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Scalar dark matter induced oscillation of a permanent-magnet field
Bloch, I. M. (Corresponding author) ; Budker, D.GSI*HIM* ; Flambaum, V. V. ; Samsonov, I. B. ; Sushkov, A. O. ; Tretiak, O.GSI*HIM*
2023
American Physical Society
Ridge, NY
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Please use a persistent id in citations: doi:10.1103/PhysRevD.107.075033 doi:10.15120/GSI-2023-00850
Note: The work of V. V. F. and I. B. S. was supported by the Australian Research Council Grants No. DP230101058 and DP200100150. The work of D. B. and O. T. is supported in part by the Cluster of Excellence “Precision Physics, Fundamental Interactions, and Structure of Matter” ( PRISMA+ EXC 2118/1) funded by the German Research Foundation (DFG) within the German Excellence Strategy (Project ID No. 39083149). This article is based in part upon work from COST Action COSMIC WISPers CA21106, supported by COST (European Cooperation in Science and Technology). The work of A. S. is supported in part by the NSF CAREER Grant No. PHY-2145162 and by the U.S. Department of Energy, Office of High Energy Physics, under the QuantISED program, No. FWP 100667.Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license
Contributing Institute(s):
- HIM / MAM (MAS)
Research Program(s):
- 612 - Cosmic Matter in the Laboratory (POF4-612) (POF4-612)
Experiment(s):
- External experiment at external facility/ no experiment at GSI (other)
Appears in the scientific report
2023
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