Abstract
We propose using an optical fiber-based interferometer to search for scalar ultralight dark matter (UDM) with particle mass in the range 10-17-10-13 eV/c2 (10-3-10 Hz). Composed of a solid core and a hollow core fiber, the proposed detector would be sensitive to relative oscillations in the fibers' refractive indices due to scalar UDM-induced modulations in the fine-structure constant α. We predict that, implementing detector arrays or cryogenic cooling, the proposed optical fiber-based scalar UDM search has the potential to reach new regions of the parameter space. Such a search would be particularly well-suited to probe for a solar halo of dark matter with a sensitivity exceeding that of previous dark matter searches over the particle mass range 7×10-17-2×10-14 eV/c2.
Cite
CITATION STYLE
Manley, J., Stump, R., Petery, R., & Singh, S. (2023). Searching for scalar ultralight dark matter via refractive index changes in fibers. Physical Review D, 108(7). https://doi.org/10.1103/PhysRevD.108.075008
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