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Gieseler, U.D.J., Jones, T.W. and Kang, H. (2000) Time Dependent Cosmic-Ray Shock Acceleration with Self-Consistent Injection. Astronomy & Astrophysics, 364, 911. Preprint.
https://doi.org/10.48550/arXiv.astro-ph/0011058

has been cited by the following article:

• TITLE: Transport in Astrophysics: VIII. Cosmic Ray Acceleration in the Solar Corona

  AUTHORS: Lorenzo Zaninetti

  KEYWORDS: Cosmic Rays, Particle Acceleration

  JOURNAL NAME: International Journal of Astronomy and Astrophysics, Vol.16 No.2, May 28, 2026

  ABSTRACT: We derive the acceleration, velocity and distance of a cosmic ray (CR) due to an astrophysical electric field in the framework of special relativity. The relation between distance and time has been inverted, which allows expressing the velocity as a function of the distance. A simulation is performed for the observed spectrum of CRs adopting two distributions for them: the Maxwell Jüttner distribution and the gamma-Pareto II distribution.