On the particle acceleration near the light surface of radio pulsars

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Abstract

The two-fluid effects on the radial outflow of relativistic electron-positron plasma are considered. It is shown that for a sufficiently large Michel magnetization parameter σ ≫ 1 and multiplication parameter λ = n/nGJ ≫ 1, the one-fluid MHD approximation remains correct in the whole region |E|

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Beskin, V. S., & Rafikov, R. R. (2000). On the particle acceleration near the light surface of radio pulsars. Monthly Notices of the Royal Astronomical Society, 313(3), 433–444. https://doi.org/10.1046/j.1365-8711.2000.03245.x

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