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Global Magnetohydrodynamic Simulations of Monster Shocks in Neutron Star Magnetospheres

  • Authors: Michael P. Grehan, Bart Ripperda, Andrei M. Beloborodov, Christopher Thompson, Elias R. Most

Michael P. Grehan et al 2026 The Astrophysical Journal 1005 .

  • Provider: AAS Journals

Caption: Figure 17.

The quasi-1D cylindrical monster shock for σ× ∈ [5, 10, 20, 30, 40, 50] × 103 with λ/R× = 0.034. Left: a snapshot of sigma30k at t = 4.0 RNS/c, showing the background and wave magnetic field Bϕ, the wave electric field Ez, and the radial four-velocity Γvr. A dashed black line shows the (RNS/r) scaling of the background magnetic field. Right: the maximum Lorentz factor of the cylindrical monster shock as a function ×/ωR×. The black dashed line is a linear function with a fitted slope and intercept.

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