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Search for Dark Matter Axions with CAST-CAPP.
Adair, C M; Altenmüller, K; Anastassopoulos, V; Arguedas Cuendis, S; Baier, J; Barth, K; Belov, A; Bozicevic, D; Bräuninger, H; Cantatore, G; Caspers, F; Castel, J F; Çetin, S A; Chung, W; Choi, H; Choi, J; Dafni, T; Davenport, M; Dermenev, A; Desch, K; Döbrich, B; Fischer, H; Funk, W; Galan, J; Gardikiotis, A; Gninenko, S; Golm, J; Hasinoff, M D; Hoffmann, D H H; Díez Ibáñez, D; Irastorza, I G; Jakovcic, K; Kaminski, J; Karuza, M; Krieger, C; Kutlu, Ç; Lakic, B; Laurent, J M; Lee, J; Lee, S; Luzón, G; Malbrunot, C; Margalejo, C; Maroudas, M; Miceli, L; Mirallas, H; Obis, L; Özbey, A; Özbozduman, K; Pivovaroff, M J.
Afiliação
  • Adair CM; Department of Physics and Astronomy, University of British Columbia, Vancouver, V6T 1Z1, BC, Canada.
  • Altenmüller K; Centro de Astropartículas y Física de Altas Energías (CAPA), Universidad de Zaragoza, Zaragoza, 50009, Spain.
  • Anastassopoulos V; Physics Department, University of Patras, Patras, 26504, Greece.
  • Arguedas Cuendis S; European Organization for Nuclear Research (CERN), Genève, CH-1211, Switzerland.
  • Baier J; Physikalisches Institut, Albert-Ludwigs-Universität Freiburg, Freiburg, 79104, Germany.
  • Barth K; European Organization for Nuclear Research (CERN), Genève, CH-1211, Switzerland.
  • Belov A; Institute for Nuclear Research (INR), Russian Academy of Sciences, Moscow, 117312, Russia.
  • Bozicevic D; University of Rijeka, Faculty of Engineering, Rijeka, 51000, Croatia.
  • Bräuninger H; Max-Planck-Institut für Extraterrestrische Physik, Garching, D-85741, Germany.
  • Cantatore G; Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Trieste, Trieste, 34127, Italy.
  • Caspers F; Università di Trieste, Trieste, 34127, Italy.
  • Castel JF; European Organization for Nuclear Research (CERN), Genève, CH-1211, Switzerland.
  • Çetin SA; European Scientific Institute (ESI), Archamps, 74160, France.
  • Chung W; Centro de Astropartículas y Física de Altas Energías (CAPA), Universidad de Zaragoza, Zaragoza, 50009, Spain.
  • Choi H; Istinye University, Institute of Sciences, Sariyer, Istanbul, 34396, Turkey.
  • Choi J; Center for Axion and Precision Physics Research, Institute for Basic Science (IBS), Daejeon, 34141, Republic of Korea.
  • Dafni T; Department of Physics, Korea Advanced Institute of Science and Technology (KAIST), Daejeon, 34141, Republic of Korea.
  • Davenport M; Center for Axion and Precision Physics Research, Institute for Basic Science (IBS), Daejeon, 34141, Republic of Korea.
  • Dermenev A; Centro de Astropartículas y Física de Altas Energías (CAPA), Universidad de Zaragoza, Zaragoza, 50009, Spain.
  • Desch K; European Organization for Nuclear Research (CERN), Genève, CH-1211, Switzerland.
  • Döbrich B; Institute for Nuclear Research (INR), Russian Academy of Sciences, Moscow, 117312, Russia.
  • Fischer H; Physikalisches Institut, University of Bonn, Bonn, 53115, Germany.
  • Funk W; European Organization for Nuclear Research (CERN), Genève, CH-1211, Switzerland.
  • Galan J; Physikalisches Institut, Albert-Ludwigs-Universität Freiburg, Freiburg, 79104, Germany.
  • Gardikiotis A; European Organization for Nuclear Research (CERN), Genève, CH-1211, Switzerland.
  • Gninenko S; Centro de Astropartículas y Física de Altas Energías (CAPA), Universidad de Zaragoza, Zaragoza, 50009, Spain.
  • Golm J; Physics Department, University of Patras, Patras, 26504, Greece.
