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Searching for Dark Matter with an Optical Cavity and an Unequal-Delay Interferometer
Etienne Savalle1, Aurélien Hees1, Florian Frank1
1SYRTE, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, LNE, 75014 Paris, France.
Physical Review Letters
|February 19, 2021
Summary
This study searched for ultralight oscillating dark matter (DM) using a novel fiber-based optical clock experiment. No evidence of DM was found, but the experiment significantly improved constraints on DM coupling constants.
Area of Science:
- Experimental Physics
- Cosmology
- Particle Physics
Background:
- Ultralight oscillating dark matter (DM) models propose new interactions with Standard Model fields.
- Optical clocks offer high precision for detecting subtle physical variations.
Purpose of the Study:
- To experimentally search for ultralight oscillating dark matter using a novel fiber-delay-line optical clock.
- To constrain DM-Standard Model coupling constants in specific DM models.
Main Methods:
- A novel experiment comparing an optical cavity clock frequency at different times using a fiber delay line.
- Utilizing mechanical resonances of the optical cavity to enhance sensitivity.
- Analyzing experimental data for signatures of DM-induced oscillations.
Main Results:
- No evidence for ultralight oscillating dark matter in the mass range [4.1×10^{-11}, 8.3×10^{-10}] eV was found.
- Improved constraints on DM coupling constants by one order of magnitude for standard galactic DM models.
- Improved constraints by up to six orders of magnitude for relaxion DM models, especially at resonance.
Conclusions:
- The experiment sets new limits on ultralight oscillating dark matter and its interactions.
- The developed technique demonstrates sensitivity to DM couplings and can be further optimized.
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