Particle acceleration in axisymmetric, magnetized neutron stars

Physics

Scientific paper

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Axisymmetric Bodies, Magnetic Stars, Neutron Stars, Particle Acceleration, Magnetic Dipoles, Magnetic Fields, Polar Coordinates, Stars

Scientific paper

The potential drop in the polar cap region of a rotating, magnetized neutron star is found assuming that the magnetic field is dipolar, with the field aligned (or anti-aligned) with the rotation axis. The curvature of the field lines is of critical importance. Charge flow is assumed to be along magnetic field lines. The electric field has a maximum at radius 1.5 R and the magnitude and functional form of the current is determined.

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