Search for transient ultralight dark matter signatures with networks of precision measurement devices using a Bayesian statistics method
B. M. Roberts, G. Blewitt, C. Dailey, A. Derevianko

TL;DR
This paper proposes a Bayesian analysis method to detect transient ultralight dark matter signatures using a global network of atomic clocks, including GPS satellites and ground stations, with potential to significantly improve existing constraints.
Contribution
It introduces a novel Bayesian search technique applied to atomic clock networks for detecting transient dark matter signals, demonstrating enhanced sensitivity over previous methods.
Findings
Method can surpass existing constraints by several orders of magnitude.
Simulated data tests validate the Bayesian search approach.
Applicable to various networks of precision measurement devices.
Abstract
We analyze the prospects of employing a distributed global network of precision measurement devices as a dark matter and exotic physics observatory. In particular, we consider the atomic clocks of the Global Positioning System (GPS), consisting of a constellation of 32 medium-Earth orbit satellites equipped with either Cs or Rb microwave clocks and a number of Earth-based receiver stations, some of which employ highly-stable H-maser atomic clocks. High-accuracy timing data is available for almost two decades. By analyzing the satellite and terrestrial atomic clock data, it is possible to search for transient signatures of exotic physics, such as "clumpy" dark matter and dark energy, effectively transforming the GPS constellation into a 50,000km aperture sensor array. Here we characterize the noise of the GPS satellite atomic clocks, describe the search method based on Bayesian…
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