002751423 001__ 2751423
002751423 005__ 20250109043715.0
002751423 0247_ $$2DOI$$9arXiv$$a10.1103/PhysRevLett.126.041301$$qpublication
002751423 0248_ $$aoai:cds.cern.ch:2751423$$pcerncds:FULLTEXT$$pcerncds:CERN:FULLTEXT$$pcerncds:CERN
002751423 037__ $$9arXiv$$aarXiv:2101.11290$$castro-ph.CO
002751423 035__ $$9arXiv$$aoai:arXiv.org:2101.11290
002751423 035__ $$9Inspire$$aoai:inspirehep.net:1843024$$d2025-01-08T16:04:11Z$$h2025-01-09T03:00:11Z$$mmarcxml$$ttrue$$uhttps://inspirehep.net/api/oai2d
002751423 035__ $$9Inspire$$a1843024
002751423 041__ $$aeng
002751423 100__ $$aDevlin, Jack A.$$jORCID:[email protected]$$uWako, RIKEN$$uCERN$$vRIKEN, Ulmer Fundamental Symmetries Laboratory , 2-1 Hirosawa, Wako, Saitama 351-0198, Japan$$vCERN , Esplanade des Particules 1, CH-1211 Geneva 23, Switzerland
002751423 245__ $$9arXiv$$aConstraints on the Coupling between Axionlike Dark Matter and Photons Using an Antiproton Superconducting Tuned Detection Circuit in a Cryogenic Penning Trap
002751423 260__ $$c2021-01-26
002751423 269__ $$c2021-01-27
002751423 300__ $$a7 p
002751423 520__ $$9APS$$aWe 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.
002751423 520__ $$9arXiv$$aWe 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.
002751423 540__ $$3preprint$$aCC BY-NC-ND 4.0$$uhttp://creativecommons.org/licenses/by-nc-nd/4.0/
002751423 540__ $$3publication$$aCC-BY-4.0$$bAPS$$uhttps://creativecommons.org/licenses/by/4.0/
002751423 542__ $$3publication$$dauthors$$g2021
002751423 65017 $$2arXiv$$aphysics.atom-ph
002751423 65017 $$2SzGeCERN$$aOther Fields of Physics
002751423 65017 $$2arXiv$$ahep-ph
002751423 65017 $$2SzGeCERN$$aParticle Physics - Phenomenology
002751423 65017 $$2arXiv$$aastro-ph.CO
002751423 65017 $$2SzGeCERN$$aAstrophysics and Astronomy
002751423 690C_ $$aCERN
002751423 690C_ $$aARTICLE
002751423 693__ $$eCAST
002751423 700__ $$aBorchert, Matthias J.$$uWako, RIKEN$$uLeibniz U., Hannover$$uBraunschweig, Phys. Tech. Bund.$$vRIKEN, Ulmer Fundamental Symmetries Laboratory , 2-1 Hirosawa, Wako, Saitama 351-0198, Japan$$vInstitut für Quantenoptik, Leibniz Universität Hannover , Welfengarten 1, D-30167 Hannover, Germany$$vPhysikalisch-Technische Bundesanstalt , Bundesallee 100, D-38116 Braunschweig, Germany
002751423 700__ $$aErlewein, Stefan$$uWako, RIKEN$$uCERN$$vRIKEN, Ulmer Fundamental Symmetries Laboratory , 2-1 Hirosawa, Wako, Saitama 351-0198, Japan$$vCERN , Esplanade des Particules 1, CH-1211 Geneva 23, Switzerland
002751423 700__ $$aFleck, Markus$$jORCID:0000-0003-4114-1902$$uTokyo U., Komaba$$uWako, RIKEN$$vRIKEN, Ulmer Fundamental Symmetries Laboratory , 2-1 Hirosawa, Wako, Saitama 351-0198, Japan$$vGraduate School of Arts and Sciences, University of Tokyo , 3-8-1 Komaba, Tokyo 153-8902, Japan
002751423 700__ $$aHarrington, James A.$$uWako, RIKEN$$uHeidelberg, Max Planck Inst.$$vRIKEN, Ulmer Fundamental Symmetries Laboratory , 2-1 Hirosawa, Wako, Saitama 351-0198, Japan$$vMax-Planck-Institut für Kernphysik , Saupfercheckweg 1, D-69117 Heidelberg, Germany
002751423 700__ $$aLatacz, Barbara$$jORCID:0000-0003-2320-1713$$uWako, RIKEN$$vRIKEN, Ulmer Fundamental Symmetries Laboratory , 2-1 Hirosawa, Wako, Saitama 351-0198, Japan
002751423 700__ $$aWarncke, Jan$$jORCID:0000-0002-3339-7302$$uWako, RIKEN$$vRIKEN, Ulmer Fundamental Symmetries Laboratory , 2-1 Hirosawa, Wako, Saitama 351-0198, Japan
