Email this article Possible acceleration of cosmic rays in a rotating system: Uehling-Uhlenbeck model
- Authors: Kwang-Hua C.R.1,2
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Affiliations:
- Transfer Centre
- Distribution Centre
- Issue: Vol 123, No 5 (2016)
- Pages: 822-826
- Section: Nuclei, Particles, Fields, Gravitation, and Astrophysics
- URL: https://journals.rcsi.science/1063-7761/article/view/190979
- DOI: https://doi.org/10.1134/S1063776116130136
- ID: 190979
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Abstract
We illustrate the possible acceleration of cosmic rays passing through a kind of amplification channel (via diffusion modes of propagating plane-wave fronts) induced by a rotating system. Our analysis is mainly based on the quantum discrete kinetic model (considering a discrete Uehling-Uhlenbeck collision term), which has been used to study the propagation of plane (e.g., acoustic) waves in a system of rotating gases.
About the authors
Chu Rainer Kwang-Hua
Transfer Centre; Distribution Centre
Author for correspondence.
Email: 1559877413@qq.com
China, 2/F, No. 24, Lane 260, Section 1, Muzha Road, Taipei, Taiwan 116; Golmud Mansion, 33, Road Yingbin, Golmud, 816000
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