyer A, Miao T, Miladinovic N, Miller L, Miller R, Miller JS, Miquel R, Miscetti S, Mishina M, Mitselmakher G, Miyamoto A, Miyazaki Y, Moggi N, Moore R, Morello M, Moulik T, Mukherjee A, Mulhearn M, Muller T, Mumford R, Munar A, Murat P, Nachtman J, Nahn S, Nakamura I, Nakano I, Napier A, Napora R, Necula V, Niell F, Nielsen J, Nelson C, Nelson T, Neu C, Neubauer MS, Newman-Holmes C, Nicollerat AS, Nigmanov T, Nodulman L, Oesterberg K, Ogawa T, Oh S, Oh YD, Ohsugi T, Oishi R, Okusawa T, Oldeman R, Orava R, Orejudos W, Pagliarone C, Palmonari F, Paoletti R, Papadimitriou V, Pashapour S, Patrick J, Pauletta G, Paulini M, Pauly T, Paus C, Pellett D, Penzo A, Phillips TJ, Piacentino G, Piedra J, Pitts KT, Pompos A, Pondrom L, Pope G, Poukhov O, Prakoshyn F, Pratt T, Pronko A, Proudfoot J, Ptohos F, Punzi G, Rademacker J, Rakitine A, Rappoccio S, Ratnikov F, Ray H, Reichold A, Rekovic V, Renton P, Rescigno M, Rimondi F, Rinnert K, Ristori L, Robertson WJ, Robson A, Rodrigo T, Rolli S, Rosenson L, Roser R, Rossin R, Rott C, Russ J, Ruiz A, Ryan D, Saarikko H, Safonov A, St Denis R, Sakumoto WK, Saltzberg D, Sanchez C, Sansoni A, Santi L, Sarkar S, Sato K, Savard P, Savoy-Navarro A, Schemitz P, Schlabach P, Schmidt EE, Schmidt MP, Schmitt M, Scodellaro L, Scribano A, Scuri F, Sedov A, Seidel S, Seiya Y, Semeria F, Sexton-Kennedy L, Sfiligoi I, Shapiro MD, Shears T, Shepard PF, Shimojima M, Shochet M, Shon Y, Sidoti A, Siket M, Sill A, Sinervo P, Sisakyan A, Skiba A, Slaughter AJ, Sliwa K, Smith JR, Snider FD, Snihur R, Somalwar SV, Spalding J, Spezziga M, Spiegel L, Spinella F, Spiropulu M, Squillacioti P, Stadie H, Stelzer B, Stelzer-Chilton O, Strologas J, Stuart D, Sukhanov A, Sumorok K, Sun H, Suzuki T, Taffard A, Tafirout R, Takach SF, Takano H, Takashima R, Takeuchi Y, Takikawa K, Tamburello P, Tanaka M, Tanaka R, Tanimoto N, Tapprogge S, Tecchio M, Teng PK, Terashi K, Tesarek RJ, Tether S, Thom J, Thompson AS, Thomson E, Thurman-Keup R, Tipton P, Tiwari V, Tkaczyk S, Toback D, Tollefson K, Tonelli D, Tönnesmann M, Torre S, Torretta D, Trischuk W, Tseng J, Tsuchiya R, Tsuno S, Tsybychev D, Turini N, Turner M, Ukegawa F, Unverhau T, Uozumi S, Usynin D, Vacavant L, Vaiciulis T, Varganov A, Vataga E, Vejcik S, Velev G, Veramendi G, Vickey T, Vidal R, Vila I, Vilar R, Volobouev I, von der Mey M, Wagner RG, Wagner RL, Wagner W, Wallace N, Walter T, Wan Z, Wang MJ, Wang SM, Warburton A, Ward B, Waschke S, Waters D, Watts T, Weber M, Wester W, Whitehouse B, Wicklund AB, Wicklund E, Williams HH, Wilson P, Winer BL, Wittich P, Wolbers S, Wolter M, Worcester M, Worm S, Wright T, Wu X, Würthwein F, Wyatt A, Yagil A, Yamashita T, Yamamoto K, Yang UK, Yao W, Yeh GP, Yi K, Yoh J, Yoon P, Yorita K, Yoshida T, Yu I, Yu S, Yu Z, Yun JC, Zanello L, Zanetti A, Zaw I, Zetti F, Zhou J, Zsenei A, Zucchelli S. Observation of the narrow state X(3872)-->J/psipi+pi- in pp collisions at sqaure root of s=1.96 TeV. Phys Rev Lett 2004; 93:072001. [PMID: 15324226 DOI: 10.1103/physrevlett.93.072001] [Citation(s) in RCA: 43] [Impact Index Per Article: 2.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 12/04/2003] [Indexed: 05/24/2023]
Abstract
We report the observation of a narrow state decaying into J/psipi+pi- and produced in 220 pb(-1) of p p-bar collisions at =1.96 Tesqaure root of sV in the CDF II experiment. We observe 730+/-90 decays. The mass is measured to be 3871.3+/-0.7(stat)+/-0.4(syst) MeV/c2, with an observed width consistent with the detector resolution. This is in agreement with the recent observation by the Belle Collaboration of the X(3872) meson.
