Possible re-acceleration regions above the inner gap and pulsar gamma-ray emission

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dc.creatorHong, B. H.
dc.creatorQiao, G. J.
dc.creatorZhang, B.
dc.creatorHan, J. L.
dc.creatorXu, R. X.
dc.date1999-11-16
dc.date.accessioned2026-07-07T02:34:29Z
dc.date.available2026-07-07T02:34:29Z
dc.descriptionWe propose that the violent breakdown of the Ruderman-Sutherland type vacuum gap above the pulsar polar cap region may produce copious primary particles and make the charge density above the gap in excess of the Goldreich-Julian density. Such an excess residue of charge density may arise some re-acceleration regions above the gap due to the space-charge-limited flow mechanism. Such re-acceleration regions, if exist, may accelerate particles to carry away more spin-down energy, and may have some implications for pulsar $γ$-ray emission.
dc.description2 pages, no figures, LaTeX
dc.identifierhttps://arxiv.org/abs/astro-ph/9911307
dc.identifierhttp://arxiv.org/abs/astro-ph/9911307
dc.identifierIAU Colloquium 177: Pulsar Astronomy -- 2000 and Beyond
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15261
dc.subjectAstrophysics
dc.titlePossible re-acceleration regions above the inner gap and pulsar gamma-ray emission
dc.typetext

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