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JOURNALS // Pis'ma v Zhurnal Èksperimental'noi i Teoreticheskoi Fiziki // Archive

Pis'ma v Zh. Èksper. Teoret. Fiz., 2008 Volume 87, Issue 7, Pages 403–405 (Mi jetpl72)

This article is cited 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

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.

PACS: 98.70.Sa

Received: 01.02.2008
Revised: 26.02.2008


 English version:
Journal of Experimental and Theoretical Physics Letters, 2008, 87:7, 343–344

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