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Affiliation(s)
- D Acosta
- University of Florida, Gainesville, Florida 32611, USA
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Acosta D, Affolder T, Ahn MH, Akimoto T, Albrow MG, Ambrose D, Amidei D, Anastassov A, Anikeev K, Annovi A, Antos J, Aoki M, Apollinari G, Arguin JF, Arisawa T, Artikov A, Asakawa T, Ashmanskas W, Attal A, Azfar F, Azzi-Bacchetta P, Bacchetta N, Bachacou H, Badgett W, Bailey S, Barbaro-Galtieri A, Barker G, Barnes VE, Barnett BA, Baroiant S, Barone M, Bauer G, Bedeschi F, Behari S, Belforte S, Bell WH, Bellettini G, Bellinger J, Benjamin D, Beretvas A, Bhatti A, Binkley M, Bisello D, Bishai M, Blair RE, Blocker C, Bloom K, Blumenfeld B, Bocci A, Bodek A, Bolla G, Bolshov A, Booth PSL, Bortoletto D, Boudreau J, Bourov S, Bromberg C, Brozovic M, Brubaker E, Budagov J, Budd HS, Burkett K, Busetto G, Bussey P, Byrum KL, Cabrera S, Calafiura P, Campanelli M, Campbell M, Canepa A, Carlsmith D, Carron S, Carosi R, Casarsa M, Caskey W, Castro A, Catastini P, Cauz D, Cerri A, Cerri C, Cerrito L, Chapman J, Chen C, Chen YC, Chertok M, Chiarelli G, Chlachidze G, Chlebana F, Cho K, Chokheli D, Chu ML, Chung JY, Chung WH, Chung YS, Ciobanu CI, Ciocci MA, Clark AG, Coca MN, Connolly A, Convery ME, Conway J, Cordelli M, Cortiana G, Cranshaw J, Culbertson R, Currat C, Cyr D, Dagenhart D, DaRonco S, D'Auria S, De Barbaro P, De Cecco S, Dell'Agnello S, Dell'Orso M, Demers S, Demortier L, Deninno M, De Pedis D, Derwent PF, Dionisi C, Dittmann JR, Doksus P, Dominguez A, Donati S, D'Onofrio M, Dorigo T, Drollinger V, Ebina K, Eddy N, Ely R, Erbacher R, Erdmann M, Errede D, Errede S, Eusebi R, Fang HC, Farrington S, Fedorko I, Feild RG, Feindt M, Fernandez JP, Ferretti C, Field RD, Fiori I, Flanagan G, Flaugher B, Flores-Castillo LR, Foland A, Forrester S, Foster GW, Franklin M, Frisch H, Fujii Y, Furic I, Gallas A, Gallinaro M, Galyardt J, Garcia-Sciveres M, Garfinkel AF, Gay C, Gerberich H, Gerchtein E, Gerdes DW, Giagu S, Giannetti P, Gibson A, Gibson K, Ginsburg C, Giolo K, Giordani M, Giurgiu G, Glagolev V, Glenzinski D, Gold M, Goldschmidt N, Goldstein D, Goldstein J, Gomez G, Gomez-Ceballos G, Goncharov M, Gorelov I, Goshaw AT, Gotra Y, Goulianos K, Gresele A, Grim G, Grosso-Pilcher C, Guenther M, Guimaraes Da Costa J, Haber C, Hahn K, Hahn SR, Halkiadakis E, Hall C, Handler R, Happacher F, Hara K, Hare M, Harr RF, Harris RM, Hartmann F, Hatakeyama K, Hauser J, Hays C, Heider E, Heinemann B, Heinrich J, Hennecke M, Herndon M, Hill C, Hirschbuehl D, Hocker A, Hoffman