  • Hasinoff MD; Universität Hamburg, Hamburg, 22762, Germany.
  • Hoffmann DHH; Institute for Nuclear Research (INR), Russian Academy of Sciences, Moscow, 117312, Russia.
  • Díez Ibáñez D; European Organization for Nuclear Research (CERN), Genève, CH-1211, Switzerland.
  • Irastorza IG; Institute for Optics and Quantum Electronics, Friedrich Schiller University Jena, Jena, 07743, Germany.
  • Jakovcic K; Department of Physics and Astronomy, University of British Columbia, Vancouver, V6T 1Z1, BC, Canada.
  • Kaminski J; Xi'An Jiaotong University, School of Science, Xi'An, 710049, China.
  • Karuza M; Centro de Astropartículas y Física de Altas Energías (CAPA), Universidad de Zaragoza, Zaragoza, 50009, Spain.
  • Krieger C; Centro de Astropartículas y Física de Altas Energías (CAPA), Universidad de Zaragoza, Zaragoza, 50009, Spain.
  • Kutlu Ç; Rudjer Boskovic Institute, Zagreb, 10000, Croatia.
  • Lakic B; Physikalisches Institut, University of Bonn, Bonn, 53115, Germany.
  • Laurent JM; Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Trieste, Trieste, 34127, Italy.
  • Lee J; University of Rijeka, Faculty of Physics, Rijeka, 51000, Croatia.
  • Lee S; University of Rijeka, Photonics and Quantum Optics Unit, Center of Excellence for Advanced Materials and Sensing Devices, and Centre for Micro and Nano Sciences and Technologies, Rijeka, 51000, Croatia.
  • Luzón G; Physikalisches Institut, University of Bonn, Bonn, 53115, Germany.
  • Malbrunot C; Institute of Experimental Physics, University of Hamburg, Hamburg, 22761, Germany.
  • Margalejo C; Center for Axion and Precision Physics Research, Institute for Basic Science (IBS), Daejeon, 34141, Republic of Korea.
  • Maroudas M; Department of Physics, Korea Advanced Institute of Science and Technology (KAIST), Daejeon, 34141, Republic of Korea.
  • Miceli L; Rudjer Boskovic Institute, Zagreb, 10000, Croatia.
  • Mirallas H; European Organization for Nuclear Research (CERN), Genève, CH-1211, Switzerland.
  • Obis L; Department of Physics, Korea Advanced Institute of Science and Technology (KAIST), Daejeon, 34141, Republic of Korea.
  • Özbey A; Center for Axion and Precision Physics Research, Institute for Basic Science (IBS), Daejeon, 34141, Republic of Korea.
  • Özbozduman K; Centro de Astropartículas y Física de Altas Energías (CAPA), Universidad de Zaragoza, Zaragoza, 50009, Spain.
  • Pivovaroff MJ; European Organization for Nuclear Research (CERN), Genève, CH-1211, Switzerland.
Nat Commun ; 13(1): 6180, 2022 Oct 19.
Article em En | MEDLINE | ID: mdl-36261453
ABSTRACT
The CAST-CAPP axion haloscope, operating at CERN inside the CAST dipole magnet, has searched for axions in the 19.74 µeV to 22.47 µeV mass range. The detection concept follows the Sikivie haloscope principle, where Dark Matter axions convert into photons within a resonator immersed in a magnetic field. The CAST-CAPP resonator is an array of four individual rectangular cavities inserted in a strong dipole magnet, phase-matched to maximize the detection sensitivity. Here we report on the data acquired for 4124 h from 2019 to 2021. Each cavity is equipped with a fast frequency tuning mechanism of 10 MHz/ min between 4.774 GHz and 5.434 GHz. In the present work, we exclude axion-photon couplings for virialized galactic axions down to gaγγ = 8 × 10-14 GeV-1 at the 90% confidence level. The here implemented phase-matching technique also allows for future large-scale upgrades.

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Nat Commun Assunto da revista: BIOLOGIA / CIENCIA Ano de publicação: 2022 Tipo de documento: Article País de afiliação: Canadá

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Nat Commun Assunto da revista: BIOLOGIA / CIENCIA Ano de publicação: 2022 Tipo de documento: Article País de afiliação: Canadá