Global Magnetohydrodynamic Simulations of Monster Shocks in Neutron Star Magnetospheres
This paper presents global relativistic magnetohydrodynamic simulations demonstrating that small perturbations in neutron star magnetospheres can steepen into ultra-relativistic "monster shocks," with findings confirming analytical predictions for equatorial shocks and revealing how oblique shocks and competing wave modes can fragment shock fronts, reduce magnetization, and intermittently generate high-energy emission.