KD, Holloway A, Hou S, Houlden MA, Huffman BT, Hughes RE, Huston J, Ikado K, Incandela J, Introzzi G, Iori M, Ishizawa Y, Issever C, Ivanov A, Iwata Y, Iyutin B, James E, Jang D, Jarrell J, Jeans D, Jensen H, Jones M, Jun SY, Junk T, Kamon T, Kang J, Karagoz Unel M, Karchin PE, Kartal S, Kato Y, Kemp Y, Kephart R, Kerzel U, Khazins D, Khotilovich V, Kilminster B, Kim BJ, Kim DH, Kim HS, Kim JE, Kim MJ, Kim MS, Kim SB, Kim SH, Kim TH, Kim YK, King BT, Kirby M, Kirk M, Kirsch L, Klimenko S, Knuteson B, Kobayashi H, Koehn P, Kondo K, Konigsberg J, Kordas K, Korn A, Korytov A, Kotelnikov K, Kotwal AV, Kovalev A, Kraus J, Kravchenko I, Kreymer A, Kroll J, Kruse M, Krutelyov V, Kuhlmann SE, Kuznetsova N, Laasanen AT, Lai S, Lami S, Lammel S, Lancaster J, Lancaster M, Lander R, Lannon K, Lath A, Latino G, Lauhakangas R, Lazzizzera I, Le Y, Lecci C, LeCompte T, Lee J, Lee J, Lee SW, Leonardo N, Leone S, Lewis JD, Li K, Lin CS, Lindgren M, Liss TM, Litvintsev DO, Liu T, Liu Y, Lockyer NS, Loginov A, Loken J, Loreti M, Loverre P, Lucchesi D, Lukens P, Lyons L, Lys J, MacQueen D, Madrak R, Maeshima K, Maksimovic P, Malferrari L, Manca G, Marginean R, Martin A, Martin M, Martin V, Martinez M, Maruyama T, Matsunaga H, Mattson M, Mazzanti P, McFarland KS, McGivern D, McIntyre PM, McNamara P, McNulty R, Menzemer S, Menzione A, Merkel P, Mesropian C, Messina A, Meyer A, Miao T, Miller L, Miller R, Miller JS, Miquel R, Miscetti S, Mishina M, Mitselmakher G, Miyamoto A, Miyazaki Y, Moggi N, Moore R, Morello M, Moulik T, Mukherjee A, Mulhearn M, Muller T, Mumford R, Munar A, Murat P, Murgia S, Nachtman J, Nahn S, Nakamura I, Nakano I, Napier A, Napora R, Necula V, Niell F, Nielsen J, Nelson C, Nelson T, Neu C, Neubauer MS, Newman-Holmes C, Nicollerat AS, Nigmanov T, Niu H, Nodulman L, Oesterberg K, Ogawa T, Oh S, Oh YD, Ohsugi T, Oishi R, Okusawa T, Oldeman R, Orava R, Orejudos W, Pagliarone C, Palmonari F, Paoletti R, Papadimitriou V, Partos D, Pashapour S, Patrick J, Pauletta G, Paulini M, Pauly T, Paus C, Pellett D, Penzo A, Phillips TJ, Piacentino G, Piedra J, Pitts KT, Pompos A, Pondrom L, Pope G, Poukhov O, Prakoshyn F, Pratt T, Pronko A, Proudfoot J, Ptohos F, Punzi G, Rademacker J, Rakitine A, Rappoccio S, Ratnikov F, Ray H, Reichold A, Rekovic V, Renton P, Rescigno M, Rimondi F, Rinnert K, Ristori L, Riveline M, Robertson WJ, Robson A, Rodrigo T, Rolli S, Rosenson L, Roser R, Rossin R, Rott C, Russ J, Ruiz A, Ryan D, Saarikko H, Safonov A, St Denis R, Sakumoto WK, Saltzberg D, Sanchez C, Sansoni A, Santi L, Sarkar S, Sato K, Savard P, Savoy-Navarro