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PAMELA positron and electron spectra are reproduced by 3-dimensional cosmic-ray modeling

, , , , and . (2013)cite arxiv:1311.5575Comment: 4 pages, 3 figures. Prepared for submission to PRB : Rapid Communications. Some of the results are obtained with the DRAGON code (http://www.dragonproject.org).

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The Role of Plasma Instabilities in the Propagation of Gamma-Rays from Distant Blazars, , and . (2013)cite arxiv:1311.6752Comment: 8 pages, 5 figures; to be submitted to MNRAS.Do Cosmic Rays Heat the Early Intergalactic Medium?, , , , , and . (2017)cite arxiv:1703.09337Comment: 10 pages, 7 figures.PAMELA positron and electron spectra are reproduced by 3-dimensional cosmic-ray modeling, , , , and . (2013)cite arxiv:1311.5575Comment: 4 pages, 3 figures. Prepared for submission to PRB : Rapid Communications. Some of the results are obtained with the DRAGON code (http://www.dragonproject.org).