Polarization modulation from Lense-Thirring precession in X-ray binaries
Adam Ingram, Thomas Maccarone, Juri Poutanen, Henric Krawczynski

TL;DR
This paper predicts that polarization degree and angle in X-ray binaries are modulated by Lense-Thirring precession, offering a new diagnostic tool for understanding strong gravity effects near compact objects.
Contribution
It introduces a model predicting polarization signatures modulated by Lense-Thirring precession, incorporating relativistic effects and providing testable predictions for future X-ray polarimetry missions.
Findings
Polarization degree and angle are modulated at QPO frequency.
Predicted polarization modulations are detectable with future X-ray polarimeters.
Model provides a new diagnostic for strong gravity in accreting systems.
Abstract
It has long been recognised that quasi-periodic oscillations (QPOs) in the X-ray light curves of accreting black hole and neutron star binaries have the potential to be powerful diagnostics of strong field gravity. However, this potential cannot be fulfilled without a working theoretical model, which has remained elusive. Perhaps the most promising model associates the QPO with Lense-Thirring precession of the inner accretion flow, with the changes in viewing angle and Doppler boosting modulating the flux over the course of a precession cycle. Here, we consider the polarization signature of a precessing inner accretion flow. We use simple assumptions about the Comptonization process generating the emitted spectrum and take all relativistic effects into account, parallel transporting polarization vectors towards the observer along null geodesics in the Kerr metric. We find that both the…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Astrophysics and Cosmic Phenomena · Radio Astronomy Observations and Technology
