# Solar X-rays as Signature for New Particles

Source: [Solar X-rays as Signature for New Particles](<https://www.sota2.com/research/paper/68fa1e037a2b558e2931e7d6>)

Collection index: [llms.txt](<https://www.sota2.com/research/llms.txt>)

Data updated: 2025-10-23T13:18:09.401Z

Authors: K. Zioutas

Published: 2004-06-08T10:07:31.000Z

## 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 \[4,15\]

## Recorded benchmark results

A research result applies to its stated dataset, split, metric and evaluation configuration. Compare like-for-like settings, preserve the metric's unit and direction, and distinguish paper-reported results from independent reproduction. The best result recorded here is not a claim of exhaustive, current global coverage.

## Original sources and implementation

[Original paper](<https://arxiv.org/abs/astro-ph/0406203>)

[PDF](<https://arxiv.org/pdf/astro-ph/0406203.pdf>)