Instabilities nulls and sub-pulse drift in radio pulsars

Details Instabilities nulls and sub-pulse drift in radio pulsars Instabilities nulls and sub-pulse drift in radio pulsars

2011-01-31

arxiv.org/abs/1101.5918v1

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

12 pages; accepted for publication in Monthly Notices of the Royal Astronomical Society

Scientific paper

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.

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