Wideband Search for Axionlike Dark Matter Using Octupolar Nuclei in a Crystal
arXiv:2410.02218 · doi:10.1103/dm9j-9pry
Abstract
Most of the matter in the Universe is in the form of dark matter, which has evaded detection so far. Ultralight axionlike particles (ALPs) are a class of dark matter candidates that produce measurable signatures in the form of oscillating violations of discrete symmetries in nuclei. We report results from a search for an oscillating parity-odd time-reversal-odd nuclear Schiff moment of Eu ions in a crystal, which leads to constraints on ALP-gluon coupling strength across a wide band spanning eight decades in ALP mass.
References in corpus (15)
- Wave Dark Matter
- Precision Metrology Meets Cosmology: Improved Constraints on Ultralight Dark Matter from Atom-Cavity Frequency Comparisons
- Search for axion-like dark matter through nuclear spin precession in electric and magnetic fields
- An even lighter QCD axion
- Experimental constraint on axion-like particle coupling over seven orders of magnitude in mass
- Search for ultralight dark matter from long-term frequency comparisons of optical and microwave atomic clocks
- Search for ultralight dark matter with spectroscopy of radio-frequency atomic transitions
- Contribution of the QCD -term to nucleon electric dipole moment
- Neutron electric dipole moment using lattice QCD simulations at the physical point
- New Limit on Axion-Like Dark Matter using Cold Neutrons
- Probing an ultralight QCD axion with electromagnetic quadratic interaction
- Searching for dark matter with the Th-229 nuclear lineshape from laser spectroscopy
- Nuclear T-violation search using octupole-deformed nuclei in a crystal
- Precision measurements of electric-field-induced frequency displacements of an ultranarrow optical transition in ions in a solid
- Comagnetometry using mirror-symmetric ions in a crystal