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dc.contributor.authorCocke, W. J.
dc.date.accessioned2018-04-06T21:46:59Z
dc.date.available2018-04-06T21:46:59Z
dc.date.issued1973
dc.identifier.citationAPJ 184: 291-300 (1973)en_US
dc.identifier.urihttp://hdl.handle.net/10150/627244
dc.description.abstractThe Einstein coefficient method is used to calculate the absorption coefficient K for a steady flux of electrons undergoing acceleration in a uniform electric field. Under the approximation that the motion is ultrarelativistic, the emission frequency is low, and the emission direction is nearly parallel to the direction of motion, we find that K is negative for certain emission directions. The formalism is applied to pulsars, and it is shown that strong maser action is expected. If the emission takes place near the velocity -of -light cylinder, the computed collisional Bremsstrahlung may be strong enough to produce the recently observed high- energy Y -rays.en_US
dc.language.isoen_USen_US
dc.publisherSteward Observatory, The University of Arizona (Tucson, Arizona)en_US
dc.relation.ispartofseriesPreprints of the Steward Observatory #0055en_US
dc.relation.urlhttp://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1973ApJ...184..291C&db_key=AST&data_type=HTML&format=&high=3ed65e9cd010558en_US
dc.rightsCopyright © All Rights Reserved.en_US
dc.sourceSteward Observatory Parker Library SO QB 4 .S752 ARCHen_US
dc.subjectPulsarsen_US
dc.subjectRadio spectraen_US
dc.subjectAccelerationen_US
dc.subjectRadiationen_US
dc.titleStimulated Linear Acceleration Radiation: A Pulsar Radio Emission Mechanismen_US
dc.typetexten_US
dc.contributor.departmentUniv Arizona, Steward Observen_US
dc.description.collectioninformationThis title from the Steward Observatory Preprints collection is made available by the Steward Observatory Parker Library and the University Libraries, The University of Arizona. If you have questions about titles in this collection, please contact Parker Library librarian Betty Fridena, bfridena@as.arizona.edu.en_US
refterms.dateFOA2018-04-06T21:46:59Z


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