A self-consistent vacuum-gap model with a coordinate-dependent gap height, solved with physics-informed neural networks, gives the first quantitative non-axisymmetric accelerating potential and secondary plasma density profiles for orthogonal pulsars, and shows inverse Compton scattering is…
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Acceleration Potential and Density Profile of Secondary Plasma in the Magnetosphere of Orthogonal Pulsars
A self-consistent vacuum-gap model with a coordinate-dependent gap height, solved with physics-informed neural networks, gives the first quantitative non-axisymmetric accelerating potential and secondary plasma density profiles for orthogonal pulsars, and shows inverse Compton scattering is…