Instabilities nulls and sub-pulse drift in radio pulsars

TL;DR

This paper models neutron star polar-cap plasma states to explain pulsar phenomena like nulls and sub-pulse drift, proposing a new mechanism for sub-pulse band separation based on proton diffusion times.

Contribution

It introduces a physically consistent model of plasma state alternation above pulsar polar caps, explaining nulls and sub-pulse drift without relying on E×B drift velocity.

Findings

Proposes plasma state alternation explains pulse nulls and sub-pulse drift.

Suggests sub-pulse band separation is governed by proton diffusion time.

Provides initial comparison with observational data.

Abstract

This paper continues a previous study of neutron stars with positive polar-cap corotational charge density in which free emission of ions maintains the surface electric-field boundary condition E.B = 0. The composition of the accelerated plasma on any subset of open magnetic flux-lines above the polar cap alternates between two states; either protons or positrons and ions, of which the proton state cannot support electron-positron pair creation at higher altitudes. The two states coexist at any instant of time above different moving elements of area on the polar cap and provide a physically consistent basis for a description of pulse nulls and sub-pulse drift. In the latter case, it is shown that the band separation P3 is determined not by the ExB drift velocity, as is generally assumed, but by the diffusion time for protons produced in reverse-electron showers to reach the region of the atmosphere from which they are accelerated. An initial comparison is made with the survey of sub-pulse drift published by Weltevrede et al.