Abstract

There are several networks of precision quantum sensors in existence, including networks of atomic clocks, magnetometers, and gravitational wave detectors. These networks can be re-purposed for searches of exotic physics, such as direct dark matter searches. Here we explore a detection strategy for macroscopic dark matter objects with such networks using the matched-filter technique. Such “clumpy” dark matter objects would register as transients sweeping through the network at galactic velocities. As a specific example, we consider a network of atomic clocks aboard the Global Positioning System (GPS) satellites. We apply the matched-filter technique to simulated GPS atomic clock data and study its utility and performance. The analysis and the developed methodology have a discovery reach up to three orders of magnitude above the previous GPS results and have a wide applicability to other networks of quantum sensors.

Highlights

  • Astrophysical observations on the galactic scale indicate that dark matter (DM) constitutes 85% of all matter in the universe, leaving only 15% to ordinary matter [1]

  • 3 Results 3.1 Analytic results for idealized network we turn to the general signal-to-noise ratio (SNR) (20) and determine the statistical properties of SNR for thin domain wall signals (22)

  • We incorporate a white noise reference sensor common to all the sensors. This common noise reference sensor is especially relevant to Global Positioning System (GPS) clock network, where it arises due to all clock biases reported with respect to a single reference clock

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Summary

Introduction

Astrophysical observations on the galactic scale indicate that dark matter (DM) constitutes 85% of all matter in the universe, leaving only 15% to ordinary matter [1]. Among the current DM searches, weakly interacting massive particles (WIMPs) have been the primary target with no success to date, thereby partially motivating alternative DM candidates [1]. One such alternative are ultralight fields where the DM candidate may take the form of a macroscopic object coherent over large scales. Such objects would exert gentle minute perturbations detectable by quantum sensors [2]. The particular hypothesized form of coupling of DM fields to baryonic matter determines the type of the sensor to be used in the DM search [3]

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