2000/02/07 by E. M. de Gouveia Dal Pino, A. Lazarian, Pino, E. M. de Gouveia Dal +1
Physics and Astronomy · #Astrophysics (astro-ph) #Astrophysics and Cosmic Phenomena #FOS: Physical sciences #Gamma-ray bursts and supernovae #Pulsars and Gravitational Waves Research #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0002158
Latex file, 4 pages, 2 figures, to appear in Proc. "Astrophysical Plasmas: Codes, Models & Observations", eds. J. Franco et al.; uses rmaa.cls
arxiv created 2000/02/07 · openalex publication_date 2000/02/07 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28
We 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).