Infrasonic, acoustic and seismic waves produced by the Axion Quark Nuggets
arXiv:2003.07363 · doi:10.3390/sym14030459
Abstract
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 ~Hz and overpressure 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.
arXiv commentPaper is restructured, title is changed. All technical results remain identically the same
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- Rare Events Detected with a Bulk Acoustic Wave High Frequency Gravitational Wave Antenna
- The ANITA Anomalous Events and Axion Quark Nuggets
- Structure Formation Paradigm and Axion Quark Nugget dark matter model
- Dark matter searches using accelerometer-based networks
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- The Pierre Auger Exotic Events and Axion Quark Nuggets
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- Microscopic composite systems bound by strong gravity in extra dimensions as candidates for dark matter
- Ball Lightning as a profound manifestation of the Dark Matter physics
- Novel Dark Matter Signatures
- Neutron Stars as the Dark Matter detectors