Signatures for Solar Axions/WISPs
Konstantin Zioutas, Theodoros Vafeiadis, Mary Tsagri, Yannis K, Semertzidis, Thomas Papaevangelou, Theopisti Dafni, Vassilis, Anastassopoulos

TL;DR
This paper explores the potential role of solar axions with a rest mass up to approximately 17 meV/c2 in explaining solar phenomena like the corona heating problem, proposing unique signatures for detection.
Contribution
It introduces atypical signatures of solar axions with specific mass range, highlighting the Sun as a source for new particle physics beyond standard models.
Findings
Proposes axion signatures with mass up to ~17 meV/c2
Suggests solar axions could explain corona heating
Highlights the Sun as a probe for new physics
Abstract
Standard solar physics cannot account for the X-ray emission and other puzzles, the most striking example being the solar corona mystery. The corona temperature rise above the non-flaring magnetized sunspots, while the photosphere just underneath becomes cooler, makes this mystery more intriguing. The paradoxical Sun is suggestive of some sort of exotic solution, axions being the (only?) choice for the missing ingredient. We present atypical axion signatures, which depict solar axions with a rest mass max ~17 meV/c2. Then, the Sun has been for decades the overlooked harbinger of new particle physics.
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Solar and Space Plasma Dynamics · Cosmology and Gravitation Theories
