Ultra-High-Energy Cosmic Ray Acceleration by Magnetic Reconnection in Newborn Pulsars

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dc.creatorPino, E. M. de Gouveia Dal
dc.creatorLazarian, A.
dc.date2000-02-07
dc.date.accessioned2026-07-07T01:52:10Z
dc.date.available2026-07-07T01:52:10Z
dc.descriptionWe here investigate the possibility that the ultra-high energy cosmic ray (UHECR) events observed above the GZK limit are mostly protons accelerated in econnection sites just above the magnetosphere of newborn millisecond pulsars which are originated by accretion induced collapse (AIC).
dc.descriptionLatex file, 4 pages, 2 figures, to appear in Proc. "Astrophysical Plasmas: Codes, Models & Observations", eds. J. Franco et al.; uses rmaa.cls
dc.identifierhttps://arxiv.org/abs/astro-ph/0002158
dc.identifierhttp://arxiv.org/abs/astro-ph/0002158
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/536
dc.subjectAstrophysics
dc.titleUltra-High-Energy Cosmic Ray Acceleration by Magnetic Reconnection in Newborn Pulsars
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