A, Schemitz P, Schlabach P, Schmidt EE, Schmidt MP, Schmitt M, Schofield G, Scodellaro L, Scribano A, Scuri F, Sedov A, Seidel S, Seiya Y, Semeria F, Sexton-Kennedy L, Sfiligoi I, Shapiro MD, Shears T, Shepard PF, Shimojima M, Shochet M, Shon Y, Sidoti A, Siket M, Sill A, Sinervo P, Sisakyan A, Skiba A, Slaughter AJ, Sliwa K, Smith JR, Snider FD, Snihur R, Somalwar SV, Spalding J, Spezziga M, Spiegel L, Spinella F, Spiropulu M, Stadie H, Stelzer B, Stelzer-Chilton O, Strologas J, Stuart D, Sukhanov A, Sumorok K, Sun H, Suzuki T, Taffard A, Takach SF, Takano H, Takashima R, Takeuchi Y, Takikawa K, Tamburello P, Tanaka M, Tanaka R, Tannenbaum B, Tanimoto N, Tapprogge S, Tecchio M, Teng PK, Terashi K, Tesarek RJ, Tether S, Thom J, Thompson AS, Thomson E, Thurman-Keup R, Tipton P, Tiwari V, Tkaczyk S, Toback D, Tollefson K, Tonelli D, Tönnesmann M, Torre S, Torretta D, Trischuk W, Tseng J, Tsuchiya R, Tsuno S, Tsybychev D, Turini N, Turner M, Ukegawa F, Unverhau T, Uozumi S, Usynin D, Vacavant L, Vaiciulis T, Varganov A, Vataga E, Vejcik S, Velev G, Veramendi G, Vickey T, Vidal R, Vila I, Vilar R, Volobouev I, Von Der Mey M, Wagner RG, Wagner RL, Wagner W, Wallace N, Walter T, Wan Z, Wang MJ, Wang SM, Ward B, Waschke S, Waters D, Watts T, Weber M, Wester W, Whitehouse B, Wicklund AB, Wicklund E, Wilkes T, Williams HH, Wilson P, Winer BL, Wittich P, Wolbers S, Wolter M, Worcester M, Worm S, Wright T, Wu X, Würthwein F, Wyatt A, Yagil A, Yamashita T, Yamamoto K, Yang UK, Yao W, Yeh GP, Yi K, Yoh J, Yoon P, Yorita K, Yoshida T, Yu I, Yu S, Yu Z, Yun JC, Zanello L, Zanetti A, Zaw I, Zetti F, Zhou J, Zsenei A, Zucchelli S. Measurement of prompt charm meson production cross sections in pp collisions at square root s = 1.96 TeV. Phys Rev Lett 2003; 91:241804. [PMID: 14683110 DOI: 10.1103/physrevlett.91.241804] [Citation(s) in RCA: 16] [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: 07/25/2003] [Indexed: 05/24/2023]
Abstract
We report on measurements of differential cross sections dsigma/dp(T) for prompt charm meson production in ppmacr; collisions at sqrt[s]=1.96 TeV using 5.8+/-0.3 pb(-1) of data from the CDF II detector at the Fermilab Tevatron. The data are collected with a new trigger that is sensitive to the long lifetime of hadrons containing heavy flavor. The charm meson cross sections are measured in the central rapidity region |y|</=1 in four fully reconstructed decay modes: D0-->K-pi(+), D(*+)-->D0pi(+), D+-->K-pi(+)pi(+), D(+)(s)-->phipi(+), and their charge conjugates. The measured cross sections are compared to theoretical calculations.
