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Abstract
Cosmological observations indicate that dark matter makes up 85% of all matter in the universe yet its microscopic composition remains a mystery. Dark matter could arise from ultralight quantum fields that form macroscopic objects. Here we use the global positioning system as a ~ 50,000 km aperture dark matter detector to search for such objects in the form of domain walls. Global positioning system navigation relies on precision timing signals furnished by atomic clocks. As the Earth moves through the galactic dark matter halo, interactions with domain walls could cause a sequence of atomic clock perturbations that propagate through the satellite constellation at galactic velocities ~ 300 km s−1. Mining 16 years of archival data, we find no evidence for domain walls at our current sensitivity level. This improves the limits on certain quadratic scalar couplings of domain wall dark matter to standard model particles by several orders of magnitude.
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1 Department of Physics, University of Nevada, Reno, NV, USA
2 Department of Physics, University of Nevada, Reno, NV, USA; Nevada Geodetic Laboratory, Nevada Bureau of Mines and Geology, University of Nevada, Reno, NV, USA
3 Department of Physics and Astronomy, University of Victoria, Victoria, BC, Canada; Perimeter Institute for Theoretical Physics, Waterloo, ON, Canada
4 National Institute of Standards and Technology, Boulder, CO, USA