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Some problems of pulsar physicsThe theories of particle acceleration along polar field lines are reviewed, and the total energization of the charge separated plasma is summarized, when pair creation is absent. The application of these theories and plasma supply to pulsars is discussed, with attention given to the total amount of electron-positron plasma created and its momentum distribution. Various aspects of radiation emission and transport are analyzed, based on a polar current flow model with pair creation, and the phenomenon of marching subpulses is considered. The coronation beaming and the relativistically expanding current sheet models for pulsar emission are also outlined, and the paper concludes with a brief discussion of the relation between the theories of polar flow with pair plasma and the problem of the energization of the Crab Nebula.
Document ID
19800034025
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Arons, J.
(California, University Berkeley, Calif., United States)
Date Acquired
August 10, 2013
Publication Date
December 1, 1979
Subject Category
Astrophysics
Accession Number
80A18195
Funding Number(s)
CONTRACT_GRANT: NSF AST-76-18897
CONTRACT_GRANT: NSF AST-77-23069
Distribution Limits
Public
Copyright
Other

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