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Affiliation(s)
- D Acosta
- University of Florida, Gainesville, Florida 32611, USA
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Geer S, Marriner J, Martens M, Ray RE, Streets J, Wester W, Hu M, Snow GR, Armstrong T, Buchanan C, Corbin B, Lindgren M, Muller T, Gustafson R. New limit on CPT violation. Phys Rev Lett 2000; 84:590-593. [PMID: 11017323 DOI: 10.1103/physrevlett.84.590] [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: 10/07/1999] [Indexed: 05/23/2023]
Abstract
A search for antiproton decay has been made at the Fermilab Antiproton Accumulator. Limits are placed on fifteen antiproton decay modes. The results are used to place limits on the characteristic mass scale m(X) that could be associated with CPT violation accompanied by baryon number violation.
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Affiliation(s)
- S Geer
- Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
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Miralles M, Wester W, Sicard GA, Thompson R, Reilly JM. Indomethacin inhibits expansion of experimental aortic aneurysms via inhibition of the cox2 isoform of cyclooxygenase. J Vasc Surg 1999; 29:884-92; discussion 892-3. [PMID: 10231640 DOI: 10.1016/s0741-5214(99)70216-8] [Citation(s) in RCA: 68] [Impact Index Per Article: 2.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/26/2022]
Abstract
PURPOSE Cyclooxygenase, either the cox1 or cox2 isoform, controls synthesis of prostaglandin E2 (PGE2), which regulates expression of matrix metalloprotease-9 (MMP-9). PGE2 and MMP-9 are elevated in aortic aneurysms. The mechanisms and time course of the inhibition of aneurysm expansion with a nonspecific cyclooxygenase inhibitor, indomethacin, were determined in an animal model. METHODS Rats underwent aortic perfusion with saline (n = 40) as controls or with elastase. Elastase-treated animals received no treatment (n = 82) or received indomethacin (n = 73). Aortic diameters were determined at the time of aortic perfusion and when the rats were killed. The aortas were harvested and used for whole organ culture, substrate gel zymography, or histologic analysis. RESULTS The control group demonstrated little change in aortic diameter. All the elastase-only animals developed aneurysms (maximal aortic diameter, 5.27 +/- 2.37 mm on day 14). Indomethacin markedly decreased the rate of aortic expansion (maximum aortic diameter, 3.45 +/- 1.11 mm; P <.001 vs the elastase-only group). The enzyme-linked immunosorbent assay of aortic explant culture media showed that PGE2 synthesis paralleled aortic expansion, and indomethacin decreased PGE2 synthesis. Histologically, the aortic elastin architecture was destroyed in the elastase group, but was preserved with indomethacin treatment. In situ, hybridization for cox1 and cox2 showed that cox2, but not cox1, was expressed and was co-localized by immunohistochemistry to macrophages associated with the aortic wall. Decreased levels of MMP-9 activity with indomethacin were shown by means of substrate zymography. MMP-9 was also localized to macrophages. CONCLUSION Indomethacin attenuates aneurysm growth, and its effects are mediated via inhibition of the cox2 isoform of cyclooxygenase, which decreases PGE2 and MMP-9 synthesis.
