Solar X-rays as Signature for New Particles
Astrophysics
2007-05-23 v1
Abstract
Massive axions of the Kaluza-Klein type, created inside the solar core, can be gravitationally trapped by the Sun itself in orbits inside/outside the Sun, where they accumulate over cosmic times. Their radiative decay can give rise to various solar phenomena, like the celebrated solar coronal heating, which lacks a conventional explanation since its first observation in 1939. Such and other recent observations favour the existence of a halo of exotic particles near the Sun. X-ray telescopes can provide novel and important information. The underlying solar axion scenario is presented in details in ref.'s [4,15]
Cite
@article{arxiv.astro-ph/0406203,
title = {Solar X-rays as Signature for New Particles},
author = {K. Zioutas},
journal= {arXiv preprint arXiv:astro-ph/0406203},
year = {2007}
}
Comments
6 pages, TeX file, Proc. Results and Perspectives in Particle Physics, La Thuile (2004)