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RESEARCH PRODUCT

Infrasonic, Acoustic and Seismic Waves Produced by the Axion Quark Nuggets

Ariel ZhitnitskyDmitry BudkerVictor Flambaum

subject

Earth and Planetary Astrophysics (astro-ph.EP)570Cosmology and Nongalactic Astrophysics (astro-ph.CO)Physics and Astronomy (miscellaneous)General MathematicsFOS: Physical sciencesGeophysics (physics.geo-ph)Physics - GeophysicsHigh Energy Physics - PhenomenologyPhysics - Atmospheric and Oceanic PhysicsHigh Energy Physics - Phenomenology (hep-ph)Chemistry (miscellaneous)ddc:570Atmospheric and Oceanic Physics (physics.ao-ph)Computer Science (miscellaneous)dark matter; axion; quark nuggetsAstrophysics - Cosmology and Nongalactic AstrophysicsAstrophysics - Earth and Planetary Astrophysics

description

We advocate an idea that the Axion Quark Nuggets (AQN) hitting the Earth can be detected by analysing the infrasound, acoustic and seismic waves which always accompany the AQN's passage in the atmosphere and underground. Our estimates for the infrasonic frequency $\nu\simeq 5$ ~Hz and overpressure $\delta p\sim 0.3 ~$Pa for relatively large size dark matter (DM) nuggets suggest that sensitivity of presently available instruments is already sufficient to detect very intense (but very rare) events today with existing technology. A study of much more frequent but less intense events requires a new type of instruments. We propose a detection strategy for a systematic study to search for such relatively weak and frequent events by using Distributed Acoustic Sensing and briefly mention other possible detection methods.

https://doi.org/10.3390/sym14030459