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Origin of Pulsed Radio Emission from Magnetars

  • Authors: Shuzhe Zeng, Alexander Philippov, James Juno, Andrei M. Beloborodov, Elena Popova

Shuzhe Zeng et al 2026 The Astrophysical Journal Letters 996 .

  • Provider: AAS Journals

Caption: Figure 4.

Dispersion of the plasma modes in the 2X1V simulation for vd/c = 0.5, ωptcool = 3000. Intensities in the Fourier space, (ω − k), are shown for electric, Ex, and magnetic, Bz, field components (panels (b)–(d) and (f)–(h), respectively), for different angles of propagation, θk = 0, π/6, π/3. The red and green dashed lines correspond to the dispersion relations of the superluminal and Alfvén modes, respectively. The white lines mark the vacuum light wave dispersion, ω = kc. For reference, panels (a) and (b) show corresponding Fourier intensities in the 1X1V simulation with the same parameters.

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