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On the acceleration of charged particles at relativistic shock frontsThe diffusive acceleration of highly relativistic particles at a shock is reconsidered. Using the same physical assumptions as Blandford and Ostriker (1978), but dropping the restriction to nonrelativistic shock velocities, the authors find approximate solutions of the particle kinetic equation by generalizing the diffusion approximation to higher order terms in the anisotropy of the particle distribution. The general solution of the transport equation on either side of the shock is constructed, which involves the solution of an eigenvalue problem. By matching the two solutions at the shock, the spectral index of the resulting power law is found by taking into account a sufficiently large number of eigenfunctions. Low-order truncation corresponds to the standard diffusion approximation and to a somewhat more general method described by Peacock (1981). In addition to the energy spectrum, the method yields the angular distribution of the particles and its spatial dependence.
Document ID
19870062179
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Kirk, J. G.
(Max-Planck-Inst. fuer Physik und Astrophysik Garching, Germany)
Schneider, P.
(Max-Planck-Institut fuer Physik und Astrophysik Garching, Germany)
Date Acquired
August 13, 2013
Publication Date
April 15, 1987
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 315
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
87A49453
Distribution Limits
Public
Copyright
Other

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