Nonlinear diffusive shock acceleration of cosmic rays: quasi-thermal and non-thermal particle distributions

Author:

Arbutina BojanORCID

Funder

Ministarstvo Prosvete, Nauke i TehnoloŠkog Razvoja

Serbian Academy of Sciences and Arts

Bulgarian Academy of Sciences

Publisher

Springer Science and Business Media LLC

Subject

General Physics and Astronomy,Fluid Flow and Transfer Processes

Reference51 articles.

1. M.S. Longair, High Energy Astrophysics. Vol. 2: Stars, the Galaxy and the Interstellar Medium, Cambridge University Press, Cambridge (1994)

2. G. Morlino, High-energy cosmic rays from supernovae, in Handbook of Supernovae. ed. by A.W. Alsabti, P. Murdin (Springer, Cham, 2016), pp.1711–1736

3. W.I. Axford, E. Leer, G. Skadron, The acceleration of cosmic rays by shock waves. in International Cosmic Ray Conference. International Cosmic Ray Conference, vol. 11, p. 132 (1977)

4. G.F. Krymskii, A regular mechanism for the acceleration of charged particles on the front of a shock wave. Akad. Nauk SSSR Dokl. 234, 1306–1308 (1977)

5. A.R. Bell, The acceleration of cosmic rays in shock fronts - I. Mon. Not. R. Astron. Soc. 182, 147–156 (1978). https://doi.org/10.1093/mnras/182.2.147

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