Solar X-rays as Signature for New Particles
| dc.creator | Zioutas, K. | |
| dc.date | 2004-06-08 | |
| dc.date.accessioned | 2026-07-07T02:13:28Z | |
| dc.date.available | 2026-07-07T02:13:28Z | |
| dc.description | 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] | |
| dc.description | 6 pages, TeX file, Proc. Results and Perspectives in Particle Physics, La Thuile (2004) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0406203 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0406203 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/7823 | |
| dc.subject | Astrophysics | |
| dc.title | Solar X-rays as Signature for New Particles | |
| dc.type | text |