English

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]

Keywords

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)