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Updated: Sep 27, 2025

Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
Published on: July 30, 2020
Telescope array bursts, radio pulses and axion quark nuggets
Xunyu Liang1, Ariel Zhitnitsky1
1Department of Physics and Astronomy, University of British Columbia, Vancouver, BC V6T 1Z1 Canada.
Researchers propose searching for synchronized radio signals (0.5-200 MHz) to detect dark matter (DM) annihilation events. These signals, distinct from lightning, could confirm the axion quark nugget (AQN) model
Area of Science:
- Particle Physics
- Astrophysics
- Cosmic Ray Physics
Background:
- The Telescope Array (TA) experiment has observed short bursts of air shower-like events.
- These bursts are distinct from typical single showers and correlate strongly with lightning.
- A previous study proposed these bursts as evidence of dark matter (DM) annihilation within the axion quark nugget (AQN) model.
Purpose of the Study:
- To propose a method for testing the AQN model's prediction of DM annihilation events.
- To identify specific radio signals associated with these proposed DM events.
Main Methods:
- Suggest searching for synchronized radio signals in the 0.5-200 MHz frequency band.
- These radio signals should coincide with the observed TA bursts.
- Develop criteria to discriminate AQN-induced radio pulses from conventional lightning-induced emissions.
Main Results:
- The proposed radio signals are predicted to be synchronized with TA bursts.
- A clear distinction is expected between AQN-induced radio pulses and lightning-induced radio emission.
Conclusions:
- The detection of synchronized radio signals offers a potential pathway to validate the AQN model.
- This approach provides a novel method for searching for dark matter annihilation signatures.
- Distinguishing these signals from natural phenomena like lightning is crucial for confirmation.
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