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arXiv · 1011.0629

Signatures for Solar Axions/WISPs

Konstantin Zioutas·Theodoros Vafeiadis·Mary Tsagri·Yannis K Semertzidis·Thomas Papaevangelou·Theopisti Dafni·Vassilis Anastassopoulos
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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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Konstantin Zioutas, Theodoros Vafeiadis, Mary Tsagri, Yannis K Semertzidis, Thomas Papaevangelou, Theopisti Dafni, Vassilis Anastassopoulos. 2010-11-02. Signatures for Solar Axions/WISPs. https://arxiv.org/abs/1011.0629

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