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Affiliation(s)
- M Miralles
- Department of Surgery, Washington University School of Medicine and John Cochran Veterans Administration Medical Center, St Louis, MO, USA
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Hu M, Snow GR, Geer S, Marriner J, Martens M, Ray RE, Streets J, Wester W, Armstrong T, Buchanan C, Corbin B, Lindgren M, Muller T, Gustafson R. Search for muonic decays of the antiproton at the Fermilab Antiproton Accumulator. Int J Clin Exp Med 1998. [DOI: 10.1103/physrevd.58.111101] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
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Abstract
PURPOSE The purpose of this study was to evaluate the expression of prostaglandin E2 (PGE2) and the two cyclooxygenase isoforms (cox1 and cox2) in human abdominal aortic aneurysm (AAA) tissue. METHODS Ten specimens each of normal aortas and aneurysmal aortas were collected and used for histologic analysis and whole organ culture. An enzyme-linked immunosorbent assay for PGE2 was performed on the media from the aortic explant whole organ culture. An immunohistochemical analysis for PGE2 was performed, as was in situ hybridization for cox1 and cox2 on tissue sections. RESULTS PGE2 production of AAA specimens was found to be 67,287 +/- 27,303 pg/ml as compared with 1698 +/- 858 pg/ml for normal aortic specimens (p < 0.001). PGE2 was localized by immunohistochemical analysis to the inflammatory infiltrate in AAAs. Minimal expression was noted in normal aortas. Using in situ hybridization, little expression of cox1 was noted in either the normal or the AAA specimens. Cox2 was expressed by macrophage-like cells within the inflammatory infiltrate of the AAA specimens but was not significantly expressed in the normal aorta. CONCLUSION The expression of PGE2 is associated with the pathogenesis of human AAAs. Its expression is localized to macrophage-like cells within the inflammatory infiltrate and is controlled by the cox2 isoform of cyclooxygenase. Cox2 is, therefore, a potential target for pharmacotherapy of AAAs.
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Affiliation(s)
- D R Holmes
- Department of Surgery, Washington University School of Medicine, St. Louis, MO 63110, USA
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Abstract
Perfusion of the rat abdominal aorta with elastase induces abdominal aortic aneurysms (AAA), in which the development of aortic dilatation correlates with the influx of inflammatory cells, increased production of matrix metalloproteinases (MMPs), and destruction of medial elastin. We tested the hypothesis that indomethacin, an inhibitor of macrophage MMP expression, might attenuate aneurysmal degeneration in this model. Fourteen adult male Wistar rats underwent 2-hr aortic perfusion with elastase. Six animals received injections of saline and eight animals received 4 mg/kg/day indomethacin for 7 days. Pre-perfusion, post-perfusion, and final aortic diameters (AD) were determined, and histology and substrate gel zymography were performed. Five out of six control animals developed AAA, while no aneurysms were observed in the indomethacin-treated group (P < 0.01). Whereas AD increased 126 +/- 16% in control animals, the mean increase in the indomethacin-treated group was only 56 +/- 6% (P < 0.001). Although animals in both groups demonstrated an inflammatory response dominated by macrophages, the marked destruction of medial elastin in the control group was not present in the treatment group. In addition, substrate zymography demonstrated decreased levels of MMP-9 in animals treated with indomethacin. Indomethacin inhibits aneurysm growth in this model, and the data suggest that it does so by decreasing macrophage expression of at least one elastolytic metalloproteinase, MMP-9.
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Affiliation(s)
- D R Holmes
- Department of Surgery, Washington University School of Medicine, St. Louis, Missouri 63110, USA
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Whittle AP, Wester W, Russell TA. Fatigue failure in small diameter tibial nails. Clin Orthop Relat Res 1995:119-28. [PMID: 7634660] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 01/26/2023]
Abstract
The prevalence of implant failure in small diameter tibial nails has not been well characterized. In a series of 130 tibial fractures stabilized with 8-mm and 9-mm nails, implant failure occurred in 18 fractures (13.8%): 4 nails (3%) broke and 16 (12.3%) screws failed. All nail failures occurred in open, unstable fractures with delayed union, and all of the nails that broke were dynamically locked during the failure. Of the 130 fractures, 128 (98.5%) eventually united. Delayed union, degree of comminution, metaphyseal location, and dynamic locking of unstable fractures contribute to hardware failure. Based on these findings, dynamization could be used to treat delayed union only in axially stable diaphyseal fractures. Exchange nailing is recommended to treat delayed union in comminuted or metaphyseal fractures to prevent hardware failure. Bone grafting should be performed at 6 to 12 weeks for fractures with > 50% bone loss.
