G. N. Kichigin, “Ultimate energy of cosmic rays generated in supernova shells”, Pis'ma v Zh. Èksper. Teoret. Fiz., 87:7 (2008), 403–405; JETP Letters, 87:7 (2008), 343

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Pis'ma v Zhurnal Èksperimental'noi i Teoreticheskoi Fiziki, 2008, Volume 87, Issue 7, Pages 403–405 (Mi jetpl72)

This article is cited in 13 scientific papers (total in 13 papers)

GRAVITY, ASTROPHYSICS

Ultimate energy of cosmic rays generated in supernova shells

G. N. Kichigin

Siberian Institute of Terrestrial Magnetism, the Ionosphere, and Radiowave Propagation, Siberian Branch, Russian Academy of Sciences, Irkutsk, 664033, Russia

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Abstract: It is shown that the ultimate energy of cosmic rays accelerated in a supernova shell due to the surfing acceleration mechanism is determined by the shell radius and the interstellar magnetic field. The ultimate energy of cosmic rays accelerated in the supernova shock does not exceed 10¹⁷ eV for typical values of the interstellar magnetic field in the vicinity of a supernova and the radii of observed supernova shells.

Received: 01.02.2008
Revised: 26.02.2008

English version:
Journal of Experimental and Theoretical Physics Letters, 2008, Volume 87, Issue 7, Pages 343–344
DOI: https://doi.org/10.1134/S0021364008070011

Bibliographic databases:

Document Type: Article

PACS: 98.70.Sa

Language: Russian

Citation: G. N. Kichigin, “Ultimate energy of cosmic rays generated in supernova shells”, Pis'ma v Zh. Èksper. Teoret. Fiz., 87:7 (2008), 403–405; JETP Letters, 87:7 (2008), 343–344

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This publication is cited in the following 13 articles:

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