X-Ray Polarization Signals from Magnetars with Axion-Like-Particles
Jean-Fran\c{c}ois Fortin, Kuver Sinha

TL;DR
This paper predicts that axion-like particles from magnetars can alter X-ray polarization signals, providing a potential observational method to detect or constrain ALPs through future X-ray polarimetry.
Contribution
It introduces a novel polarization signature, the normalized Stokes parameter R, that isolates ALP effects from astrophysical backgrounds in X-ray spectra.
Findings
The parameter R factorizes into ALP-photon conversion probability and cos(2χ₀).
Predictions for O-mode polarization component depend on ALP production and conversion.
Future X-ray polarimeters can test these predictions to constrain or detect ALPs.
Abstract
Axion-like-particles (ALPs) produced in the core of a magnetar can convert to photons in the magnetosphere, giving rise to novel features in the X-ray spectrum. Since ALPs only mix with the parallel mode of the photon, the polarization of the soft and hard X-ray spectra is predicted to have an O-mode component, in addition to the mainly X-mode component given by most astrophysical models. The relative strength of the O-mode component depends on the intensity of ALPs produced in the core and the probability of conversion. We quantify our results by considering X-ray emission produced both by astrophysical processes and by ALP-photon conversion, in an uncorrelated fashion, and in different relative proportions, which we parametrize by the angle . We then define a normalized astrophysics-subtracted Stokes parameter which only acquires non-zero values in the presence of…
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