002751423 700__ $$aWursten, Elise$$uCERN$$uWako, RIKEN$$vRIKEN, Ulmer Fundamental Symmetries Laboratory , 2-1 Hirosawa, Wako, Saitama 351-0198, Japan$$vCERN , Esplanade des Particules 1, CH-1211 Geneva 23, Switzerland
002751423 700__ $$aBohman, Matthew A.$$uWako, RIKEN$$uHeidelberg, Max Planck Inst.$$vRIKEN, Ulmer Fundamental Symmetries Laboratory , 2-1 Hirosawa, Wako, Saitama 351-0198, Japan$$vMax-Planck-Institut für Kernphysik , Saupfercheckweg 1, D-69117 Heidelberg, Germany
002751423 700__ $$aMooser, Andreas H.$$uHeidelberg, Max Planck Inst.$$uWako, RIKEN$$vRIKEN, Ulmer Fundamental Symmetries Laboratory , 2-1 Hirosawa, Wako, Saitama 351-0198, Japan$$vMax-Planck-Institut für Kernphysik , Saupfercheckweg 1, D-69117 Heidelberg, Germany
002751423 700__ $$aSmorra, Christian$$uWako, RIKEN$$uMainz U., Inst. Phys.$$vRIKEN, Ulmer Fundamental Symmetries Laboratory , 2-1 Hirosawa, Wako, Saitama 351-0198, Japan$$vInstitut für Physik, Johannes Gutenberg-Universität , Staudinger Weg 7, D-55128 Mainz, Germany
002751423 700__ $$aWiesinger, Markus$$uWako, RIKEN$$uHeidelberg, Max Planck Inst.$$vMax-Planck-Institut für Kernphysik , Saupfercheckweg 1, D-69117 Heidelberg, Germany$$vRIKEN, Ulmer Fundamental Symmetries Laboratory , 2-1 Hirosawa, Wako, Saitama 351-0198, Japan
002751423 700__ $$aWill, Christian$$jORCID:0000-0003-4622-7799$$uHeidelberg, Max Planck Inst.$$vMax-Planck-Institut für Kernphysik , Saupfercheckweg 1, D-69117 Heidelberg, Germany
002751423 700__ $$aBlaum, Klaus$$uHeidelberg, Max Planck Inst.$$vMax-Planck-Institut für Kernphysik , Saupfercheckweg 1, D-69117 Heidelberg, Germany
002751423 700__ $$aMatsuda, Yasuyuki$$uTokyo U., Komaba$$vGraduate School of Arts and Sciences, University of Tokyo , 3-8-1 Komaba, Tokyo 153-8902, Japan
002751423 700__ $$aOspelkaus, Christian$$uBraunschweig, Phys. Tech. Bund.$$uLeibniz U., Hannover$$vPhysikalisch-Technische Bundesanstalt , Bundesallee 100, D-38116 Braunschweig, Germany$$vInstitut für Quantenoptik, Leibniz Universität Hannover , Welfengarten 1, D-30167 Hannover, Germany
002751423 700__ $$aQuint, Wolfgang$$uDarmstadt, GSI$$vGSI-Helmholtzzentrum für Schwerionenforschung GmbH , Planckstraße 1, D-64291 Darmstadt, Germany
002751423 700__ $$aWalz, Jochen$$uHelmholtz Inst., Mainz$$uMainz U., Inst. Phys.$$vInstitut für Physik, Johannes Gutenberg-Universität , Staudinger Weg 7, D-55128 Mainz, Germany$$vHelmholtz-Institut Mainz, Johannes Gutenberg-Universität , Staudinger Weg 18, D-55128 Mainz, Germany
002751423 700__ $$aYamazaki, Yasunori$$jORCID:0000-0001-5712-0853$$uWako, RIKEN$$vRIKEN, Ulmer Fundamental Symmetries Laboratory , 2-1 Hirosawa, Wako, Saitama 351-0198, Japan
002751423 700__ $$aUlmer, Stefan$$jORCID:0000-0002-4185-4147$$uWako, RIKEN$$vRIKEN, Ulmer Fundamental Symmetries Laboratory , 2-1 Hirosawa, Wako, Saitama 351-0198, Japan
002751423 773__ $$c041301$$mpublication$$n4$$pPhys. Rev. Lett.$$v126$$xPhysical Review Letters 126, 041301 (2021)$$y2021
002751423 8564_ $$82276960$$s973133$$uhttps://cds.cern.ch/record/2751423/files/2101.11290.pdf$$yFulltext
002751423 8564_ $$82276961$$s973133$$uhttps://cds.cern.ch/record/2751423/files/PhysRevLett.126.pdf$$yFulltext
002751423 960__ $$a13
002751423 980__ $$aARTICLE