New limit on dark photon kinetic mixing in the 0.21.2μeV mass range from the Dark E-field Radio experiment

Author:

Levine Joseph1ORCID,Godfrey Benjamin1ORCID,Tyson J. Anthony1ORCID,Tripathi S. Mani1ORCID,Polin Daniel1ORCID,Aminaei Amin1ORCID,Kolner Brian H.22ORCID,Stucky Paul2ORCID

Affiliation:

1. University of California

2. University of California, Davis

Abstract

We report new limits on the kinetic mixing strength of the dark photon spanning the mass range 0.211.24μeV corresponding to a frequency span of 50–300 MHz. The Dark E-field Radio experiment is a wideband search for dark photon dark matter. In this paper we detail changes in calibration and upgrades since our proof-of-concept pilot run. Our detector employs a wide-bandwidth E-field antenna moved to multiple positions in a shielded room, a low noise amplifier, wideband analog-to-digital converter, followed by a 224-point fast Fourier transform. An optimal filter searches for signals with Q106. In nine days of integration, this system is capable of detecting dark photon signals corresponding to a kinetic mixing strength ε several orders of magnitude lower than previous limits. We find a 95% exclusion limit on ε over this mass range between 6×1015 and 6×1013, tracking the complex resonant mode structure in the shielded room. Published by the American Physical Society 2024

Funder

Brinson Foundation

U.S. Department of Energy

National Nuclear Security Administration

Publisher

American Physical Society (APS)

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