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Pis'ma v Zhurnal Èksperimental'noi i Teoreticheskoi Fiziki, 2010, Volume 92, Issue 4, Pages 226–232
(Mi jetpl1383)
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This article is cited in 10 scientific papers (total in 10 papers)
GRAVITY, ASTROPHYSICS
Fractional models of cosmic ray acceleration in the Galaxy
V. V. Uchaikin Ulyanovsk State University, Ulyanovsk, Russia
Abstract:
Possible formulations of the problem of the acceleration of cosmic rays in the interstellar galactic medium
with fractional differential equations have been considered. The applied technique has been physically justified. A Fermi result has been generalized to the case of the acceleration of particles in shock waves in the
supernovae remnants fractally distributed in the Galaxy.
Received: 15.06.2010 Revised: 14.07.2010
Citation:
V. V. Uchaikin, “Fractional models of cosmic ray acceleration in the Galaxy”, Pis'ma v Zh. Èksper. Teoret. Fiz., 92:4 (2010), 226–232; JETP Letters, 92:4 (2010), 200–205
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https://www.mathnet.ru/eng/jetpl1383 https://www.mathnet.ru/eng/jetpl/v92/i4/p226
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Abstract page: | 313 | Full-text PDF : | 134 | References: | 34 |
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