Searching for ultralight scalar dark matter with muonium and muonic atoms
arXiv:2206.10808 · doi:10.1103/PhysRevLett.131.011001
Abstract
Ultralight scalar dark matter may induce apparent oscillations of the muon mass, which may be directly probed via temporal shifts in the spectra of muonium and muonic atoms. Existing datasets and ongoing spectroscopy measurements with muonium are capable of probing scalar-muon interactions that are up to 12 orders of magnitude more stringent than astrophysical bounds. Ongoing free-fall experiments with muonium can probe forces associated with the exchange of virtual ultralight scalar bosons between muons and standard-model particles, offering up to 5 orders of magnitude improvement in sensitivity over complementary laboratory and astrophysical bounds.
14 pages, 2 figures, version accepted for publication in PRL
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Cited by in corpus (9)
- Spin-dependent exotic interactions
- Precision measurements of muonium and muonic helium hyperfine structure at J-PARC
- CP-violating axion interactions II: axions as Dark Matter
- Axion Bounds from Quantum Technology
- Unveiling Orbital Chaos: The Wild Heart of Fuzzy Dark Matter Structures
- Limits on scalar dark matter interactions with particles other than the photon via loop corrections to the scalar-photon coupling
- Is it possible to separate baryonic from dark matter within the -CDM formalism?
- Torsion Balance Experiments Enable Direct Detection of Sub-eV Dark Matter
- Muonium Spectroscopy as a Quantum Sensor for Ultralight Axion Dark Matter