{"paper":{"title":"On the particle acceleration near the light surface of radio pulsars","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"2), (2) P.N.Lebedev Physical Institute, (3) Princeton University Observatory, Japan, R.R.Rafikov (3) ((1) National Astronomical Observatory, Russia, USA), V.S.Beskin (1","submitted_at":"2000-02-29T17:42:57Z","abstract_excerpt":"The two-fluid effects on the radial outflow of relativistic electron-positron plasma are considered. It is shown that for large enough Michel magnetization parameter (1969) and multiplication parameter, the one-fluid MHD approximation remains correct in the whole region where |E| < |B|. In the case in which the longitudinal electric current is smaller than the Goldreich-Julian one, the acceleration of particles is determined near the light surface where |E| = |B|.\n It is shown that, as in the previously considered cylindrical geometry (Beskin, Gurevich & Istomin 1983), almost all electromagnet"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0002525","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}