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Affiliation(s)
- A P Whittle
- University of Tennessee-Campbell Clinic, Department of Orthopaedic Surgery, Memphis, USA
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Wester W, Canale ST, Dutkowsky JP, Warner WC, Beaty JH. Prediction of angular deformity and leg-length discrepancy after anterior cruciate ligament reconstruction in skeletally immature patients. J Pediatr Orthop 1994; 14:516-21. [PMID: 8077439 DOI: 10.1097/01241398-199407000-00019] [Citation(s) in RCA: 52] [Impact Index Per Article: 1.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 02/07/2023]
Abstract
Injuries to the anterior cruciate ligament (ACL) in young children and adolescents are becoming more common as more youngsters participate in organized sports. The dilemma for the orthopaedic surgeon is that untreated ACL ruptures may result in meniscal damage and joint degeneration, whereas surgical treatment may result in physeal arrest, with shortening and angular deformity. To help determine the appropriate timing for ACL repair in skeletally immature patients, graphs have been developed to predict the amount of shortening and angular deformity to expect after repair.
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Affiliation(s)
- W Wester
- Department of Orthopaedic Surgery, University of Tennessee-Campbell Clinic, Memphis
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Abe F, Amidei D, Apollinari G, Atac M, Auchincloss P, Baden A, Bailey M, Bamberger A, Barnett B, Barbaro-Galtieri A, Barnes V, Baumann T, Bedeschi F, Behrends S, Belforte S, Bellettini G, Bellinger J, Bensinger J, Beretvas A, Berge J, Bertolucci S, Bhadra S, Binkley M, Blair R, Blocker C, Bolognesi V, Booth A, Boswell C, Brandenburg G, Brown D, Buckley-Geer E, Budd H, Byon A, Byrum K, Campagnari C, Campbell M, Carey R, Carithers W, Carlsmith D, Carroll J, Cashmore R, Cervelli F, Chadwick K, Chiarelli G, Chinowsky W, Cihangir S, Clark A, Connor D, Contreras M, Cooper J, Cordelli M, Crane D, Curatolo M, Day C, Dell'Agnello S, Dell'Orso M, Demortier L, Derwent P, Devlin T, DiBitonto D, Drucker R, Elias J, Ely R, Eno S, Errede S, Esposito B, Flaugher B, Foster G, Franklin M, Freeman J, Frisch H, Fuess T, Fukui Y, Funayama Y, Garfinkel A, Gauthier A, Geer S, Giannetti P, Giokaris N, Giromini P, Gladney L, Gold M, Goulianos K, Grassmann H, Grosso-Pilcher C, Haber C, Hahn S, Handler R, Hara K, Harris R, Hauser J, Hawk C, Hessing T, Hollebeek R, Holloway L, Hu P, Hubbard B, Huffman B, Hughes R, Hurst P, Huth J, Incagli M, Ino T, Iso H, Jensen H, Jessop C, Johnson R, Joshi U, Kadel R, Kamon T, Kanda S, Kardelis D, Karliner I, Kearns E, Keeble L, Kephart R, Kesten P, Keup R, Keutelian H, Kim D, Kim S, Kirsch L, Kondo K, Konigsberg J, Kovacs E, Kuhlmann S, Kuns E, Laasanen A, Lamoureux J, Leone S, Li W, Liss T, Lockyer N, Luchini C, Maas P, Maeshima K, Mangano M, Marriner J, Markeloff R, Markosky L, Mattingly R, McIntyre P, Menzione A, Meyer T, Mikamo S, Miller M, Mimashi T, Miscetti S, Mishina M, Miyashita S, Morita Y, Moulding S, Mueller J, Mukherjee A, Nakae L, Nakano I, Nelson C, Newman-Holmes C, Ng J, Ninomiya M, Nodulman L, Ogawa S, Paoletti R, Para A, Pare E, Patrick J, Phillips T, Plunkett R, Pondrom L, Proudfoot J, Punzi G, Quarrie D, Ragan K, Redlinger G, Rhoades J, Roach M, Rimondi F, Ristori L, Rohaly T, Roodman A, Sakumoto W, Sansoni A, Sard R, Savoy-Navarro