Solar Corona Heating by the Axion Quark Nugget Dark Matter
Nayyer Raza, Ludovic van Waerbeke, Ariel Zhitnitsky

TL;DR
This paper proposes that axion quark nugget dark matter interactions could explain both the high temperature of the solar corona and the nature of dark matter, supported by numerical simulations matching observed energy levels.
Contribution
It introduces a novel model linking dark matter and solar corona heating via AQN annihilation events, supported by detailed simulations and testable predictions.
Findings
Simulations predict energy injection at the transition region altitude.
The model accounts for the corona's extreme ultraviolet excess.
Predictions can be tested by the Parker Solar Probe.
Abstract
In this work we advocate for the idea that two seemingly unrelated 80-year-old mysteries - the nature of dark matter and the high temperature of the million degree solar corona - may have resolutions that lie within the same physical framework. The current paradigm is that the corona is heated by nanoflares, which were originally proposed as miniature versions of the observed solar flares. It was recently suggested that the nanoflares could be identified as annihilation events of the nuggets from the Axion Quark Nugget (AQN) dark matter model. This model was invented as an explanation of the observed ratio , based only on cosmological and particle physics considerations. In this new paradigm, the AQN particles moving through the coronal plasma and annihilating with normal matter can lead to the drastic change of temperatures seen in the Sun's…
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