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Black Hole Polarimetry: Universal Polarization of Synchrotron Radiation at the Horizon

  • Authors: Andrew Chael, Alexandru Lupsasca, George N. Wong, Zachary Gelles, Eliot Quataert

Andrew Chael et al 2026 The Astrophysical Journal Letters 1009 .

  • Provider: AAS Journals

Caption: Figure 4.

The phase ∠β2 as a function of observed impact parameter b in an equatorial monopole model viewed face-on from the south pole (θo = π). For several values of the black hole spin a* ∈ {0.1, 0.5, 0.9, 0.99}, we plot ∠β2 for models over a range of field-line angular velocities parameterized by w = ΩFH. The shaded regions show the full range of ∠β2 over 1/4 ≤ w ≤ 3/4, while the solid lines show the models with w = 1/2. Dashed lines indicate the observed ∠β2 from a flat-space monopole with w = 1/2. Solid dots at the left end of each curve show the horizon value of ∠β2 (Equation (36)) for face-on equatorial emission.

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