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Constraints on the Coupling between Axionlike Dark Matter and Photons Using an Antiproton Superconducting Tuned Detection Circuit in a Cryogenic Penning Trap
We constrain the coupling between axionlike particles (ALPs) and photons, measured with the superconducting resonant detection circuit of a cryogenic Penning trap. By searching the noise spectrum of our fixed-frequency resonant circuit for peaks caused by dark matter ALPs converting into photons in...
| Autores principales: | , , , , , , , , , , , , , , , , , , , |
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| Lenguaje: | eng |
| Publicado: |
2021
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| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1103/PhysRevLett.126.041301 http://cds.cern.ch/record/2751423 |
| _version_ | 1780969187813883904 |
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| author | Devlin, Jack A. Borchert, Matthias J. Erlewein, Stefan Fleck, Markus Harrington, James A. Latacz, Barbara Warncke, Jan Wursten, Elise Bohman, Matthew A. Mooser, Andreas H. Smorra, Christian Wiesinger, Markus Will, Christian Blaum, Klaus Matsuda, Yasuyuki Ospelkaus, Christian Quint, Wolfgang Walz, Jochen Yamazaki, Yasunori Ulmer, Stefan |
| author_facet | Devlin, Jack A. Borchert, Matthias J. Erlewein, Stefan Fleck, Markus Harrington, James A. Latacz, Barbara Warncke, Jan Wursten, Elise Bohman, Matthew A. Mooser, Andreas H. Smorra, Christian Wiesinger, Markus Will, Christian Blaum, Klaus Matsuda, Yasuyuki Ospelkaus, Christian Quint, Wolfgang Walz, Jochen Yamazaki, Yasunori Ulmer, Stefan |
| author_sort | Devlin, Jack A. |
| collection | CERN |
| description | We constrain the coupling between axionlike particles (ALPs) and photons, measured with the superconducting resonant detection circuit of a cryogenic Penning trap. By searching the noise spectrum of our fixed-frequency resonant circuit for peaks caused by dark matter ALPs converting into photons in the strong magnetic field of the Penning-trap magnet, we are able to constrain the coupling of ALPs with masses around 2.7906–2.7914 neV/c2 to gaγ<1×10-11 GeV-1. This is more than one order of magnitude lower than the best laboratory haloscope and approximately 5 times lower than the CERN axion solar telescope (CAST), setting limits in a mass and coupling range which is not constrained by astrophysical observations. Our approach can be extended to many other Penning-trap experiments and has the potential to provide broad limits in the low ALP mass range. |
| id | cern-2751423 |
| institution | Organización Europea para la Investigación Nuclear |
| language | eng |
| publishDate | 2021 |
| record_format | invenio |
| spelling | cern-27514232023-01-31T10:16:39Zdoi:10.1103/PhysRevLett.126.041301http://cds.cern.ch/record/2751423engDevlin, Jack A.Borchert, Matthias J.Erlewein, StefanFleck, MarkusHarrington, James A.Latacz, BarbaraWarncke, JanWursten, EliseBohman, Matthew A.Mooser, Andreas H.Smorra, ChristianWiesinger, MarkusWill, ChristianBlaum, KlausMatsuda, YasuyukiOspelkaus, ChristianQuint, WolfgangWalz, JochenYamazaki, YasunoriUlmer, StefanConstraints on the Coupling between Axionlike Dark Matter and Photons Using an Antiproton Superconducting Tuned Detection Circuit in a Cryogenic Penning Trapphysics.atom-phOther Fields of Physicshep-phParticle Physics - Phenomenologyastro-ph.COAstrophysics and AstronomyWe constrain the coupling between axionlike particles (ALPs) and photons, measured with the superconducting resonant detection circuit of a cryogenic Penning trap. By searching the noise spectrum of our fixed-frequency resonant circuit for peaks caused by dark matter ALPs converting into photons in the strong magnetic field of the Penning-trap magnet, we are able to constrain the coupling of ALPs with masses around 2.7906–2.7914 neV/c2 to gaγ<1×10-11 GeV-1. This is more than one order of magnitude lower than the best laboratory haloscope and approximately 5 times lower than the CERN axion solar telescope (CAST), setting limits in a mass and coupling range which is not constrained by astrophysical observations. Our approach can be extended to many other Penning-trap experiments and has the potential to provide broad limits in the low ALP mass range.We constrain the coupling between axionlike particles (ALPs) and photons, measured with the superconducting resonant detection circuit of a cryogenic Penning trap. By searching the noise spectrum of our fixed-frequency resonant circuit for peaks caused by dark matter ALPs converting into photons in the strong magnetic field of the Penning-trap magnet, we are able to constrain the coupling of ALPs with masses around $2.7906-2.7914\,\textrm{neV/c}^2$ to $g_{a\gamma}< 1 \times 10^{-11}\,\textrm{GeV}^{-1}$. This is more than one order of magnitude lower than the best laboratory haloscope and approximately 5 times lower than the CERN axion solar telescope (CAST), setting limits in a mass and coupling range which is not constrained by astrophysical observations. Our approach can be extended to many other Penning-trap experiments and has the potential to provide broad limits in the low ALP mass range.arXiv:2101.11290oai:cds.cern.ch:27514232021-01-27 |
| spellingShingle | physics.atom-ph Other Fields of Physics hep-ph Particle Physics - Phenomenology astro-ph.CO Astrophysics and Astronomy Devlin, Jack A. Borchert, Matthias J. Erlewein, Stefan Fleck, Markus Harrington, James A. Latacz, Barbara Warncke, Jan Wursten, Elise Bohman, Matthew A. Mooser, Andreas H. Smorra, Christian Wiesinger, Markus Will, Christian Blaum, Klaus Matsuda, Yasuyuki Ospelkaus, Christian Quint, Wolfgang Walz, Jochen Yamazaki, Yasunori Ulmer, Stefan Constraints on the Coupling between Axionlike Dark Matter and Photons Using an Antiproton Superconducting Tuned Detection Circuit in a Cryogenic Penning Trap |
| title | Constraints on the Coupling between Axionlike Dark Matter and Photons Using an Antiproton Superconducting Tuned Detection Circuit in a Cryogenic Penning Trap |
| title_full | Constraints on the Coupling between Axionlike Dark Matter and Photons Using an Antiproton Superconducting Tuned Detection Circuit in a Cryogenic Penning Trap |
| title_fullStr | Constraints on the Coupling between Axionlike Dark Matter and Photons Using an Antiproton Superconducting Tuned Detection Circuit in a Cryogenic Penning Trap |
| title_full_unstemmed | Constraints on the Coupling between Axionlike Dark Matter and Photons Using an Antiproton Superconducting Tuned Detection Circuit in a Cryogenic Penning Trap |
| title_short | Constraints on the Coupling between Axionlike Dark Matter and Photons Using an Antiproton Superconducting Tuned Detection Circuit in a Cryogenic Penning Trap |
| title_sort | constraints on the coupling between axionlike dark matter and photons using an antiproton superconducting tuned detection circuit in a cryogenic penning trap |
| topic | physics.atom-ph Other Fields of Physics hep-ph Particle Physics - Phenomenology astro-ph.CO Astrophysics and Astronomy |
| url | https://dx.doi.org/10.1103/PhysRevLett.126.041301 http://cds.cern.ch/record/2751423 |
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