Scalar-Magnetometer Search for Ultralight Dark Photon Dark Matter with a Single-Site, Two-Sensor Array: A 6-Channel DTFT Likelihood Analysis with Scalar Optically Pumped Magnetometers

Abstract

We report on a laboratory search for ultralight dark photon dark matter using a single-site, two-sensor scalar magnetometer array. The experiment employs two scalar optically pumped magnetometers (OPMs) operated in a differential configuration to suppress common-mode noise and enhance sensitivity to spatially coherent dark photon fields. We analyze 10.5 hours of continuous data with a six-channel complex data vector evaluated at the three physical frequencies of the expected dark photon signal triplet. Assuming Gaussian noise, we develop a likelihood framework to set robust, frequency-resolved upper limits on the kinetic-mixing parameter $\epsilon$, which governs the coupling between Standard Model photons and dark photons. Within the mass range $4\times 10^{-15}\mathrm{eV}\le m_{A^{\prime }}\le 3\times 10^{-14}\mathrm{eV}$, we obtain the most stringent direct laboratory limits to date on $\epsilon$, complementing existing astrophysical bounds including those inferred from observations of the Leo-T dwarf galaxy.

22 pages, 6 figures. Submitted to Physical Review D

References in corpus (3)

• Ultralight scalars as cosmological dark matter
• Bosonic super-WIMPs as keV-scale dark matter
• Earth as a transducer for dark-photon dark-matter detection

Cited by in corpus (1)

• Cavity, lumped-circuit, and spin-based detection of axion dark matter: differences and similarities