Nature Communications (Oct 2022)
Search for Dark Matter Axions with CAST-CAPP
- C. M. Adair,
- K. Altenmüller,
- V. Anastassopoulos,
- S. Arguedas Cuendis,
- J. Baier,
- K. Barth,
- A. Belov,
- D. Bozicevic,
- H. Bräuninger,
- G. Cantatore,
- F. Caspers,
- J. F. Castel,
- S. A. Çetin,
- W. Chung,
- H. Choi,
- J. Choi,
- T. Dafni,
- M. Davenport,
- A. Dermenev,
- K. Desch,
- B. Döbrich,
- H. Fischer,
- W. Funk,
- J. Galan,
- A. Gardikiotis,
- S. Gninenko,
- J. Golm,
- M. D. Hasinoff,
- D. H. H. Hoffmann,
- D. Díez Ibáñez,
- I. G. Irastorza,
- K. Jakovčić,
- J. Kaminski,
- M. Karuza,
- C. Krieger,
- Ç. Kutlu,
- B. Lakić,
- J. M. Laurent,
- J. Lee,
- S. Lee,
- G. Luzón,
- C. Malbrunot,
- C. Margalejo,
- M. Maroudas,
- L. Miceli,
- H. Mirallas,
- L. Obis,
- A. Özbey,
- K. Özbozduman,
- M. J. Pivovaroff,
- M. Rosu,
- J. Ruz,
- E. Ruiz-Chóliz,
- S. Schmidt,
- M. Schumann,
- Y. K. Semertzidis,
- S. K. Solanki,
- L. Stewart,
- I. Tsagris,
- T. Vafeiadis,
- J. K. Vogel,
- M. Vretenar,
- S. Youn,
- K. Zioutas
Affiliations
- C. M. Adair
- Department of Physics and Astronomy, University of British Columbia
- K. Altenmüller
- Centro de Astropartículas y Física de Altas Energías (CAPA), Universidad de Zaragoza
- V. Anastassopoulos
- Physics Department, University of Patras
- S. Arguedas Cuendis
- European Organization for Nuclear Research (CERN)
- J. Baier
- Physikalisches Institut, Albert-Ludwigs-Universität Freiburg
- K. Barth
- European Organization for Nuclear Research (CERN)
- A. Belov
- Institute for Nuclear Research (INR), Russian Academy of Sciences
- D. Bozicevic
- University of Rijeka, Faculty of Engineering
- H. Bräuninger
- Max-Planck-Institut für Extraterrestrische Physik
- G. Cantatore
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Trieste
- F. Caspers
- European Organization for Nuclear Research (CERN)
- J. F. Castel
- Centro de Astropartículas y Física de Altas Energías (CAPA), Universidad de Zaragoza
- S. A. Çetin
- Istinye University, Institute of Sciences
- W. Chung
- Center for Axion and Precision Physics Research, Institute for Basic Science (IBS)
- H. Choi
- Department of Physics, Korea Advanced Institute of Science and Technology (KAIST)
- J. Choi
- Center for Axion and Precision Physics Research, Institute for Basic Science (IBS)
- T. Dafni
- Centro de Astropartículas y Física de Altas Energías (CAPA), Universidad de Zaragoza
- M. Davenport
- European Organization for Nuclear Research (CERN)
- A. Dermenev
- Institute for Nuclear Research (INR), Russian Academy of Sciences
- K. Desch
- Physikalisches Institut, University of Bonn
- B. Döbrich
- European Organization for Nuclear Research (CERN)
- H. Fischer
- Physikalisches Institut, Albert-Ludwigs-Universität Freiburg
- W. Funk
- European Organization for Nuclear Research (CERN)
- J. Galan
- Centro de Astropartículas y Física de Altas Energías (CAPA), Universidad de Zaragoza
- A. Gardikiotis
- Physics Department, University of Patras
- S. Gninenko
- Institute for Nuclear Research (INR), Russian Academy of Sciences
- J. Golm
- European Organization for Nuclear Research (CERN)
- M. D. Hasinoff
- Department of Physics and Astronomy, University of British Columbia
- D. H. H. Hoffmann
- Xi’An Jiaotong University, School of Science
- D. Díez Ibáñez
- Centro de Astropartículas y Física de Altas Energías (CAPA), Universidad de Zaragoza
- I. G. Irastorza
- Centro de Astropartículas y Física de Altas Energías (CAPA), Universidad de Zaragoza
- K. Jakovčić
- Rudjer Bošković Institute
- J. Kaminski
- Physikalisches Institut, University of Bonn
- M. Karuza
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Trieste
- C. Krieger
- Physikalisches Institut, University of Bonn
- Ç. Kutlu
- Center for Axion and Precision Physics Research, Institute for Basic Science (IBS)
- B. Lakić
- Rudjer Bošković Institute
- J. M. Laurent
- European Organization for Nuclear Research (CERN)
- J. Lee
- Department of Physics, Korea Advanced Institute of Science and Technology (KAIST)
- S. Lee
- Center for Axion and Precision Physics Research, Institute for Basic Science (IBS)
- G. Luzón
- Centro de Astropartículas y Física de Altas Energías (CAPA), Universidad de Zaragoza
- C. Malbrunot
- European Organization for Nuclear Research (CERN)
- C. Margalejo
- Centro de Astropartículas y Física de Altas Energías (CAPA), Universidad de Zaragoza
- M. Maroudas
- Physics Department, University of Patras
- L. Miceli
- Center for Axion and Precision Physics Research, Institute for Basic Science (IBS)
- H. Mirallas
- Centro de Astropartículas y Física de Altas Energías (CAPA), Universidad de Zaragoza
- L. Obis
- Centro de Astropartículas y Física de Altas Energías (CAPA), Universidad de Zaragoza
- A. Özbey
- Istinye University, Institute of Sciences
- K. Özbozduman
- Istinye University, Institute of Sciences
- M. J. Pivovaroff
- Lawrence Livermore National Laboratory
- M. Rosu
- Extreme Light Infrastructure - Nuclear Physics (ELI-NP)
- J. Ruz
- Lawrence Livermore National Laboratory
- E. Ruiz-Chóliz
- Institut für Physik, Johannes Gutenberg Universität Mainz
- S. Schmidt
- Physikalisches Institut, University of Bonn
- M. Schumann
- Physikalisches Institut, Albert-Ludwigs-Universität Freiburg
- Y. K. Semertzidis
- Center for Axion and Precision Physics Research, Institute for Basic Science (IBS)
- S. K. Solanki
- Max-Planck-Institut für Sonnensystemforschung
- L. Stewart
- European Organization for Nuclear Research (CERN)
- I. Tsagris
- Physics Department, University of Patras
- T. Vafeiadis
- European Organization for Nuclear Research (CERN)
- J. K. Vogel
- Lawrence Livermore National Laboratory
- M. Vretenar
- University of Rijeka, Faculty of Physics
- S. Youn
- Center for Axion and Precision Physics Research, Institute for Basic Science (IBS)
- K. Zioutas
- Physics Department, University of Patras
- DOI
- https://doi.org/10.1038/s41467-022-33913-6
- Journal volume & issue
-
Vol. 13,
no. 1
pp. 1 – 9
Abstract
Haloscopes aim at detecting axions by converting them into photons using high-quality resonant cavities, where the cavity resonance should be tuned with the unknown axion mass. Here, the authors improve exclusion limits using four phase-matched resonant cavities and a fast frequency scanning technique.
