Improved bounds on ultralight scalar dark matter in the radio-frequency range
arXiv:2201.02042 · doi:10.1103/PhysRevLett.129.031301
Abstract
We present a search for fundamental constant oscillations in the range ~kHz- MHz, that may arise within models for ultralight dark matter (UDM). Using two independent, significantly upgraded optical-spectroscopy apparatus, we achieve up to 1000 greater sensitivity in the search relative to previous work. We report no observation of UDM and thus constrain respective couplings to electrons and photons within the investigated UDM particle mass range eV. The constraints significantly exceed previously set bounds, and as we show, may surpass in future experiments those provided by equivalence-principle experiments in a specific case regarding the combination of UDM couplings probed by the latter.
arXiv comment13 pages, 11 figures
References in corpus (46)
- Test of the Equivalence Principle Using a Rotating Torsion Balance
- Cosmological Relaxation of the Electroweak Scale
- A custodial symmetry for Zbb
- The Well-Tempered Neutralino
- Torsion-balance tests of the weak equivalence principle
- Searching for dilaton dark matter with atomic clocks
- The MICROSCOPE mission: first results of a space test of the Equivalence Principle
- Dark Matter Direct Detection with Accelerometers
- Can dark matter induce cosmological evolution of the fundamental constants of Nature?
- Search for ultralight scalar dark matter with atomic spectroscopy
- Short-range tests of the equivalence principle
- Searching for dark matter and variation of fundamental constants with laser and maser interferometry
- Searching for an oscillating massive scalar field as a dark matter candidate using atomic hyperfine frequency comparisons
- Precision Metrology Meets Cosmology: Improved Constraints on Ultralight Dark Matter from Atom-Cavity Frequency Comparisons
- Redefining the Axion Window
- MICROSCOPE mission: first constraints on the violation of the weak equivalence principle by a light scalar dilaton
- Revealing the Dark Matter Halo with Axion Direct Detection
- Violation of the equivalence principle from light scalar dark matter
- Search for light scalar dark matter with atomic gravitational wave detectors
- First observation with global network of optical atomic clocks aimed for a dark matter detection
- Relaxion Stars and their detection via Atomic Physics
- Sound of Dark Matter: Searching for Light Scalars with Resonant-Mass Detectors
- Stochastic fluctuations of bosonic dark matter
- Enhanced effects of variation of the fundamental constants in laser interferometers and application to dark matter detection
- Phenomenology of relaxion-Higgs mixing
- Search for variation of the fundamental constants in atomic, molecular and nuclear spectra
- Novel signatures of dark matter in laser-interferometric gravitational-wave detectors
- Direct limits for scalar field dark matter from a gravitational-wave detector
- Two clock transitions in neutral Yb for the highest sensitivity to variations of the fine-structure constant
- Searching for ultra-light dark matter with optical cavities
- Coherent relaxion dark matter
- Searching for dark matter with an unequal delay interferometer
- Searching for Scalar Dark Matter via Coupling to Fundamental Constants with Photonic, Atomic and Mechanical Oscillators
- Scalar dark matter in the radio-frequency band: atomic-spectroscopy search results
- Probing the Relaxed Relaxion at the Luminosity and Precision Frontiers
- Searching for scalar dark matter with compact mechanical resonators
- violation from , and dimension-6 Yukawa couplings -- interplay of baryogenesis, EDM and Higgs physics
- Constraining Rapidly Oscillating Scalar Dark Matter Using Dynamic Decoupling
- Searching for Earth/Solar Axion Halos
- Constraints on scalar field dark matter from co-located Michelson interferometers
- Spectral signatures of axionlike dark matter
- BBN constraints on universally-coupled ultralight scalar dark matter
- Laser Phase and Frequency Stabilization Using Atomic Coherence
- A Custodial Symmetry for Muon g-2
- Sensitivity coefficients to variation of fundamental constants
- Fast apparent oscillations of fundamental constants