Signatures for Solar Axions/WISPs
Solar and Stellar Astrophysics
2010-11-03 v1
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.
Keywords
Cite
@article{arxiv.1011.0629,
title = {Signatures for Solar Axions/WISPs},
author = {Konstantin Zioutas and Theodoros Vafeiadis and Mary Tsagri and Yannis K Semertzidis and Thomas Papaevangelou and Theopisti Dafni and Vassilis Anastassopoulos},
journal= {arXiv preprint arXiv:1011.0629},
year = {2010}
}
Comments
To appear in the proceedings of the 6th Patras Workshop, Zurich 5-9 July 2010