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X-ray Comptonization in an Accreting Kerr Black Hole System with a Tilted Disc and Thermal Corona: A General-Relativistic Monte Carlo Simulation. II. Polarization Signatures
Relativistic precession of the inner accretion flow is widely invoked to explain low-frequency QPOs, and the Relativistic Precession Model (RPM) predicts phase-dependent X-ray polarization. However, IXPE observations challenge simple precession and Comptonization models; for example: SwiftJ1727.8-16
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