Constraints on the Acceleration of Ultra–High‐Energy Cosmic Rays in Accretion‐induced Collapse Pulsars-Reference-Cited by-同舟云学术

Constraints on the Acceleration of Ultra–High‐Energy Cosmic Rays in Accretion‐induced Collapse Pulsars

Published:2001-10-10 Issue:1 Volume:560 Page:358-364
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

de Gouveia Dal Pino Elisabete M.,Lazarian A.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/560/i=1/a=358/pdf

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3. Primordial black holes as a source of extremely high energy cosmic rays

4. Biskamp, D. 1997, in Advanced Topics in Astrophysical and Space Plasmas, ed. E. M. de Gouveia Dal Pino, A. Perat, G. A. Medina Tanco, & A. C. L. Chian (Dordrecht: Kluwer), 165

5. Two-fluid theory of collisionless magnetic reconnection

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