Listening for ultra-heavy dark matter with underwater acoustic detectors
Damon Cleaver, Christopher McCabe, Ciaran A. J. O'Hare

TL;DR
This paper proposes using underwater acoustic arrays to detect ultra-heavy dark matter particles through energy deposition and thermo-acoustic wave generation, providing a new detection method with extended sensitivity.
Contribution
It introduces the first detailed theoretical framework for dark matter-induced acoustic signals in seawater, including attenuation effects, and assesses the potential sensitivity of large underwater arrays.
Findings
Acoustic detection can probe dark matter masses of 0.1-10 micrograms.
Sensitivity estimates show potential to explore previously inaccessible mass ranges.
The method is applicable to existing hydrophone data and future detector designs.
Abstract
Ultra-heavy dark matter candidates evade traditional direct detection experiments due to their low particle flux. We explore the potential of large underwater acoustic arrays, originally developed for ultra-high energy neutrino detection, to detect ultra-heavy dark matter interactions. These particles deposit energy via nuclear scattering while traversing seawater, generating thermo-acoustic waves detectable by hydrophones. We present the first robust first-principles calculation of dark matter-induced acoustic waves, establishing a theoretical framework for signal modelling and sensitivity estimates. Our framework incorporates frequency-dependent attenuation effects, including viscous and chemical relaxation, not considered in previous calculations. A sensitivity analysis for a hypothetical 100 cubic kilometre hydrophone array in the Mediterranean Sea demonstrates that such an array…
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