7 research outputs found
Solar X-rays from Axions: Rest-Mass Dependent Signatures
The spectral shape of solar X-rays is a power law. The more active the Sun
is, the less steep the distribution. This behaviour can be explained by axion
regeneration to X-rays occurring ~400km deep into the photosphere. Their
down-comptonization reproduces the measured spectral shape, pointing at axions
with rest mass m_a~17 meV/c2, without contradicting astrophysical-laboratory
limits. Directly measured soft X-ray spectra from the extremely quiet Sun
during 2009 (SphinX mission), though hitherto overlooked, fitt the axion
scenario.Comment: To appear in Proceedings of the 5th Patras Axion Workshop, Durham
200
Signatures for Solar Axions/WISPs
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.Comment: To appear in the proceedings of the 6th Patras Workshop, Zurich 5-9
July 201