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Magnetar Fireballs and Short Bursts: Curved Spacetime Lensing, Quantum Electrodynamical Effects, Spectra, Polarization, and Impulse Responses

  • Authors: Zorawar Wadiasingh, Hoa Dinh Thi, Constantinos Kalapotharakos, Kun Hu, Matthew G. Baring, Alice K. Harding, George Younes, Sebastien Guillot, Andrea Sanna, Michela Negro, Jeremy D. Schnittman, Oliver J. Roberts, Eric Burns, Chin-Ping Hu, Ersin Göğüş

Zorawar Wadiasingh et al 2026 The Astrophysical Journal Supplement Series 286 .

  • Provider: AAS Journals

Caption: Figure 4.

Two-dimensional anisotropy angular distributions (for a slab where ﹩{\hat{{\boldsymbol{n}}}}_{{ \mathcal S }}\cdot \hat{{\boldsymbol{B}}}=0﹩) as a function of the cosine of the zenith angle, ﹩{\mu }_{kn}=\cos {\theta }_{kn}﹩, and the azimuthal angle ϕkB, of the intensity (Equation (38), left column), and the averaged electric field components ﹩| {\bar{{ \mathcal E }}}_{\parallel }^{2}| ﹩ (middle column) and ﹩| {\bar{{ \mathcal E }}}_{\perp }^{2}| ﹩ (right column), obtained in MAGTHOMSCATT. Rows correspond, from top to bottom, to ω/B = 0.01, 0.1, 0.25, 0.5, 2.0, and 100.0, spanning the strong field to effectively nonmagnetic scattering regimes discussed in Section 2.5. Note the varying normalization color scale for each row for HI.

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