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D123
Searching for scalar dark maer using anprotons at BASE
Elise Wursten1,2,3, Yevgeny Stadnik4, Matthias Borchert1,5,6, Jack Devlin1,2, Stefan Erlewein1,2,3,
Markus Fleck1,7, James Harrington1,3, Julia Jäger2,3, Barbara Latacz1,2, Gilbertas Umbrazunas8, Bela
Arndt3,9, Klaus Blaum3, Yasuyuki Matsuda7, Andreas Mooser3, Christian Ospelkaus5,6, Wolfgang
Quint9, Christian Smorra1,10, Anna Soter8, Jochen Walz11, Yasunori Yamazaki1, Stefan Ulmer1,10
1RIKEN, Wako, Japan. 2CERN, Meyrin, Switzerland. 3Max-Planck-Institut für Kernphysik, Heidelberg,
Germany. 4University of Sydney, Sydney, Australia. 5Leibniz Univeristät Hannover, Hannover,
Germany. 6Physikalisch-Technische Bundesanstalt, Braunschweig, Germany. 7University of Tokyo,
Tokyo, Japan. 8ETH Zürich, Zürich, Switzerland. 9GSI-Helmholtzzentrum für Schwerionenforschung,
Darmstadt, Germany. 10Heinrich Heine University, Düsseldorf, Germany. 11Johannes Gutenberg
Universität, Mainz, Germany
Abstract
The Standard Model of Parcle Physics has known many successes, but it is known to be incomplete. It
does not provide an explanaon for the striking imbalance of maer over anmaer observed in our
Universe, nor does it account for dark maer which makes up 27% of the Universe’s energy content. To
invesgate the cause of this maer-anmaer asymmetry, a diverse physics program was set up at
CERN’s Anproton Decelerator (AD) facility to study baryonic anmaer. Comparisons of maer and
anmaer conjugates provide sensive probes for possible CPT and Lorentz violaon in Nature, tesng
two cornerstones of the Standard Model.
The Baryon Anbaryon Symmetry Experiment (BASE) at the AD searches for physics beyond the
Standard Model by comparing the fundamental properes of protons and anprotons. Using single-
parcle mul-Penning-trap techniques, we compare their charge-to-mass raos [1] and magnec
moments [2,3] with high precision. All results so far have been compable with Lorentz and CPT
invariance.
In this contribuon I will present new results constraining the coupling of scalar dark maer to
anprotons. I will review the 16-parts-per-trillion charge-to-mass rao measurement of 2022 [1] and
detail its re-interpretaon in the search for scalar-dark-maer-induced oscillang signatures.
[1] M. J. Borchert et al., Nature 601, 53 (2022).
[2] C. Smorra et al., Nature 550, 371 (2017).
[3] G. Schneider et al., Science 358, 1081 (2017).
Categories
Precision measurements