Pith. sign in

REVIEW

Solar X-rays as Signature for New Particles

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv astro-ph/0406203 v1 pith:7OAL2VP4 submitted 2004-06-08 astro-ph

classification astro-ph
keywords solarinsideparticlesaccumulateaxionaxionscelebratedconventional
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original 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]

Discussion (0). Continue with ORCID to comment.

Pith tools