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New physics searches with highly charged ions

ORAL

Abstract

Highly charged ions (HCI) are promising candidates for novel optical clocks with applications in frequency metrology and tests of fundamental physics [1]. Typically, megakelvin-range temperatures needed to produce HCI hinder high-precision spectroscopy. To overcome this, we extract HCI from an electron beam ion trap (EBIT) and transfer them to a cryogenic linear Paul trap. There, single HCI are sympathetically cooled by laser-cooled Be+ ions down to millikelvin temperatures, thus enabling quantum logic state readout [2]. We demonstrated in this way an optical clock based on Ar13+, and determined its absolute frequency with sub-Hz uncertainty [3] against the Yb+ octupole ion clock at PTB [4]. Our techniques are readily applicable to many ions, e. g. Ca14+ [5] as well as Xe HCI [6]. Recently, we determined the isotope shift of a narrow M1 transition in stable even isotopes of Ca14+ with 150 mHz accuracy. We combine these results with available isotope-shift data of Ca+ [7] in a King plot which is sensitive to a new force that would couple electrons and neutrons [8,9]. In this way, we strengthen the constraints on the existence of such a hypothetical interaction by a factor of about ten as compared to previous studies [10]. We also estimate how far improved measurements of Ca isotope masses and isotope shifts of the Ca+ 2S1/2 - 2D5/2 transition would enhance such constraints.

Publication: [1] M. Kozlov, et al., Rev. Mod. Phys., 90, 045005 (2018)<br>[2] P. Micke, T. Leopold, S.A. King et al., Nature 578 (2020)<br>[3] S. A. King, L. J. Spiess, et al., Nature 611, 43 (2022)<br>[4] R. Lange et al., Phys. Rev. Lett. 126, 011102 (2021)<br>[5] N. Rehbehn, et al., Phys. Rev. A 103, L040801 (2021) <br>[6] N. Rehbehn, et al., Phys. Rev. Lett. 131, 161803 (2023)<br>[7] F. W. Knollmann et al., Phys. Rev. A 100, 022514 (2019)<br>[8] J. C. Berengut, et al., Phys. Rev. Lett. 120, 091801 (2018)<br>[9] J. C. Berengut, et al., Phys. Rev. Research 2 043444 (2020)<br>[10] C. Solaro et al., Phys. Rev. Lett. 125, 123003 (2020)

Presenters

  • Alexander Wilzewski

    Physikalisch-Technische Bundesanstalt

Authors

  • Alexander Wilzewski

    Physikalisch-Technische Bundesanstalt

  • Malte Wehrheim

    Physikalisch-Technische Bundesanstalt

  • Lukas J Spieß

    Physikalisch-Technische Bundesanstalt

  • Shuying Chen

    Physikalisch-Technische Bundesanstalt

  • Steven A King

    Physikalisch-Technische Bundesanstalt

  • Michael K Rosner

    Max-Planck-Institut für Kernphysik

  • Nils Rehbehn

    Max-Planck-Institut für Kernphysik

  • Anna Viatkina

    Physikalisch-Technische Bundesanstalt

  • Jan Richter

    Physikalisch-Technische Bundesanstalt

  • Andrey Surzhykov

    Physikalisch-Technische Bundesanstalt

  • Vladimir Yerokhin

    Max-Planck-Institut für Kernphysik

  • Agnese Mariotti

    Leibniz Universität Hannover

  • Elina Fuchs

    Leibniz Universität Hannover

  • Erik Benkler

    Physikalisch-Technische Bundesanstalt

  • Melina Filzinger

    Physikalisch-Technische Bundesanstalt

  • Nils Huntemann

    Physikalisch-Technische Bundesanstalt

  • Jose R Crespo Lopez-Urrutia

    Max-Planck-Institut fuer Kernphysik

  • Piet O Schmidt

    Physikalisch-Technische Bundesanstalt