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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 2.

Comparison of the equatorial monster shock to analytic predictions (B23). Left: the upstream Lorentz factor of the monster shock on the equator as a function of cylindrical radius, plotted for multiple values of σ× and λ = 2πc/ω. The black dashed line is the expected analytical scaling (Equation (12)). Right: the maximum Lorentz factor of the equatorial monster shock as a function ×/ωR×. The wave amplitude Ew (green circles), wave frequency ω (blue diamonds), and magnetization σ× (red squares) are varied. The black dashed line is a linear function with slope set by the analytical expectation (Equation (11)) and a fitted nonzero y-intercept. Details of the spherical FMS wave simulations can be found in Table 1. All values are taken on the equator, z/R× = 0. Individual linear fits where a single parameter is varied are presented in Appendix D, showing excellent agreement with the analytical expectation.

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