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Electromagnetic Precursors to Binary Neutron Star Mergers: Kinetic Simulations of Magnetospheric Flaring

  • Authors: Jasmine Parsons, Anatoly Spitkovsky, Alexander Philippov, Hayk Hakobyan

Jasmine Parsons et al 2026 The Astrophysical Journal Letters 1007 .

  • Provider: AAS Journals

Caption: Figure 3.

Top: volume rendering of the current density j (compensated by r) (grayscale), overlaid with the dissipation rate j · E (compensated by r2) (red), with field lines in white showing the flux tube. Bottom: 1D profile of σ/σ0 (dark blue), n/nGJ,* (teal), Bxy/B* (red), and Bz/B* (yellow) along a line piercing through the current sheet (see light-green arrow in the top panel). The reconnecting field Bz begins to reverse when σ ∼ σ0, while the guide field Bxy remains roughly constant.

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