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Enßlin, T., Pfrommer, C., Miniati, F. and Subramanian, K. (2011) Cosmic Ray Transport in Galaxy Clusters: Implications for Radio Halos, Gamma-Ray Signatures, and Cool Core Heating. Astronomy & Astrophysics, 527, A99.
https://doi.org/10.1051/0004-6361/201015652

has been cited by the following article:

• TITLE: Transport in Astrophysics: VI. Ultra-High Energy Cosmic Rays

  AUTHORS: Lorenzo Zaninetti

  KEYWORDS: Cosmic Rays, Particle Diffusion, Random Walks

  JOURNAL NAME: International Journal of Astronomy and Astrophysics, Vol.14 No.1, March 29, 2024

  ABSTRACT: Two new solutions of the homogeneous diffusion equation in 1D are derived in the presence of losses and a trigonometric profile for a profile of density. A simulation for the ankle in the energy distribution of cosmic rays (CRs) is provided in the framework of the fine tuning of the involved parameters. A theoretical image for the overall diffusion of CRs in galactic coordinates is provided.