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Fig. 1.

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Initial numerical setup. The pulsar, of a radius, r and angular velocity, Ω, lies at the center of the spherical box of coordinates (r,ϕ) and radius rmax. The companion, of radius rcomp, is settled at a fixed distance dcomp along the ϕ = 0 direction. Initially, the box is empty of particles. Magnetic field lines (blue and red arrows) are radial, directed outwards on one hemisphere and inwards on the other hemisphere, according to the split-monopole configuration. The plane inclination in between both hemispheres is perpendicular to the magnetic moment μ shown in green. An absorbing layer is implemented at rabsorb = 0.9rmax. The light-cylinder radius RLC is represented by the black dashed circle and the fast magnetosonic radius rfms is given by the red dashed circle.

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