Inspiraling hotspots in Kerr spacetime produce precessing unwinding Stokes Q-U loops in polarization, unlike the closed loops from fixed-radius orbits.
Modeling uncertainties in X-ray reflection spectroscopy measurements II: Impactoftheradiationfromtheplungingregion,
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Polarization Signatures of Inspiraling Hotspots around Kerr Black Holes
Inspiraling hotspots in Kerr spacetime produce precessing unwinding Stokes Q-U loops in polarization, unlike the closed loops from fixed-radius orbits.