Pis'ma v Zhurnal Èksperimental'noi i Teoreticheskoi Fiziki
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Pis'ma v Zhurnal Èksperimental'noi i Teoreticheskoi Fiziki, 2010, Volume 92, Issue 4, Pages 226–232 (Mi jetpl1383)  
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
Full-text PDF (206 kB) Citations (10)
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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
English version:
Journal of Experimental and Theoretical Physics Letters, 2010, Volume 92, Issue 4, Pages 200–205
DOI: https://doi.org/10.1134/S0021364010160022
Bibliographic databases:
Document Type: Article
Language: Russian
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
Citation in format AMSBIB
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\pages 226--232
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\vol 92
\issue 4
\pages 200--205
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    • This publication is cited in the following 10 articles:
    Citing articles in Google Scholar: Russian citations, English citations
    Related articles in Google Scholar: Russian articles, English articles
    		Письма в Журнал экспериментальной и теоретической физики Pis'ma v Zhurnal Иksperimental'noi i Teoreticheskoi Fiziki
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