Radio impulsive events in quiet solar corona and Axion Quark Nugget Dark Matter
Shuailiang Ge, Md Shahriar Rahim Siddiqui, Ludovic Van Waerbeke and, Ariel Zhitnitsky

TL;DR
This paper suggests that impulsive radio events observed in the quiet solar corona are caused by dark matter annihilation within the axion quark nugget framework, linking solar phenomena with dark matter physics.
Contribution
It proposes a novel interpretation of solar impulsive radio events as AQN annihilations, supported by matching observational data and offering testable predictions.
Findings
Radio impulsive events match AQN annihilation signatures
Predicted correlations between different frequency bands
Proposed cross-correlation with solar UV observations
Abstract
The Murchison Widefield Array (MWA) recorded \cite{Mondal-2020} impulsive radio events in the quiet solar corona at frequencies 98, 120, 132, and 160 MHz. We propose that these radio events are the direct manifestation of dark matter annihilation events within the axion quark nugget (AQN) framework. It has been argued \cite{Zhitnitsky:2017rop,Raza:2018gpb} that the AQN annihilation events in the quiet solar corona can be identified with the nanoflares conjectured by Parker \cite{Parker-1983}. We further support this claim by demonstrating that observed impulsive radio events \cite{Mondal-2020}, including their rate of appearance, their temporal and spatial distributions and their energetics, are matching the generic consequences of AQN annihilations in the quiet corona. We propose to test this idea by analyzing the correlated clustering of impulsive radio events in different frequency…
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