A, Scarpine V, Schlabach P, Schmidt E, Schub M, Schwitters R, Scribano A, Segler S, Seiya Y, Sekiguchi M, Shapiro M, Shaw N, Sheaff M, Shochet M, Siegrist J, Sinervo P, Skarha J, Sliwa K, Smith D, Snider F, Song L, St. Denis R, Stefanini A, Sullivan G, Swartz R, Takano M, Tartarelli F, Takikawa K, Tarem S, Theriot D, Timko M, Tipton P, Tkaczyk S, Tollestrup A, Tonnison J, Trischuk W, Tsay Y, Ukegawa F, Underwood D, Vejcik S, Vidal R, Wagner R, Wagner R, Wainer N, Walsh J, Watts T, Webb R, Wendt C, Wester W, Westhusing T, White S, Wicklund A, Williams H, Winer B, Yagil A, Yamashita A, Yasuoka K, Yeh G, Yoh J, Yokoyama M, Yun J, Zetti F. Measurement of the e+e- Invariant-Mass Distribution in p-barp Collisions at s=1.8 TeV. Phys Rev Lett 1991; 67:2418-2422. [PMID: 10044421 DOI: 10.1103/physrevlett.67.2418] [Citation(s) in RCA: 7] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/23/2023]
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Brau JE, Franek B, Wester W, Abe K, Bacon TC, Ballam J, Bingham HH, Braune K, Brick D, Bugg WM, Butler JM, Cameron W, Carroll JT, Cautis CV, Cohn HO, Colley DC, Condo GT, Dado S, Diamond R, Dingus P, Erickson R, Fieguth T, Field RC, Fortney L, Fujiwara N, Gearhart R, Glanzman T, Godfrey IM, Goldberg JJ, Goshaw AT, Hall G, Hancock ER, Handler T, Hargis HJ, Hart EL, Harwin MJ, Hasegawa K, Hulsizer RI, Jobes M, Kafka T, Kalmus GE, Kelsey DP, Kent J, Kitagaki T, Levy A, Mann WA, Merenyi R, Milburn R, Milstene C, McCrory E, Moffeit KC, Napier A, Noguchi S, Ochiai F, O'Dell VR, O'Neale S, Palounek AP, Pless IA, Rankin P, Sagawa H, Sato T, Schneps J, Sewell SJ. Production and decay properties of the omega pi 0 state at 1250 MeV/c2 produced by 20-GeV polarized photons on hydrogen. Phys Rev D Part Fields 1988; 37:2379-2390. [PMID: 9958954 DOI: 10.1103/physrevd.37.2379] [Citation(s) in RCA: 6] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 04/12/2023]
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Cohen BG, Colligan MJ, Wester W, Smith MJ. An investigation of job satisfaction factors in an incident of mass psychogenic illness at the workplace. Occup Health Nurs 1978; 26:10-6. [PMID: 564008 DOI: 10.1177/216507997802600102] [Citation(s) in RCA: 6] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 12/23/2022]
Abstract
An investigation was undertaken of an apparent outbreak of contagious psychogenic illness at an electronics plant in which approximately 50 females reported a variety of subjective nonspecific symptoms. The workers believed that the physical symptomatology was triggered by an unidentified odor in the plant which was not verified by environmental sampling for chemicals or by medical evaluations of affected workers. A random sample of non-affected and affected workers was surveyed by means of psychological health status inventories and epidemiological indices to determine the role that life-history, personality characteristics and job dissatisfaction had on susceptibility to illness. Results indicated that those workers reporting the highest level of perceived stress due to job dissatisfaction, family problems, and personal conflict were most likely to experience somatic symptoms. In the present study sources of dissatisfaction identified as potential precipitating factors of the illness outbreak were: 1) working conditions, 2) supervisory style, and 3) personal lifestyle.
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