The radio telescope search for the resonant conversion of cold dark matter axions from the magnetized astrophysical sources
classification
✦ hep-ph
astro-ph.COastro-ph.HE
keywords
axionscoldconversiondarkmatterradioresonantthose
pith:ZMTX2XMM Add to your LaTeX paper
What is a Pith Number?\usepackage{pith}
\pithnumber{ZMTX2XMM}
Prints a linked pith:ZMTX2XMM badge after your title and writes the identifier into PDF metadata. Compiles on arXiv with no extra files. Learn more
read the original abstract
We study the conditions for the adiabatic resonant conversion of the cold dark matter (CDM) axions into photons in existence of the astrophysically sourced strong magnetic fields such as those in the neutron star magnetosphere. We demonstrate the possibility that the forthcoming radio telescopes such as the SKA (Square Kilometre Array) can probe those photon signals from the CDM axions.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.