A null-field continuation of force-free electrodynamics, with geodesic principal null directions, is introduced and shown to match 1D PIC simulations after loss of magnetic dominance in Alfvén wave collisions and type-changing solutions.
Monster Radiative Shocks in the Perturbed Magnetospheres of Neutron Stars,
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Magnetically driven shocks from neutron star merger remnants can reheat ejecta to nuclear statistical equilibrium, alter r-process yields, and produce observable changes in kilonova color and light curves.
Nonlinear collapse of X-modes in magnetized pair plasma near current starvation produces short bright EM pulses identified as Fast Radio Bursts.
citing papers explorer
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Continuation of Force-Free Electrodynamics upon the loss of magnetic dominance
A null-field continuation of force-free electrodynamics, with geodesic principal null directions, is introduced and shown to match 1D PIC simulations after loss of magnetic dominance in Alfvén wave collisions and type-changing solutions.
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Effects of magnetically driven shocks on nucleosynthesis and kilonovae from neutron star mergers
Magnetically driven shocks from neutron star merger remnants can reheat ejecta to nuclear statistical equilibrium, alter r-process yields, and produce observable changes in kilonova color and light curves.
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Fast Radio Bursts produced during collapse of macroscopic X-mode in magnetized pair plasma
Nonlinear collapse of X-modes in magnetized pair plasma near current starvation produces short bright EM pulses identified as Fast Radio Bursts.