Acceleration Potential and Density Profile of Secondary Plasma in the Magnetosphere of Orthogonal Pulsars

A new method for determining the accelerating potential above the polar caps of radio pulsars with an arbitrary inclination angle of the magnetic axis to the rotation axis has been proposed. The approach has been based on the concept of a vacuum gap, the height and shape of the upper boundary of which are found self-consistently together with the solution of the corresponding Poisson equation. In turn, knowledge of the accelerating potential has made it possible to determine the transverse profiles of the secondary plasma de-nsity. It has also been shown that the effect of inverse Compton scattering on the considered processes is insignificant.