Cosmic Ray Acceleration by Magnetic Traps

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dc.creatorZirakashvili, V. N.
dc.date2001-06-05
dc.date.accessioned2026-07-07T01:58:48Z
dc.date.available2026-07-07T01:58:48Z
dc.descriptionCosmic ray acceleration in turbulent interstellar medium is considered. Turbulence is treated as ensemble of moving magnetic traps. We derive equations for particle momentum distribution function that describes acceleration of particles in this case. Rate of acceleration calculated is estimated for our Galaxy and compared with ones given by other acceleration mechanisms.
dc.description4 pages, LaTeX, published in Proc. 26th ICRC
dc.identifierhttps://arxiv.org/abs/astro-ph/0106077
dc.identifierhttp://arxiv.org/abs/astro-ph/0106077
dc.identifierProc. 26th ICRC 4,439, Salt Lake City, USA, 1999
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2861
dc.subjectAstrophysics
dc.titleCosmic Ray Acceleration by Magnetic Traps
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