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Impact of Resonant Compton Scattering on Magnetar X-Ray Polarization with Quantum Electrodynamics Vacuum Resonance

  • Authors: Tu Guo, Dong Lai

Tu Guo and Dong Lai 2026 The Astrophysical Journal 1007 .

  • Provider: AAS Journals

Caption: Figure 3.

The relative O-mode and X-mode fluxes and polarization spectra for two first-order prescriptions (see Equation (28)) for the scattered-in component, compared with the unscattered case in the simplified model setup. The blue curves show the unweighted first-scattered baseline, while the orange curves apply the ﹩\exp (-{\tau }_{\alpha })﹩ attenuation factor to the scattered-in component. Other parameters are Bp = 5 × 1013 G, kT = 0.6 keV, R = 10 km, a hot spot at (θsϕs) = (65°, 30°), viewing angle θ = 25°, and ζ ≡ ξτ/β0 = 7.0 (see Equations (2) and (16)).

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